WEBVTT

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Again , the areas in black are the

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total area covered , uh , which we

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obtained , uh , from the mission , and

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the areas in red are the pieces which

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we missed due to the , uh , deletion of

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the plane change and the Uh , day early

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return . This little piece down here

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was an oblique pass which we had

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planned with the hand camera , uh ,

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would have taken place on Rev 72 in

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order to get photographs of ascending ,

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which is a , a , an area of particular

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interest to the geologists . Uh , so

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you can see that we did lose some data .

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On the other hand , we did pick up some

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data that we would not have gotten , uh ,

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and I think overall the effectiveness

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of the , of the coverage was about 90%

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of what we had hoped for , uh ,

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pre-emission . I really want to express

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the Uh , thanks of the photo team , uh ,

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to the flight planners here and also to

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Ken for his operation of the cameras uh

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during the mission . I know that uh it

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was very confusing to be continually

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changing the flight plan and uh Ken

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probably We wondered what the hell we

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were doing with all these on-offs and

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so on . Uh , but , uh , uh , really , I

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think we did , uh , a very effective

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job of recovering almost all of the

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data that we had planned , uh , for the

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mission . Uh , may I have the , the

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next slide , please ? Uh , this is a

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diagram showing what the Apollo 15

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coverage was like . This is the planned

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coverage for the 16 mission , and in

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the dotted line is the planned coverage

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for the 17 mission . The only reason I

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show this is to indicate that the areas

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where we did lose data , uh ,

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unfortunately are in the areas that

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will . were not covered by 15 and will

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not be covered by 17 , so that the

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losses , although small , were real .

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the next slide . Ken ,

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during the film recovery EVA , you

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reported that the stellar camera glare

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shield was hung up on the handrail .

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I'm not 100% clear as to exactly

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what that situation was . This is the

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stellar camera glare shield , and this

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is a little cover that comes down and

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covers that when the when the mapping

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camera is retracted . Maybe you've

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discussed this with the other people

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here . At the center , but for my own

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information , I would like to know

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whether this is the cover that was hung

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up or this cover . Both of them , the

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shield at the fore and that one , this

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one , no , the first one you looked at ,

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yeah , that was sticking up . That was

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sticking up , uh huh , yeah , but the

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The tip out here was mashed against the

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handrail , mashed against the handrail

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out along here . Yeah , the rail isn't

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in this picture . The rail is not

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installed . That's right . And this lip

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was up against it and bent back out of

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the way . I see . It was not in a full

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extended position . It looked like it

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was a partial extension . Could you

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tell whether this was bent , whether

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this rail was bent , this extend rail ?

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No , but I think we have a photo that

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probably tell you that . Uh , I don't

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remember . The , the end of the shield

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was bent . Now whether that rail , no .

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He , yeah , in the next , in the next

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section of the accordion , that one was .

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Whether that rail itself was bent I

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didn't notice . The implication of

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course is that if this had happened

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early in the mission and this shield

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were bent down , we might get excessive

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light into the stellar camera and our

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background density would be would be

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higher than we expected . We might not

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see as many stars . The other

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indication of malfunction that we had ,

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of course , was in the exposure control

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on the pan camera , and that

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would indicate that the pictures away

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from the terminator may be overexposed .

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That situation is also being looked at ,

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and again we're going to talk about it

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this afternoon before we actually

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process the film . Uh , yeah , the next

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slide . This is the information which I

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have with regard to the laser altimeter

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operation . The first row across here

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is what the nominal mission would have

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been , and the second row is the actual

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results from the Apollo 16 . We had

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planned a total of 20 hours and a few

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minutes of operating time . We've got

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14.5 hours , so that we are down about

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25% in the total operating time .

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This is the total revolutions in

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longitude that we had planned 10.3 and

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we got 7.5 , so again we're down about

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25% in that regard . The

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total number of firings , 3283 and

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2106 is the actual number that was

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recorded , so we are down nearly

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30% in the total number of

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firings . Also the The number of valid

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elevation readings that we got was

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appreciably less than the total number

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of firings , so the actual mission in

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terms of altimeter observations gave us

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a little bit less than half of what we

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had actually planned . That's really

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not as serious a shortfall as it

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sounds just from the numbers because

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the readings were quite well

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distributed throughout the mission .

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The general operation that we saw on

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the altimeter , the first several revs

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were completely nominal . All of the

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elevation readings were valid . Then it

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began to fall off about 75% , 65% , and

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down to about 60% , except on the last

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data pass on RV 62 , where it was only

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about 10% effective .

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Generally what we seem to observe is

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that there would be one good shot ,

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then one bad shot , then one good , one

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bad , and then maybe several good ones

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in a row . We can talk about the

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reason for that , but that's more

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appropriately covered in the systems

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review tomorrow . The effect that it

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will have on the data is simply to give

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us Larger spacing between data points

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so far as its effect on the reduction

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of the photography is concerned ,

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that's absolutely inconsequential so

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far as its effect on the correlation

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between the tracking and gravity . And

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the profiles , it's a little bit more

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of a concern . They do have a little

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bit more smoothing to do between the

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data points that they got , but

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essentially I don't think that it

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really hurts us so far as the

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scientific return from the mission is

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concerned . I would like to say just a

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word or so about the utilization of the

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photography . It has been

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proceeding much more slowly than I had

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anticipated . In reducing the pictures

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from Apollo 15 , however , the work

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which is being done by the ACIC in St .

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Louis is indicating that the

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photography , photographic reduction

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will provide positional coordinates of

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features on the lunar surface with the

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accuracy of 10 to 12 m in position and

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in elevation . And that seems to

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coincide very well with what we had

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predicted pre-mission . So uh we are

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quite confident that uh that we're

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getting very good information from the

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pictures in that regard . The tracking

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data generally is consistent

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within an orbital pass , but we do find

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discrepancies of up to 11 kilometer

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between adjacent photographic passes ,

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so that the reduction of the

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photographs is giving us a much better

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tie between orbital passes than we get

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from the from the tracking data itself .

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Consequently , we do expect eventually

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to come up with a , an internally

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consistent coordinate system ,

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reference system , figure of the moon

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with an accuracy on the order of 12 to

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15 m . Uh , that's uh highly gratifying

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to me . So far as the pan camera

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utilization is concerned , there have

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been some map compilations done .

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The indicated precision of those is on

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the order of 3 m , which again is about

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what we had expected , but that is a

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precision and not an accuracy number

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because of the geometric problems with

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the pan camera photography . However ,

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so far as the resolution of the pan

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camera is concerned , that has held up

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to just about what we had expected , uh ,

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from 1.5 to 3 m at the

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sub-vehicle point and decreasing up to

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about 5 to 6 m at the limits of the of

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the film . So , so far as

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our indications at the moment are that

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the results from 16 are quite

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satisfactory , we do have these

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problems that we have to resolve in the

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processing of the film , and once that

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is done , we will be able to say

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exactly what we did obtain . But again ,

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I want to express the photo team's

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thanks to you , particularly Ken , for

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the time and attention that

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you gave to the camera operation and

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the results that we have obtained .

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Thanks for any questions . Could you ,

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do you have a plot of the altimetry ?

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You know , last time someone had drawn

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up a rough hand sketch of . Of the

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altimetry did anyone do that this time

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profiles ? Yes sir . No , I don't , Ken .

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I think maybe uh Shogren has one of

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those , uh , and I don't . Is he here ?

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Do you have a plot ? Yeah , I thought

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you had one . He'll show that these are

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particles that you found in the mapping

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camera that . Is that handfuls or a

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couple of shavings or I don't know

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how extensive they were . They

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were enough to concern the people

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in the processing lab . All I

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know , that's about all that I know

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about it . We're supposed to have a

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review of that this afternoon . It

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could have very serious implications ,

10:54.141 --> 10:58.109
obviously . One thing that I seem

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to recall from during the mission

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is that we had apparently more film

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left for post-TEI photography than we

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had anticipated . And what that could

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mean , of course , is that the camera

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was not passing film when we thought it

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was and things were being chewed up

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pretty badly inside . So we're going to

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have to look that over very carefully

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before we go ahead with the processing

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of the film . We expect the camera

11:28.219 --> 11:31.739
contractor to Look at the shavings and

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tell us where he thinks they came from ,

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and that may give us a better clue as

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to what they actually are . Do you have

11:38.350 --> 11:40.350
a processing schedule yet ? I guess

11:40.350 --> 11:42.406
it's all in advance to to hold until

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this afternoon , after our meeting this

11:44.628 --> 11:46.795
afternoon , assuming you're determined

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to go ahead and develop it , will it

11:48.850 --> 11:51.017
take you 3 or 4 days to process . Uh ,

11:51.017 --> 11:53.183
I think the , the anticipated schedule

11:53.183 --> 11:56.590
was to have the original film processed

11:56.590 --> 11:58.650
within this week and all of the

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duplicate copies within 4 weeks and

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distributed is the accuracy .

