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Day 1: Transposition, Docking and Extraction Journal Home Page Day 2, part 1: Settling down & navigation

Apollo 17

Day 1: "A regular human weather satellite"

Corrected Transcript and Commentary Copyright © 2017 by W. David Woods and Ben Feist. All rights reserved.
Last updated 2018-06-27
005:08:55 Cernan: And, Bob, we're on page 3-9 of the Flight Plan now. We'll check the LM/CM Delta-P, get the cabin fan filter in. We'll go over the check - the Systems Checklist, get the primary EVAP and a few odds and ends, and start doffing our PGAs. How's that sound?
005:09:16 Overmyer: Sounds like a winner, Gene.
005:09:19 Cernan: Okay.
005:11:01 Schmitt: I guess you saw that one, Houston. That had no caution or warning with it.
005:11:10 Overmyer: Roger. That a Master Alarm?
005:11:12 Schmitt: Yes, sir.
005:11:14 Overmyer: How about the LEB?
005:11:15 Schmitt: Gene's got [garble] say again. [Laughter.] You caught me. I forgot to look. Keep after us; we'll get you that data point.
005:11:26 Overmyer: Roger, Jack.
005:11:30 Schmitt: Gene's got his hands all over panel 2, which probably is what caused it.
005:11:52 Overmyer: Jack, we think that might have been a real one due to the accumulator cycle with the O2 makeup flow going on there. It gave - it held the O2 flow higher for - greater than the 16 seconds.
005:12:06 Schmitt: Well, that's certainly a possibility. We didn't notice it - Looked upright at the time. But it - Sure that was the right time?
005:12:17 Overmyer: Well, EECOM's watching it here, and he feels it is.
005:12:24 Schmitt: Gee, I can't argue with him.
005:13:50 Schmitt: Okay, Houston. Ready to deactivate the primary evaporator if you concur.
005:14:01 Overmyer: Roger, Jack. We concur.
The spacecraft's evaporators are a means of losing excess heat when the Service Module's radiators are already working at full capacity. There is a primary and secondary unit and they work by evaporating water to space. This carries off heat and serves to cool the fluid in the spacecraft's coolant loop.
005:15:50 Schmitt: Okay, Bob. VHF Simplex Alpha's Off.
005:15:57 Overmyer: Roger.
005:16:01 Schmitt: And we're gradually moving into getting out of the suits.
005:16:05 Overmyer: Yes. I'll bet you're looking forward to that.
005:16:10 Schmitt: Well, I'll tell you it's a different world without that old 1-g on you. The old suit's a little bit friendlier.
005:17:16 Schmitt: And, as you may have noticed, Bob, we've come to the end of the Launch Checklist.
005:17:23 Overmyer: That's affirmative, and we've put ours away for posterity. We also stored it with our TLI-0 data that we worked so hard to generate.
005:17:37 Schmitt: Well, I'm just happy - didn't - use it. That view of the Earth for a rev there was something I was looking forward to and I was not disappointed.
005:17:49 Overmyer: That's great, Jack.
005:17:54 Cernan: Bob, you've got a pretty good size storm over the north - I guess the north-western coast of India, where it starts to wrap up and around to the west. It's a - rounded out on the horizon, so I can't make out exactly where it is too well.
005:18:17 Overmyer: Roger.
005:18:21 Overmyer: Could we get a read-out on the LM/CM Delta-P?
005:18:51 Schmitt: Plus 0.4.
005:18:56 Overmyer: Roger. We copy that.
The absolute pressure within the CM is 0.4 psi or 2.8kPa higher than that of the tunnel just beyond the forward hatch. The tunnel's pressure should also be the same as the LM's as it was normal for the overhead dump valve in the upper hatch to be left open before launch in order to have the LM cabin evacuate as the vehicle entered space.
005:19:00 Cernan: Bob, Antarctica is what I would call effectively just a solid white cap down on the - South Pole. There's definite contact between the continent and the water. But, as Ron said, most of the clouds seem to be, well very artistic, very picturesque - some in clockwise rotating fashion but appear to be very thin where you can, for the most part, kind of see through those clouds to the blue water below.
005:19:45 Overmyer: Roger.
005:19:46 Cernan: The continent - the continent itself is - is the same color as the clouds; but, of course, more dense - and striking difference than any of the other white background around because you can definitely see that contact with the water and with the clouds over the water.