12:05.640 --> 12:09.119
The least count of the altimeter

12:09.119 --> 12:12.919
is 1 m . The accuracy

12:12.919 --> 12:16.820
is dependent pretty much upon

12:16.820 --> 12:18.719
the slope in the area which is

12:18.719 --> 12:22.719
illuminated and a little bit on

12:22.719 --> 12:24.497
the albedo in the area which is

12:24.497 --> 12:27.080
illuminated . In general , I think it's

12:27.080 --> 12:29.239
fair to say that the reading that we

12:29.239 --> 12:31.406
get from the altimeter will be correct

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to within 3 to 5 m .

12:37.960 --> 12:40.016
Have you figured out what to do with

12:40.016 --> 12:42.182
the pan camera for processing ? you've

12:42.182 --> 12:45.710
got a correction for the closure . I

12:45.710 --> 12:47.877
don't know what has been figured out .

12:47.877 --> 12:50.043
We had a group working on it last week

12:50.043 --> 12:52.154
and they're going to give us a report

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right after this meeting . We'll decide

12:54.377 --> 12:52.840
what to do .

13:00.010 --> 13:02.270
Uh , they think that there will be some

13:02.270 --> 13:04.492
slight loss near the terminator if they

13:04.492 --> 13:06.880
would do that . Um , in other words ,

13:06.890 --> 13:09.489
that they can handle the over explosion .

13:10.469 --> 13:13.869
But at some penalty where we have

13:13.869 --> 13:16.150
minimum rights and the question as to

13:16.150 --> 13:18.261
whether there's anything else you can

13:18.261 --> 13:20.428
say about that penalty like cutting it

13:20.428 --> 13:23.739
up . Which is not fun . The situation

13:23.739 --> 13:26.090
is really that near the terminator ,

13:26.390 --> 13:28.669
the pictures are underexposed anyhow

13:28.669 --> 13:30.669
because we can't open the slit wide

13:30.669 --> 13:32.725
enough and so on , so the camera was

13:32.725 --> 13:35.469
wide open at the terminator , but it

13:35.469 --> 13:37.780
was open wider than it should have been

13:37.780 --> 13:40.002
when we were away from the terminator ,

13:40.002 --> 13:42.113
so that the Terminator pictures are a

13:42.113 --> 13:44.113
little bit underexposed , then they

13:44.113 --> 13:46.289
become properly exposed and after that

13:46.830 --> 13:48.330
they will be overexposed .

13:50.760 --> 13:52.649
So what we would really like , of

13:52.649 --> 13:54.960
course , is a variable uh processing uh

13:54.960 --> 13:57.016
through each photo path , but that's

13:57.016 --> 13:59.127
probably not a feasible thing to even

13:59.127 --> 14:00.127
contemplate .

14:03.799 --> 14:07.570
Thanks , Fred . will be the particles

14:07.570 --> 14:09.739
and fields of the subsatellite , and I

14:09.739 --> 14:12.017
think Jim McCoy is going to cover that .

14:12.017 --> 14:15.119
Is he here ? You know , Oh , there he

14:15.119 --> 14:16.119
is .

14:26.530 --> 14:28.697
We got a mic right over there . Yeah .

14:28.697 --> 14:31.119
I don't have anything at all . Yeah ,

14:31.549 --> 14:33.716
they'll they'll project it up there in

14:33.716 --> 14:35.771
the back booth if you want to . uh ,

14:37.340 --> 14:39.451
where's where's Baldwin would , could

14:39.451 --> 14:41.340
you get this projected up there ?

14:53.809 --> 14:56.390
I guess uh Michael

15:08.280 --> 15:12.159
OK , can you hear me OK ? OK , uh .

15:13.369 --> 15:17.299
Quickly the subsatellite was

15:17.299 --> 15:21.080
deployed successfully . Our spin rate

15:21.080 --> 15:24.830
was nominal , about 58 2nd , spin

15:24.830 --> 15:27.760
period . We want 5 plus or minus a

15:27.760 --> 15:31.229
couple . Uh , the attitude was good .

15:31.919 --> 15:33.586
Uh , according to preliminary

15:33.586 --> 15:35.752
indication from the sun sensor , we're

15:35.752 --> 15:37.975
have a couple of degrees , uh , tip off

15:37.975 --> 15:39.863
from the ecliptic , which is well

15:39.863 --> 15:43.750
within the limits we needed . The

15:43.750 --> 15:45.750
operation of all of the uh

15:45.909 --> 15:48.799
electrostatic analyzers and both solid

15:48.799 --> 15:52.780
state telescopes is good . Uh , we

15:52.780 --> 15:54.880
don't seem to have the noise problem

15:55.619 --> 15:58.140
that we had on Apollo 15 and a couple

15:58.140 --> 16:01.320
of the analyzers , and we've

16:01.979 --> 16:04.146
gotten rid of our accumulator counting

16:04.146 --> 16:06.257
error that was characteristic of 15 .

16:06.419 --> 16:08.641
It's given us some problems in our data

16:08.641 --> 16:12.020
analysis now from that satellite . I'll

16:12.090 --> 16:15.830
OK , that's , The quick look uh

16:16.119 --> 16:18.969
results on our first magnetotail pass

16:19.119 --> 16:21.359
indicated again the uh presence of

16:21.359 --> 16:25.239
these rather , uh , unexpected , rather

16:25.239 --> 16:28.580
high uh fluxes of low energy protons

16:29.080 --> 16:31.960
which have also been seen now with a

16:31.960 --> 16:35.440
new IM Series I satellite

16:35.440 --> 16:39.099
experiment too . And on this

16:39.099 --> 16:41.619
magnetotail pass we appear to have the

16:41.619 --> 16:45.299
remnants of a small solar event .

16:46.330 --> 16:49.140
Uh , the form of some high energy solar

16:49.140 --> 16:51.840
cosmic ray electrons and protons around

16:52.659 --> 16:55.960
which should prove , uh , interesting

16:55.960 --> 16:57.738
for our shadow interpretation ,

16:58.010 --> 17:00.380
particularly on electric fields in the

17:00.380 --> 17:04.339
magnetotail . Beyond

17:04.339 --> 17:06.839
that , if they have those slides there ,

17:07.140 --> 17:09.859
I'd like to briefly describe some of

17:09.859 --> 17:12.099
the results we got from Apollo 15 ,

17:13.260 --> 17:15.427
which would hope to be similar to this

17:15.427 --> 17:18.800
one . I Our

17:18.800 --> 17:21.979
primary experiment was to

17:22.280 --> 17:25.619
examine . Particle shadow

17:25.619 --> 17:29.069
configurations in the magnetotail that

17:29.069 --> 17:31.291
while we're passing through this region

17:31.291 --> 17:34.709
back here where we are in the Earth's

17:34.709 --> 17:38.699
magnetic field . And uh use that to

17:38.699 --> 17:42.180
examine the uh question of openness and

17:42.180 --> 17:45.719
access through the magnetotail to the

17:45.719 --> 17:49.069
magnetic field lines and uh ultimately

17:49.069 --> 17:53.000
to the Van Allen belts . Where , uh ,

17:53.420 --> 17:55.609
theory generally holds that , uh , the

17:55.609 --> 17:57.720
Van Allen radiation must somehow come

17:57.720 --> 18:00.920
in and then be trapped and accelerated .

18:02.290 --> 18:05.510
The degree of connection back here with

18:05.510 --> 18:08.109
the interplanetary field has been in

18:08.109 --> 18:11.349
quite a bit of question . And briefly

18:11.349 --> 18:14.430
stated the Apollo 15 results indicate

18:14.430 --> 18:17.189
pretty clearly that at least most of

18:17.189 --> 18:20.670
the time at the uh latitudes where we

18:20.670 --> 18:22.910
passed through the tail , of course we

18:22.910 --> 18:26.510
only have a couple of passes . That uh

18:26.510 --> 18:29.989
these uh field lines are in fact open

18:29.989 --> 18:32.589
out here , connect directly into the

18:32.589 --> 18:35.949
interplanetary field and have direct

18:35.949 --> 18:39.109
access of uh solar cosmic ray particles .

18:41.689 --> 18:45.380
We have also observed the existence

18:45.380 --> 18:49.290
of a plasma sheet which is known to

18:49.290 --> 18:52.069
form in closer to the Earth to extend

18:52.530 --> 18:54.430
out to the moon's distance .

18:56.189 --> 18:58.349
And , uh , uh , at least a couple of

18:58.349 --> 19:01.109
occasions we have observed , uh , cross

19:01.280 --> 19:03.770
tail electric fields which are

19:04.510 --> 19:07.750
important to theoretical models , uh .

19:08.859 --> 19:12.339
Accounting for uh aurora and for

19:12.339 --> 19:14.390
acceleration of particles into the

19:14.869 --> 19:18.859
radiation belts . An unexpected

19:18.859 --> 19:22.140
observation which we

19:22.180 --> 19:25.939
found interesting was 30 KV

19:25.939 --> 19:29.020
or thereabouts protons in very large

19:29.020 --> 19:31.339
numbers which we observed quite

19:31.339 --> 19:33.780
frequently back in the magnetotail and

19:33.780 --> 19:36.599
also observed outside the magnetotail

19:36.599 --> 19:40.500
in very similar fluxes . Our first

19:40.500 --> 19:42.819
feeling was that these must also be

19:42.819 --> 19:43.239
some .

19:46.130 --> 19:49.010
Component of the solar cosmic ray

19:49.010 --> 19:51.739
proton spectrum . They're , of course ,

19:51.790 --> 19:55.790
very low energy uh . would be

19:55.790 --> 19:58.270
stopped by even the thinnest piece of

19:58.270 --> 20:02.060
material . But the uh numbers of them

20:02.319 --> 20:04.719
and the consistency of their flux

20:04.719 --> 20:08.280
densities make them uh very attractive

20:08.280 --> 20:11.000
as probably being indicative , quite

20:11.000 --> 20:13.199
indicative of uh the source that they

20:13.199 --> 20:15.640
come from and the mechanism bringing

20:15.640 --> 20:17.920
them . Uh , further examination ,

20:18.339 --> 20:21.020
however , of the locations where we see

20:21.020 --> 20:24.750
them and of the almost constant

20:24.750 --> 20:28.280
intensities that we see . Uh ,

20:28.469 --> 20:31.170
almost forced us to the conclusions

20:31.170 --> 20:34.089
that they must somehow be protons from

20:34.089 --> 20:37.630
the uh outer Van Allen belt region

20:37.630 --> 20:41.579
here . Which are somehow uh coming

20:41.579 --> 20:44.719
loose from the Earth's field and

20:45.579 --> 20:48.660
Moving outward and then getting onto

20:48.660 --> 20:50.979
the interplanetary fields and then

20:50.979 --> 20:53.900
moving out to where we see them and uh

20:53.900 --> 20:57.400
perhaps an inverse process of the

20:57.739 --> 20:58.900
postulated

21:01.959 --> 21:04.126
process where we bring uh solar cosmic

21:04.126 --> 21:06.237
particles in from the sun to populate

21:06.237 --> 21:09.589
the Van Allen belts initially . Uh ,

21:09.689 --> 21:11.849
we're anxiously waiting , getting our

21:11.849 --> 21:15.449
data , and now our computer programs

21:15.449 --> 21:17.616
that , uh , Berkeley in shape where we

21:17.616 --> 21:20.040
can examine this in detail . We've

21:20.040 --> 21:22.096
unfortunately been delayed in that .

21:24.560 --> 21:27.520
If I have the next slide , I'll show

21:27.520 --> 21:30.160
you one orbit of data from the

21:30.160 --> 21:33.900
telescopes when these uh very

21:34.310 --> 21:36.760
uh steady fluxes of protons were

21:36.760 --> 21:40.069
present . And uh during this period and

21:40.069 --> 21:43.890
actually for a period of uh A couple

21:43.890 --> 21:47.250
of orbits earlier , these fluxes were

21:47.250 --> 21:50.150
almost constant . There is some uh

21:50.449 --> 21:52.782
changing here . There , there is a very ,

21:53.290 --> 21:56.010
very slight shadowing of protons , not

21:56.010 --> 21:58.410
very much at all . This motion electron

21:58.410 --> 22:01.810
phenomena . But then these particles

22:01.810 --> 22:04.770
essentially turn off uh so somebody

22:04.770 --> 22:08.099
closed a valve . And this is

22:08.099 --> 22:10.321
characteristic of the way they behave .

22:10.321 --> 22:12.569
When they appear , they're suddenly

22:12.569 --> 22:15.579
there . And when they disappear ,

22:16.000 --> 22:19.410
they're gone just as fast . And

22:20.079 --> 22:23.609
Uh , we're very hopeful that we'll be

22:23.609 --> 22:26.410
able to make some sense out of what

22:26.410 --> 22:29.260
turns these things on and off . And

22:29.260 --> 22:31.719
determine what , where they're coming

22:31.719 --> 22:34.560
from and what the mechanism is and

22:35.180 --> 22:37.579
presumably now in the magnetosphere .

22:42.920 --> 22:45.329
OK , I think I'll just throw it open to

22:45.650 --> 22:48.520
any questions , uh , now . OK .

22:50.359 --> 22:52.192
What is the lifetime estimate of

22:55.459 --> 22:57.626
wish you hadn't brought that up . Uh ,

22:57.626 --> 23:01.000
um , will get that for us . We had been

23:01.000 --> 23:03.619
very hopeful of getting another dozen

23:03.619 --> 23:05.675
or a couple of dozen magnetic passes

23:05.675 --> 23:07.939
out of this satellite since it works so

23:07.939 --> 23:10.219
beautifully . Um

23:12.150 --> 23:14.317
I think we're gonna cover that . Chris

23:14.317 --> 23:16.650
said it was gonna stay up there forever ,

23:16.650 --> 23:19.780
so it better . Well

23:20.729 --> 23:23.869
it doesn't crash , we hope it will the

23:23.869 --> 23:26.036
world's going to come to an end pretty

23:26.036 --> 23:28.091
shortly I'm afraid . We'll see . Any

23:28.091 --> 23:30.202
other , any questions about particles

23:30.202 --> 23:32.849
and fields ? OK , let's continue on

23:32.849 --> 23:35.016
with subsatellite and get on the map .

23:35.016 --> 23:37.016
We didn't say anything about it . I

23:37.016 --> 23:38.905
assume that that our satellite is

23:38.905 --> 23:41.127
sending out good data . Is it , is it ,

23:41.127 --> 23:42.960
is batteries are charging OK and

23:42.960 --> 23:45.238
everything ? It's not running into the ,

23:45.238 --> 23:47.571
the problem that the 15 guys , uh , had ,

23:47.571 --> 23:49.738
or was that normal for the seems to be

23:49.738 --> 23:51.793
a little bit better battery charge .

23:51.793 --> 23:53.849
Yeah , the machine is working . OK ,

23:53.849 --> 23:56.016
and all the detectors are operating as

23:56.016 --> 23:59.150
far as we know , yeah . It's just that

23:59.150 --> 24:01.780
it's got a short lifetime . OK , let's

24:01.780 --> 24:03.891
see . I think Larry Sharp is going to

24:03.891 --> 24:06.290
take , uh , Uh , colon's place , right ?

24:06.750 --> 24:10.500
OK . Magnetometer . The objectives of

24:10.500 --> 24:12.278
the magnetometer experiment are

24:12.278 --> 24:14.349
essentially threefold . First is to

24:14.939 --> 24:17.050
measure and map the remnant magnetism

24:17.050 --> 24:19.780
on the lunar surface . Second is to map

24:19.780 --> 24:21.724
the electrical conductivity of the

24:21.724 --> 24:23.891
lunar interior . and finally study the

24:23.891 --> 24:25.558
various aspects of the moon's

24:25.558 --> 24:27.336
interaction with the fields and

24:27.336 --> 24:29.869
particles in its environment . The wide

24:29.869 --> 24:31.758
scope of these objectives is made

24:31.758 --> 24:33.980
possible by the geometry of orbit as it

24:33.980 --> 24:36.050
passes through three fundamentally

24:36.050 --> 24:38.479
different regions of space . For

24:38.479 --> 24:41.400
example , uh , to get the spatial

24:41.400 --> 24:43.567
variations of remnant magnetism on the

24:43.567 --> 24:45.511
lunar surface , one must be in the

24:45.511 --> 24:47.622
geomagnetic tail , where the temporal

24:47.622 --> 24:50.319
variations are almost absent in the

24:50.319 --> 24:52.597
magnetic field , very steady situation .

24:54.020 --> 24:55.699
The initial orbit of the

24:57.449 --> 24:59.650
subsatellite was somewhat lower than

24:59.650 --> 25:02.290
Apollo 15 , and the inclination about

25:02.290 --> 25:05.130
11 degrees instead of 28 . And I'd like

25:05.130 --> 25:07.819
to show you the Predictions

25:12.479 --> 25:13.479
Of the orbit .

25:16.540 --> 25:18.819
Right over there . On the backside

25:18.819 --> 25:19.760
backside of .

25:24.189 --> 25:24.640
Oops .

25:33.219 --> 25:36.880
See . Mm .

25:39.530 --> 25:41.869
OK , we've plotted days past deployment

25:42.199 --> 25:45.810
versus the parallel altitude . OK . We

25:45.810 --> 25:47.921
start out here in pretty good shape ,

25:47.921 --> 25:50.489
about 97 kilometers or 97 by 123 , I

25:50.489 --> 25:54.010
guess , and the prediction was a very

25:54.010 --> 25:57.930
rapid drop down to 30 some , back up

25:57.930 --> 26:01.310
in good shape , no real trouble until ,

26:01.369 --> 26:04.380
uh , here's the ground line . About

26:04.380 --> 26:08.119
200 days when the probability is 50/50

26:08.119 --> 26:10.920
of a crash the error bars here , you

26:10.920 --> 26:13.142
can say the probability was 1 chance in

26:13.142 --> 26:15.630
10 of a crash here and maybe 1 in 5 .

26:15.959 --> 26:17.403
We've updated this plot .

26:27.719 --> 26:31.500
Whoops . And the odds have changed

26:31.500 --> 26:34.069
considerably . This is the prediction .

26:34.270 --> 26:36.603
Notice the time scale has been expanded .

26:37.939 --> 26:40.106
Greatly these are hours now instead of

26:40.106 --> 26:42.160
days . Here was the initial

26:43.859 --> 26:46.989
initial prediction that 30 . 7

26:46.989 --> 26:49.211
kilometers and here are the actual data

26:49.211 --> 26:51.045
points . This one was taken this

26:51.045 --> 26:53.560
morning around in here , and if you can

26:53.560 --> 26:55.680
extrapolate by eye , it looks like we

26:55.680 --> 26:58.760
have about 4 days left . I guess Bill

26:58.760 --> 27:00.729
Sogren's taking 50/50 odds it will

27:00.729 --> 27:02.840
crash if anyone's in a betting mood .

27:02.959 --> 27:04.848
It's possible that we'll skim the

27:04.848 --> 27:07.420
surface and come back out , even if we

27:07.420 --> 27:09.476
make it through this one , that next

27:09.476 --> 27:11.753
dip is going to probably finish us off .

27:13.030 --> 27:15.319
Which is curiosity , uh , might be out

27:15.319 --> 27:17.541
of your field , but , uh , how come our

27:17.541 --> 27:20.520
prediction didn't match the uh the

27:20.520 --> 27:24.479
actuality , I mean we . You have a

27:24.479 --> 27:26.646
gravity experiment . We don't know the

27:26.646 --> 27:28.812
gravity field that well , and that's ,

27:28.812 --> 27:30.868
uh , the business of this , uh . Sub

27:30.868 --> 27:32.923
satellite initially to determine the

27:32.923 --> 27:35.146
gravitysphere you're you're gonna throw

27:35.146 --> 27:38.890
that though I think right . OK , and uh

27:38.890 --> 27:41.001
we've been screaming like about these

27:41.001 --> 27:43.650
pads that I know Bill Wal out here at

27:43.650 --> 27:46.209
MSC has tried to drive that point home

27:46.209 --> 27:48.369
so many times . I think we're really

27:48.369 --> 27:51.900
seeing it coming . Man , just goes to

27:51.900 --> 27:53.900
show you you can't redo 6 months of

27:53.900 --> 27:55.660
planning in 2 days . OK .

27:58.290 --> 28:00.569
any event , we have one month's worth

28:00.569 --> 28:02.680
of good data which we will add to our

28:02.680 --> 28:05.930
Apollo 15 results and to get some idea

28:05.930 --> 28:07.986
of what we're doing with this data ,

28:07.986 --> 28:10.430
I'd like to show the first slide which

28:10.430 --> 28:14.430
represents An average of 17 different

28:14.430 --> 28:18.010
orbits . Taken when the moon was in the

28:18.010 --> 28:21.829
Earth's magnetotail . And we've plotted

28:21.829 --> 28:24.500
the moon's longitude . Along the

28:24.500 --> 28:28.099
horizontal and the magnetic field in

28:28.099 --> 28:30.420
gammas along the vertical , these

28:30.420 --> 28:32.309
numbers are representative of the

28:32.309 --> 28:34.531
Earth's tail field and of course if you

28:34.531 --> 28:36.709
subtract out an average value , this

28:36.939 --> 28:40.099
residual would represent the lunar

28:40.099 --> 28:42.619
surface field and of course the big

28:42.619 --> 28:45.939
result is . Really huge

28:46.520 --> 28:48.800
magnetic dip going over the Van de

28:48.800 --> 28:50.911
Graaf crater , or a region right near

28:50.911 --> 28:53.550
the Vonder Graf crater . Also , the

28:53.930 --> 28:56.041
other initial result we got out of 15

28:56.041 --> 28:58.152
data was that most of the dips in the

28:58.152 --> 29:00.041
magnetic field seem to be clearly

29:00.041 --> 29:02.208
associated with craters lying within a

29:02.208 --> 29:04.430
few degrees of the ground track defined

29:04.430 --> 29:07.050
by the orbit subsatellite . We've

29:07.050 --> 29:10.369
numbered the 7 most obvious local

29:10.369 --> 29:12.609
minima and named 5 of them with

29:12.609 --> 29:15.599
associated craters . Initial results

29:15.599 --> 29:18.719
from Apollo 16 show the same type of

29:18.719 --> 29:20.608
structure , although we don't see

29:20.608 --> 29:22.941
anything as big as Van de Graf . We see ,

29:22.941 --> 29:24.997
we do go over Korolev again . That's

29:24.997 --> 29:27.108
where the orbits intersect when we're

29:27.108 --> 29:29.920
in the tail . And we see a few other

29:29.920 --> 29:33.319
Hertzprung and Pavlov type bumps . One

29:33.319 --> 29:35.319
is with a little tiny crater called

29:35.319 --> 29:38.890
Stein . And uh one near Mendelev .

29:41.239 --> 29:43.239
Repeat this procedure several times

29:43.239 --> 29:45.461
with different lunations , so you cover

29:45.461 --> 29:47.550
different tracks over the moon , and

29:47.550 --> 29:49.849
this allows a contour map to be made .

29:50.280 --> 29:52.002
So if I go to the next slide .

29:54.890 --> 29:56.890
Oh this shows the ground track from

29:56.890 --> 29:59.880
where we . Uh . Found the island .

29:59.959 --> 30:02.237
Here's one over Hertz Sprung , Korolev ,

30:02.939 --> 30:05.050
uh , here's Van de Graf . You can see

30:05.050 --> 30:07.050
we went right close to the northern

30:07.050 --> 30:09.217
border , Pavlov , and one over Milne .

30:09.217 --> 30:10.939
So it was a pretty good 1 to 1

30:10.939 --> 30:13.050
correspondence with , uh , with large

30:13.050 --> 30:15.719
craters . Uh , the initial .

30:17.060 --> 30:19.171
11 orbit of course is much nearer the

30:19.171 --> 30:21.227
equator . The inclination goes up to

30:21.227 --> 30:24.660
plus or -11 , so we saw one over

30:24.660 --> 30:27.209
Korolev and Stein crater is located

30:27.209 --> 30:29.320
right about here . It's not too big .

30:29.420 --> 30:31.531
The next map shows a compilation of a

30:31.531 --> 30:34.020
lot of these linear profiles . Next

30:34.020 --> 30:36.930
slide into a contour map .

30:38.709 --> 30:41.042
It's a little hard to read the contours .

30:41.739 --> 30:44.780
You can see this big black blotch here

30:44.780 --> 30:47.219
is a result of contours stacked on top

30:47.219 --> 30:49.386
of each other near this Von de graph .

30:50.000 --> 30:52.569
Anomaly . You can see the

30:54.079 --> 30:56.246
Numbers are hard to make out . You can

30:56.246 --> 30:58.468
see the structure over Korolev , a hint

30:58.468 --> 31:00.989
of some structure over Hertzprung . And

31:01.000 --> 31:03.780
uh . The Southern Sea over here is

31:03.780 --> 31:06.310
actually an enhancement sticking out of

31:06.310 --> 31:08.366
the moon , so to speak . You can see

31:08.366 --> 31:10.532
Milne shows a definite structure . The

31:10.532 --> 31:14.430
Apollo 16 results should enable

31:14.430 --> 31:16.319
us to expand this map . We'll get

31:16.319 --> 31:18.541
better resolutions throughout this area

31:18.541 --> 31:20.819
and be able to extend it along in here .

31:20.819 --> 31:23.041
We'll probably still have a gap down in

31:23.041 --> 31:22.329
this region .

31:27.359 --> 31:30.229
Oh yes . The numbers presented in the

31:30.229 --> 31:32.118
chart , if you can see them , are

31:32.118 --> 31:34.229
measured in 10th of gamma at an

31:34.229 --> 31:36.939
altitude of 100 kilometers . So for

31:36.939 --> 31:40.030
example , a good representative value

31:40.030 --> 31:41.959
is about 30 , and the zero we've

31:41.959 --> 31:44.181
arbitrarily chosen at the bottom of the

31:44.181 --> 31:46.181
Van de Graf dip , since this is the

31:46.181 --> 31:48.619
lowest value of magnetism we observed .

31:48.699 --> 31:50.421
We just call it zero and scale

31:50.421 --> 31:52.630
everything relative to it . So if

31:52.630 --> 31:54.852
you're at 100 kilometers , you'll see a

31:54.852 --> 31:57.709
3 gamma dip going over Van de Graaf on

31:57.709 --> 32:01.150
the average . Oh , we were fortunate .

32:02.300 --> 32:04.522
Uh , also , the near side of the moon ,

32:04.522 --> 32:06.829
does the gravity profile look have any

32:07.170 --> 32:09.410
can you correlate ? I've looked at the

32:09.410 --> 32:11.780
gravity profile and it doesn't seem to

32:12.160 --> 32:15.219
correlate at all uh we don't actually

32:15.219 --> 32:17.330
the laser data correlates better with

32:17.330 --> 32:19.441
you don't , there's no gravity on the

32:19.441 --> 32:21.552
backside , OK , but on the front side

32:21.552 --> 32:23.608
understand uh . It correlates pretty

32:23.608 --> 32:25.775
well with the laser data which shows a

32:25.775 --> 32:27.941
great big hole here in the backside of

32:27.941 --> 32:29.997
the moon around Fendi graph . That's

32:29.997 --> 32:29.910
where we get our big hole , but I can't

32:29.910 --> 32:32.459
see any scientific justification for

32:32.459 --> 32:34.780
connecting the two results . I will add

32:34.780 --> 32:38.469
the gamma rays secondary peak is also .

32:39.510 --> 32:41.621
I don't know what it means . It could

32:41.621 --> 32:43.677
be an alien star base or something .

32:43.689 --> 32:46.089
Anyway , the next slide shows the front

32:46.089 --> 32:49.569
side of the moon . And

32:50.750 --> 32:53.540
It's upside down . The thing to

32:53.540 --> 32:56.140
contrast is the much smoother nature of

32:56.140 --> 32:58.949
could we do a 180 on the . The slide ,

32:58.989 --> 32:59.989
please .

33:04.030 --> 33:07.790
A job . Can you hear me ? Can you turn

33:07.790 --> 33:11.680
the slide around , please ? Well , it's

33:11.680 --> 33:15.569
on a coffee break , OK , right . Anyway ,

33:15.810 --> 33:17.866
the front side of the moon is much ,

33:17.866 --> 33:20.032
much smoother than the back side . The

33:20.032 --> 33:22.869
variations are on the order of a factor

33:22.869 --> 33:25.050
of 10 smooth . We don't see very much

33:25.050 --> 33:27.280
structure at all . It's very hard to

33:27.280 --> 33:28.630
even draw contours .

33:34.920 --> 33:37.087
Can , can you sort out the differences

33:37.087 --> 33:39.031
in that and the effects of running

33:39.031 --> 33:40.976
through the , The Earth's magnetic

33:40.976 --> 33:43.329
field effects , since you're , the

33:43.329 --> 33:46.479
front side is always , Close to the

33:46.479 --> 33:50.329
earth , can you sort out Are we really

33:50.329 --> 33:53.410
measuring magnetic variations on the

33:53.410 --> 33:55.188
backside caused by being on the

33:55.188 --> 33:57.188
backside , not due to our measuring

33:57.188 --> 33:59.410
environment ? All right , there , there

33:59.410 --> 34:01.743
are scale fields , very , very constant ,

34:01.743 --> 34:03.966
uh , when you're in the . A good second

34:03.966 --> 34:06.299
when you're away from the neutral sheet ,

34:06.299 --> 34:08.632
and that's where all this data is taken .

34:08.632 --> 34:10.688
Uh , well , I guess we never got the

34:10.688 --> 34:13.069
front slide complete . OK , this is a

34:13.069 --> 34:15.668
blow up of the Vander Graaf region in

34:15.668 --> 34:18.509
attempt to pinpoint the exact source of

34:18.849 --> 34:21.049
this large anomaly . We kind of

34:21.049 --> 34:23.382
suspected it was over the crater itself .

34:25.010 --> 34:27.177
Since we had always put forth a theory

34:27.177 --> 34:29.399
that what we were actually observing in

34:29.399 --> 34:31.621
these dips was some sort of a meteorite

34:31.621 --> 34:33.732
impact that caused a rather uniformly

34:33.732 --> 34:35.954
magnetized crust to suddenly have holes

34:35.954 --> 34:38.177
in it , and we're seeing the equivalent

34:38.177 --> 34:40.399
dipole of what was left over , and this

34:40.399 --> 34:42.510
kind of shoots holes in the theory we

34:42.510 --> 34:44.677
see . This is the BX component , which

34:44.677 --> 34:46.677
is the radio component , and a plus

34:46.677 --> 34:48.843
number indicates a value sticking into

34:48.843 --> 34:52.100
the moon . So you see this Rather

34:52.100 --> 34:55.718
large Hole here magnetically in between

34:55.718 --> 34:58.979
two craters . And uh ,

35:00.239 --> 35:02.560
If you look at various models of double

35:02.560 --> 35:04.560
dipoles and stuff , it just doesn't

35:04.560 --> 35:06.879
quite fit . The other components , BY

35:06.879 --> 35:08.959
and BZ show that it can't be one of

35:08.959 --> 35:11.181
these angling dipoles from the crater .

35:13.639 --> 35:15.695
And presently , we're now conducting

35:15.695 --> 35:17.861
the same sort of studies over the rest

35:17.861 --> 35:19.917
of the anomalies to see if it checks

35:19.917 --> 35:22.139
out . I just , just yesterday completed

35:22.139 --> 35:24.195
the one over Korolev and that one is

35:24.195 --> 35:26.195
right in the middle of the crater ,

35:26.195 --> 35:28.250
which is Promising for this shocking

35:28.250 --> 35:31.909
magnetization theory . Uh ,

35:34.659 --> 35:36.548
How much do we have in the ground

35:36.548 --> 35:36.179
tracking and the military ?

35:40.780 --> 35:43.780
How much footage ? How much validity do

35:43.780 --> 35:46.002
we have in the ephemeras ? I understand

35:46.002 --> 35:48.169
there's no chance that we could be off

35:48.169 --> 35:47.760
by .

35:52.300 --> 35:55.459
Uh , but now you're talking about the

35:55.459 --> 35:56.626
finding read there .

36:00.010 --> 36:01.843
So it doesn't seem much chance .

36:03.929 --> 36:05.770
We'll get maybe one more as the

36:05.770 --> 36:07.992
subsatellite comes crashing down on the

36:07.992 --> 36:10.048
moon . The last 10 kilometers should

36:10.048 --> 36:12.270
give us a good swath of data which will

36:12.270 --> 36:14.326
give us another high resolution plot

36:14.326 --> 36:17.189
like this , but other than that we're

36:17.560 --> 36:20.550
kind of out of . OK ,

36:23.040 --> 36:24.040
OK , thank you .

36:26.989 --> 36:30.949
OK , there's the front side of the moon .

36:31.659 --> 36:34.219
OK , and our coverage from Apollo 11

36:34.219 --> 36:36.300
will extend , I believe this is the

36:36.300 --> 36:38.840
equator across here . That's .

36:42.530 --> 36:46.129
I'm sorry . OK , this is 0 degrees . OK ,

36:46.139 --> 36:48.195
we go from 0 to 90 degree east to 90

36:48.195 --> 36:49.972
west , the Terminator . This is

36:49.972 --> 36:52.028
Southern Sea region , which is about

36:52.028 --> 36:54.028
the only distinctive feature on the

36:54.028 --> 36:56.195
front side per se , and even that's on

36:56.195 --> 36:58.361
the Terminator . And again , these are

36:58.361 --> 37:00.306
relatively high values of magnetic

37:00.306 --> 37:02.361
fields sticking out of the moon . So

37:02.361 --> 37:04.528
you might say that the Southern Sea is

37:04.528 --> 37:06.750
a highly magnetized region . Notice the

37:06.750 --> 37:10.189
16 site is out of our coverage . As

37:10.189 --> 37:12.639
were all the Apollo landing sites . You

37:12.639 --> 37:15.629
have about a 3 , a 3 game of Belgium on

37:15.629 --> 37:17.796
the backside . What did you see on the

37:17.796 --> 37:19.740
front sides ? Well , most of these

37:19.740 --> 37:22.689
values are about 30 , 28 , 27 , which

37:22.689 --> 37:24.800
means they're all 3 gamma higher than

37:24.800 --> 37:27.090
that zero bendi graph . So I would say

37:27.090 --> 37:29.146
the maximum plus or minus is about a

37:29.146 --> 37:31.312
half a gamma on the whole front side .

37:32.969 --> 37:34.247
elongate parallel to ?

37:37.169 --> 37:40.020
This is a function of not having quite

37:40.020 --> 37:42.300
enough data . Instead of making

37:42.300 --> 37:44.300
physical looking contours , we drew

37:44.300 --> 37:46.189
actual contours of the data , and

37:46.189 --> 37:48.244
obviously if there's a little bit of

37:48.244 --> 37:50.244
offset from one orbit to the next ,

37:50.244 --> 37:52.133
it's going to result in elongated

37:52.133 --> 37:54.356
contours . If we fixed this up and made

37:54.356 --> 37:57.260
some intelligent looking guesses , they

37:57.260 --> 37:59.850
would be much more circular . You have

37:59.850 --> 38:03.570
a data on the Apollo 12 and the 15 and

38:03.570 --> 38:05.959
16 . Surface .

38:07.310 --> 38:09.540
Yes , with 1214 , 15 , yes ,

38:13.790 --> 38:15.957
well , you see , the surface data is ,

38:15.957 --> 38:18.179
is , uh , deals with much smaller scale

38:18.179 --> 38:20.750
size phenomena , uh , and so there's

38:20.750 --> 38:22.830
really no 1 to 1 correlation , I

38:22.830 --> 38:26.489
suppose . That the Apollo .

38:33.159 --> 38:35.326
Well , if we could be sure that over a

38:35.326 --> 38:37.215
region of 100 kilometers that the

38:37.215 --> 38:39.326
average field was 38 gamma , which no

38:39.326 --> 38:41.540
one would bet on , then we could make

38:41.540 --> 38:43.699
some interesting predictions about

38:43.699 --> 38:45.689
other places on the moon . But I

38:45.689 --> 38:47.800
suspect if you went down to Apollo 12

38:47.800 --> 38:50.100
and went 100 m away , you'd find a much

38:50.100 --> 38:52.300
different value in magnetic field . We

38:52.300 --> 38:54.578
know it's the case . Look at Apollo 14 .

38:54.578 --> 38:56.578
They went 1 kilometer and they went

38:56.578 --> 38:59.000
from 43 gamma to 103 gamma . So who's

38:59.000 --> 39:01.056
to say what's a representative value

39:01.056 --> 39:03.333
for the magnetic field in a given area .

39:04.129 --> 39:07.409
How about 50 ? Apollo 15 they saw a

39:07.409 --> 39:10.159
steady field of 6 plus or minus 4 gamma ,

39:10.209 --> 39:12.320
which is essentially zero , but there

39:12.320 --> 39:14.290
again , you know , behind the next

39:14.290 --> 39:16.070
boulder probably be 100 gamma .

39:19.070 --> 39:21.126
And the results in 16 I thought were

39:21.126 --> 39:23.292
tremendous , tremendous gradients they

39:23.292 --> 39:25.348
got between one place and another at

39:25.348 --> 39:28.709
313 . Uh , Gamma Field really surprised

39:28.709 --> 39:32.159
me as far as . Get value at large .

39:34.909 --> 39:37.669
Yes , have you seen any distinctive

39:37.669 --> 39:40.050
features about , uh , the , uh ,

39:40.060 --> 39:42.116
correlate which might make you think

39:42.116 --> 39:44.469
that it was , uh , say a hot spot that

39:44.469 --> 39:48.250
had been , uh , near the surface

39:48.250 --> 39:50.560
and was That

39:52.560 --> 39:54.959
Soil covering which would change the

39:54.959 --> 39:57.800
surface temperature . The change .

39:59.929 --> 40:02.250
No , I'm not a , not a geologist type ,

40:02.489 --> 40:05.560
uh . Well I already on about 17 .

40:06.649 --> 40:10.330
Uh That would change .

40:12.689 --> 40:14.633
It would seem to me that the , the

40:14.633 --> 40:16.800
younger a crater was , the more chance

40:16.800 --> 40:18.911
it would have to produce a good clean

40:18.911 --> 40:22.179
cut signature . On the uh magnetic

40:22.179 --> 40:25.070
field data . I mean , for example , Van

40:25.070 --> 40:27.014
de Graf itself looks like a fairly

40:27.014 --> 40:29.237
young crater because there's no there's

40:29.237 --> 40:31.126
very few secondary craters in the

40:31.126 --> 40:33.459
bottom of it , so it looks fairly young ,

40:33.459 --> 40:35.626
whereas uh Things like Kurtzprung seem

40:35.626 --> 40:37.792
to be very old . They're well blotched

40:37.792 --> 40:39.181
with secondary graders .

40:43.330 --> 40:45.949
Center of the anomaly . Uh , it's 80

40:45.949 --> 40:49.040
kilometers from the northern rim . So

40:49.040 --> 40:51.096
from the center of Andy graph , it's

40:51.096 --> 40:53.540
about 130 , 140 kilometers .

40:57.540 --> 41:00.189
Any other questions ? OK , thank you ,

41:00.250 --> 41:03.870
Larry , and Yeah , got a question ? No .

41:04.889 --> 41:07.056
Last subject will be the transponder .

41:35.659 --> 41:37.580
Uh , this is a , uh , gravity

41:37.580 --> 41:40.340
experiment , and , uh , we monitor the

41:40.340 --> 41:43.280
gravity by just monitoring the , uh ,

41:43.489 --> 41:46.780
velocity of the spacecraft or the limb

41:46.780 --> 41:50.639
or the , uh , Sub-satellite . Of course ,

41:50.719 --> 41:52.941
on uh this particular mission , we lost

41:52.941 --> 41:55.199
our LEM data on impact cause it started

41:55.199 --> 41:58.120
tumbling . And so that data was lost .

41:58.159 --> 42:02.129
We do have , how have the uh CSM in the

42:02.129 --> 42:04.909
low altitude orbit , which is Uh ,

42:05.729 --> 42:07.062
very interesting data .

42:14.270 --> 42:15.550
These parts on right .

42:27.879 --> 42:31.639
Here's the orbital track and hopefully

42:31.639 --> 42:35.239
I can get this aligned . Uh ,

42:35.600 --> 42:38.639
not like that . This profile just below

42:38.639 --> 42:42.350
it is the Gravity

42:42.350 --> 42:44.709
anomaly that was detected . This line

42:44.709 --> 42:47.189
right here represents zero

42:48.370 --> 42:50.592
gravity central isostatic equilibrium ,

42:50.750 --> 42:52.750
and anything below it , of course ,

42:52.750 --> 42:56.229
that'd be negative gravity deviations .

42:57.070 --> 42:58.903
Here we are at Ptolemais going .

43:00.310 --> 43:02.366
Essentially over the center with the

43:02.366 --> 43:04.366
track , and we can see the large uh

43:04.366 --> 43:06.477
negative anomaly again and almost 100

43:06.477 --> 43:10.179
mgs . Uh . Uh , here we see , uh ,

43:10.459 --> 43:12.737
some highland material where we have a ,

43:12.737 --> 43:14.848
a positive , then we drop down into a

43:15.090 --> 43:17.679
relative low in between these two old

43:17.679 --> 43:19.830
craters , Hipparchus and Alvitgnius ,

43:20.620 --> 43:23.500
and then a , a high in here . Uh , at

43:23.500 --> 43:25.722
this point , there's a Descartes , uh .

43:26.310 --> 43:28.421
The landing site , and we're actually

43:28.421 --> 43:30.588
about a 50 mg negative anomaly in that

43:30.588 --> 43:32.489
region . Uh , there's some nice

43:32.489 --> 43:35.209
correlations here with the , uh , laser

43:35.209 --> 43:37.431
altimetry measurements . I'll show them

43:37.431 --> 43:39.889
in the next , uh , profile . But this

43:39.889 --> 43:41.889
is continuous . I've just taken one

43:41.889 --> 43:44.111
small section here . We have this thing

43:44.111 --> 43:46.889
from Uh , limb to limb , so about 110

43:46.889 --> 43:50.770
longitude plus to 100 110 minus . And

43:50.770 --> 43:54.659
uh , Essentially , 3 revs , and

43:54.659 --> 43:57.449
rev 3 through rev . Uh ,

43:58.389 --> 44:01.550
11 , that's 8 revs , 8 revs of data

44:01.550 --> 44:03.669
that are pretty good and then they

44:03.669 --> 44:06.629
started their . Station keeping and uh

44:06.760 --> 44:08.927
the data kind of got garbaged up a lot

44:08.927 --> 44:11.149
with all the maneuvering was going on .

44:14.800 --> 44:17.022
Uh , I don't even point out one kind of

44:17.022 --> 44:19.610
interesting thing here . Uh , notice

44:19.610 --> 44:21.499
that , uh , Ptolemais here has an

44:21.499 --> 44:23.721
anomaly much , much lower than Nubium .

44:23.721 --> 44:25.888
Although Nubium , which is this region

44:25.888 --> 44:28.110
right in here , this Maran Nubium right

44:28.110 --> 44:31.010
in here , uh , It's still about -50 mg .

44:41.949 --> 44:44.129
Here's an altimeter profile .

44:45.780 --> 44:48.780
And uh going right to the Nubian

44:49.090 --> 44:51.146
Ptolemais region again , we see that

44:51.300 --> 44:54.090
Nubium uh elevation here is , uh , some ,

44:54.500 --> 44:57.209
by the way , the scale here is uh 2

44:57.209 --> 44:59.979
kilometers per heavy line . So we've

44:59.979 --> 45:02.090
dropped down here almost 2 kilometers

45:02.090 --> 45:04.035
from the floor of Ptolemais to the

45:04.035 --> 45:06.139
floor of Nubium . Yet the uh

45:07.850 --> 45:10.017
gravity anomaly is just the opposite ,

45:10.017 --> 45:12.530
that Ptolemais is some 50 milligaus

45:12.530 --> 45:16.229
lower than the Nubian region . And

45:16.229 --> 45:18.340
another interesting point is , Fred ,

45:18.340 --> 45:21.370
on these ACIC maps , Nubium is shown 1

45:21.370 --> 45:25.310
kilometer higher than Ptolemais . And

45:25.310 --> 45:27.500
here we are 2 kilometers lower , so

45:27.500 --> 45:29.389
we're talking about a 3 kilometer

45:29.389 --> 45:31.444
discrepancy in just that little area

45:31.444 --> 45:33.611
right there . So I think some of these

45:33.611 --> 45:35.833
guys were talking about the right thing

45:35.833 --> 45:35.149
when they said we really didn't know

45:35.149 --> 45:38.750
the altitudes too well . I , I think

45:38.750 --> 45:40.861
that shows up quite dramatically when

45:40.861 --> 45:44.050
you look at the . At the low sun angle .

45:45.090 --> 45:47.201
View as you approach the Terminator ,

45:47.201 --> 45:49.330
the things that were in Nubum didn't

45:49.330 --> 45:52.689
show up until significantly after we

45:52.689 --> 45:54.745
anticipated . We missed our times on

45:54.745 --> 45:56.800
those things a great deal , and that

45:56.800 --> 45:58.633
could only be called by having a

45:58.633 --> 46:00.745
discrepancy in our relative heights .

46:00.745 --> 46:03.022
Yeah , this is not just this is Rev 28 .

46:03.022 --> 46:05.610
We've looked at there are 5 real good

46:06.169 --> 46:08.169
tracking laser tracking passes over

46:08.169 --> 46:10.336
this region , and we've looked at 3 of

46:10.336 --> 46:12.058
them , and all 3 show the same

46:12.058 --> 46:14.280
consistency of the drop there . Another

46:14.280 --> 46:16.391
interesting thing here , Procolarum ,

46:16.550 --> 46:19.110
Franklotati , Fecunditatus are all seem

46:19.110 --> 46:21.909
to be about on the same level . Smithyi

46:21.909 --> 46:24.739
again being a low about 4.5 kilometers .

46:24.790 --> 46:26.846
That was the same thing on Apollo 15

46:26.846 --> 46:28.901
when we passed over it . It was some

46:28.901 --> 46:31.300
4.5 kilometers below as mean radius

46:31.300 --> 46:33.522
here , and we're still referencing this

46:33.522 --> 46:37.050
to a 1738 0.1

46:38.510 --> 46:41.850
radius off the CG . If you take

46:41.850 --> 46:44.969
this stuff and start fitting it to an

46:44.969 --> 46:48.770
optical center with a CG

46:48.770 --> 46:52.080
offset , that you do indeed get the 2

46:52.080 --> 46:54.810
kilometer shift again of the CG being

46:54.810 --> 46:56.477
closer to the Earth by some 2

46:56.477 --> 46:59.520
kilometers . Let's say that tranquility

46:59.520 --> 47:01.479
is about 2.5 kilometers lower than

47:01.479 --> 47:04.250
Descartes . That's right , yeah ,

47:04.409 --> 47:06.520
here's the landing site right in here

47:06.520 --> 47:08.353
and uh this is we had a negative

47:08.353 --> 47:10.465
gravity anomaly in here , well , kind

47:10.465 --> 47:12.631
of according to this , maybe that's uh

47:12.631 --> 47:14.853
the situation because it looks like a ,

47:14.853 --> 47:18.379
a topographic globe . Yeah .

47:27.909 --> 47:30.620
This is the backside . We had some ,

47:30.739 --> 47:32.906
these are the limbs where the data was

47:32.906 --> 47:35.072
missing . These are taken from those ,

47:35.072 --> 47:37.072
this data is taken from that thrift

47:37.072 --> 47:39.295
printout that we get in real time , and

47:39.295 --> 47:39.250
there's some gaps in the data . These

47:39.250 --> 47:41.419
will be filled in , uh , once they get

47:41.419 --> 47:44.419
the station tapes delivered . But we

47:44.419 --> 47:46.475
can see the crater Hertz Sprung here

47:46.475 --> 47:48.697
very evidently with the central peak or

47:48.697 --> 47:50.863
something in it . You , you don't have

47:50.863 --> 47:54.540
any data on that . 100 , 120 degree

47:54.540 --> 47:57.300
region , not now . We should have it

47:57.300 --> 47:59.411
next week or so whenever they get the

47:59.411 --> 48:00.578
tapes here reduced .

48:03.169 --> 48:06.350
Uh , one of the things that , well , on

48:06.350 --> 48:08.620
Apollo 15 , there was a , a definite ,

48:08.770 --> 48:11.100
well , centered about 180 . There was a

48:11.100 --> 48:13.860
definite , uh , big , uh , trough in

48:13.860 --> 48:15.860
here which went down about some 4.5

48:15.860 --> 48:18.459
kilometers . It was very jagged , but

48:18.459 --> 48:20.626
it was centered just about here and on

48:20.626 --> 48:22.780
Apollo 16 now , we do not really see

48:22.780 --> 48:25.260
that . We see this hyland material here

48:25.260 --> 48:28.090
which we had on 6 , on 15 , that's ,

48:28.459 --> 48:30.792
that started about in here and showed a ,

48:30.979 --> 48:34.149
a marked , uh . High region in there .

48:34.520 --> 48:36.631
And then this is holding on , on , on

48:36.631 --> 48:38.853
16 also . So this is kind of consistent

48:38.853 --> 48:40.280
with Uh

48:42.350 --> 48:46.040
15 . Uh , here's , uh , another , this

48:46.040 --> 48:48.679
is orbit 38 on the backside . I'll just

48:48.679 --> 48:50.800
kind of lay it there to show you some

48:50.800 --> 48:54.639
of the consistency . This is 10

48:54.639 --> 48:57.969
orbits later and uh the profile is

48:57.969 --> 49:00.360
almost A Smith , the eye and uh oh here

49:00.360 --> 49:02.989
we have some data in that . So there's ,

49:03.110 --> 49:06.979
there's your data . OK . I don't know .

49:07.300 --> 49:09.356
Were you looking for some particular

49:09.356 --> 49:12.340
teacher for something around 105 , 105 .

49:18.719 --> 49:22.300
Uh , probably nothing dramatic .

49:25.340 --> 49:27.939
Uh , I do have some data on the

49:27.939 --> 49:29.995
sub-satellite from Apollo 15 , but I

49:29.995 --> 49:32.217
don't know if that's the time to really

49:32.217 --> 49:31.909
show here . I think I've shown enough

49:31.909 --> 49:34.790
stuff on 16 . Yeah , well , I'd like to

49:34.790 --> 49:36.679
stick to 16 . Any of the , of the

49:36.679 --> 49:38.679
problems we have or any of the data

49:38.679 --> 49:40.790
that we got for the crew . Well , I'm

49:40.790 --> 49:42.800
very happy with all the data I've

49:42.800 --> 49:46.550
gotten on 16 and Sub-satellite on 16

49:46.550 --> 49:50.010
like uh Larry mentioned just before me ,

49:50.590 --> 49:52.701
it's pretty grim although there was ,

49:52.709 --> 49:54.820
there was an OD solution just run out

49:54.820 --> 49:57.629
about an hour ago where the last state

49:57.629 --> 50:01.219
vector was uh Us as

50:01.219 --> 50:04.600
the uh Position

50:04.600 --> 50:07.139
for running out the lifetime program

50:07.489 --> 50:09.322
and the lifetime program , if we

50:09.322 --> 50:11.322
believe that 15-8 model that we had

50:11.322 --> 50:13.211
used initially back there when we

50:13.211 --> 50:15.156
injected that thing says that this

50:15.156 --> 50:17.360
thing should come back up , still says

50:17.360 --> 50:20.679
it's not going to crash . But this will

50:20.679 --> 50:22.901
be a very interesting thing to watch in

50:22.901 --> 50:22.750
the next couple of days , right ?

50:25.159 --> 50:26.603
That's the seismometers .

50:30.510 --> 50:32.760
Uh , I asked , uh , Kovach about that ,

50:32.840 --> 50:34.951
and I don't know whether he can speak

50:34.951 --> 50:37.062
for Latham or not , but , uh , I told

50:37.062 --> 50:39.284
him it's 50 pounds and whether they can

50:39.284 --> 50:41.679
actually see an impact of 50 pounds . I

50:41.679 --> 50:44.199
think that's all it weighs , the

50:44.199 --> 50:47.560
central station . Uh ,

50:49.010 --> 50:51.232
let's see , it should hit about maybe .

50:52.090 --> 50:54.570
Some 20 or 30 degrees west longitude

50:54.570 --> 50:56.800
and 5 or 6 degrees north , is that

50:56.800 --> 51:00.320
right , Something like that about 5 or

51:00.320 --> 51:03.020
6 north latitude and about 30 west .

51:03.659 --> 51:05.770
That's what it looks like that linear

51:05.770 --> 51:08.540
extrapolation that that's .

51:10.669 --> 51:13.360
Thank you , Bill . Thank you gentlemen

51:13.360 --> 51:15.304
for attending . This concludes our

51:15.304 --> 51:18.120
scientific debrief . And I'd like to

51:18.120 --> 51:20.342
thank the crew for giving their time up

51:20.342 --> 51:22.120
to come on over to give us some

51:22.120 --> 51:24.287
information and also learn some things

51:24.287 --> 51:26.342
that would happen . OK , uh , let me

51:26.342 --> 51:28.509
say something for the crew . I want to

51:28.509 --> 51:30.287
commend Ken for the way that he

51:30.287 --> 51:32.320
operated the Simba . I don't think

51:32.320 --> 51:34.320
you'll ever find a guy who's either

51:34.320 --> 51:36.959
more interested in it or more aware of

51:36.959 --> 51:39.126
what the operational problems were and

51:39.126 --> 51:42.100
who could do a better job . He really

51:42.100 --> 51:44.322
did an outstanding job and I think he's

51:44.322 --> 51:46.544
well done . The other thing I'd like to

51:46.544 --> 51:48.378
say is , since I've been on this

51:48.378 --> 51:50.156
program , I've been continually

51:50.156 --> 51:52.267
impressed with the importance of what

51:52.267 --> 51:56.020
we're doing in in uh . In our support

51:56.020 --> 51:58.187
of you guys , these experiments , they

51:58.187 --> 52:00.679
look way out right now , and they're

52:00.679 --> 52:02.846
difficult for the man in the street to

52:02.846 --> 52:06.489
relate to . But my feeling is from some

52:06.489 --> 52:08.600
of the things I've seen here and from

52:08.600 --> 52:12.250
the thrust of science and technology in

52:12.250 --> 52:15.250
this country that in our lifetime and

52:15.399 --> 52:17.689
and I won't want to say when , but I

52:17.689 --> 52:19.856
imagine it's going to be a site sooner

52:19.856 --> 52:22.078
than anybody even here in this room can

52:22.078 --> 52:24.189
imagine they're going to be practical

52:24.189 --> 52:25.856
applications of some of these

52:25.856 --> 52:27.911
discoveries that have been made that

52:27.911 --> 52:29.911
will affect every one of us . And I

52:29.911 --> 52:32.078
think you're to be congratulated . The

52:32.078 --> 52:31.939
other thing is that I get out of all

52:31.939 --> 52:33.939
this that I think the United States

52:33.939 --> 52:36.050
ought to be spending 2 to 3 times the

52:36.050 --> 52:38.272
amount of money that we are spending on

52:38.272 --> 52:40.217
basic research and development and

52:40.217 --> 52:42.383
applied research and development . And

52:42.383 --> 52:44.495
I think if you really look at the big

52:44.495 --> 52:46.661
picture of our energy requirements for

52:46.661 --> 52:48.828
clean energy in the future in order to

52:48.828 --> 52:50.828
improve the life of human beings on

52:50.828 --> 52:52.939
this planet , we ought to do that and

52:52.939 --> 52:54.550
get on with it . Thank you .

52:58.649 --> 53:02.459
During the next couple of months

53:02.879 --> 53:05.100
we'll probably have an opportunity to

53:06.070 --> 53:08.320
Talked to a lot of people that helped

53:08.320 --> 53:10.810
to have some influence or shape the

53:10.810 --> 53:12.959
pattern of our program and related

53:12.959 --> 53:16.580
programs . And I would appreciate

53:16.580 --> 53:19.189
it very much . I'm sure we all could

53:19.189 --> 53:21.300
use the data as you find out things ,

53:21.300 --> 53:23.356
we realize that you have preliminary

53:23.356 --> 53:25.590
data today and a lot of the things are

53:25.590 --> 53:27.812
only hints and suggestions of things to

53:27.812 --> 53:31.709
come . I would personally appreciate

53:31.709 --> 53:33.653
it very much if you give us a call

53:34.270 --> 53:36.603
periodically and tell us what you found .

53:36.979 --> 53:39.201
It's too easy for us to go through here

53:39.201 --> 53:41.629
and at the end of a week or so walk off

53:41.629 --> 53:43.851
and never really know what happened and

53:43.851 --> 53:46.073
never know what kind of data came out .

53:46.073 --> 53:48.879
And uh I think that makes us very poor

53:48.879 --> 53:52.850
salesmen . I think you could help us do

53:52.850 --> 53:55.129
the job to kind of feedback the quality

53:55.129 --> 53:57.296
of the data that you've been getting .

53:57.296 --> 53:59.296
If you could keep us informed , and

53:59.296 --> 54:01.240
please don't ever feel like you're

54:01.240 --> 54:03.462
interfering with our operation or don't

54:03.462 --> 54:05.462
be inhibited to call us if we can't

54:05.462 --> 54:07.629
come to the phone and take the data or

54:07.629 --> 54:09.685
talk to you about it . The secretary

54:09.685 --> 54:11.685
will take the number and we will be

54:11.685 --> 54:13.851
glad to call you back . And if there's

54:13.851 --> 54:15.907
any time when you have some question

54:15.907 --> 54:18.073
about the data , and it doesn't matter

54:18.073 --> 54:20.296
how trivial it may seem to you , if you

54:20.296 --> 54:20.129
want to look at some data and you're

54:20.129 --> 54:22.351
curious to know whether we've ever seen

54:22.351 --> 54:24.810
a particular observation or whether the

54:24.810 --> 54:26.977
spacecraft was moving at the time your

54:26.977 --> 54:29.399
data was taken . I don't care how far

54:29.399 --> 54:31.500
out it might seem to you , questions

54:31.500 --> 54:33.600
are pretty cheap , and not asking

54:33.600 --> 54:35.656
questions can be very expensive . So

54:35.656 --> 54:38.120
please feel like our job isn't finished

54:38.120 --> 54:40.342
until you guys have all the information

54:40.342 --> 54:42.679
you can use , and I would like for you

54:42.679 --> 54:44.679
to feel like you can call anytime .

54:44.679 --> 54:48.040
Thank you very much . I'd like to give

54:48.040 --> 54:50.320
you my thanks also . I was very pleased

54:50.320 --> 54:52.264
with the way all the gear worked ,

54:52.949 --> 54:55.171
especially my part on the lunar surface

54:55.171 --> 54:58.330
and the part I saw of Ken in orbit . Uh ,

54:58.600 --> 55:00.711
it was just a real pleasure to , uh ,

55:00.919 --> 55:03.086
have him placed all this stuff for all

55:03.086 --> 55:05.197
you people , and , uh , I'm glad it's

55:05.197 --> 55:07.479
working so well . And , uh , thanks for

55:07.479 --> 55:09.590
the opportunity of going . If you can

55:09.590 --> 55:11.757
gin up another one , I'll be glad to ,

55:11.757 --> 55:13.100
uh , go along again . Thank you .