005:20:05 Overmyer: Roger. Understand. There'll soon be a comm switch over to Madrid here shortly. We may break lock in a few minutes here. Or a few seconds, rather.
005:20:26 Overmyer: And you might watch - your accumulator's going to cycle in about 20 seconds here. Let's see what happens on the Master Alarm.
005:21:03 Overmyer: 17, Houston. How do you read through Madrid?
005:21:07 Schmitt: You're loud and clear, Bob, and could you give us our distance from the Earth?
005:21:12 Overmyer: Roger. I'm looking up at the board. I'd guess at about 19,000 [nautical] miles [35,000 km]. Want me to get it exact?
005:21:18 Evans: No, just approximate's good enough.
005:21:24 Overmyer: 18,100 [nautical miles, 33,520 km], FIDO says.
005:21:27 Cernan: Okay. And I suppose we're seeing as 100 percent full Earth as we'll ever see; certainly as I've ever seen. It appears to be - it may be a little bit - a little bit of a terminator way out to the - well, to the east - out beyond Australia and beyond India. But beyond that it's about 99 percent pure.
005:22:59 Cernan: Bob, it's these kind of views - these kind of views that stick with you forever.
005:23:07 Overmyer: Roger, Gene.
005:23:09 Cernan: We've got a - I guess probably the continent of Africa dominates the world right now. It's covering the - oh, the upper third - upper and western third of the - of the world. We can see the Sinai; we can see up into the Mediterranean; we can see across the Mediterranean, although we can't quite make out the countries up there; we can see across into India. I catch a glimpse of Australia out in the far horizon. Got Zanzibar on the southern tip of Africa, the Cape down there just almost directly below us. And, I don't know exactly how big Antarctica is, but I guess we can certainly see more than 50 percent of it. And - the rest of it is all ocean. The Indian Ocean out into the Pacific Ocean and back into the Atlantic Ocean. And for the most part relatively clear of clouds except in the Antarctica region, and up towards Europe which is - which is on the horizon, across the Mediterranean, it looks like there might be some clouds back up in that way. I can probably - probably - well, not probably - I can make out the entire coast of Africa from Mediterranean around to the west, coming back to the south, back where it takes its big dip to the east, back around the Cape, back around up through the Suez Canal, almost perfectly.
005:24:59 Overmyer: Roger. We understand.
005:25:02 Cernan: And there's one batch of clouds in northern Africa, just a small batch, it looks like it may be up near the - well, no, it's not near the mouth of the Nile; it's quite a bit west of that as a matter of fact, I can see the mouth of the Nile; I can see it running straight down towards us as it parallels the Suez, and then sort of fades out into the central darker brown or darker green portions of Africa.
005:25:37 Overmyer: Roger, Gene. Sure be nice to have that on TV, wouldn't it?
005:25:42 Cernan: Boy, I'd love to give it to you; any way I could.
005:25:56 Cernan: You know - and there's no strings holding it up either. It's out there all by itself.
005:26:07 Overmyer: Roger. I just was going through the 17 status report on CSM systems and, boy, everything is absolutely nominal, with the exception of [garble] glitching Master Alarms that we're trying to still track down; but every other system is just nominal it's - everything is great.
005:26:30 Cernan: Okay. Sounds good. That's the way they built it for us.
005:27:29 Overmyer: Gene, looking at our plot board, you're directly over the southern tip of Africa or just slightly out in the Indian Ocean there, according to our plot board, which isn't exactly accurate all the time. But shortly you're going to start going backwards on the Earth here and head back across the Atlantic. That ought to be some sort of a first. You cross the Atlantic twice, going from west to east, and then, now you're going to cross it going from east to west here shortly. All in a very short span of time.
005:28:09 Schmitt: Yes. I guess that does sound like a first.
005:30:00 - This is Apollo Control at 5 hours, 30 minutes Ground Elapsed Time. The White team of flight controllers, headed by Gene Kranz, is in the process now of handing over to the team headed by Flight Director Pete Frank. After 12 hours, the team came on about 3 hours prior to the scheduled launch time of 8:53 pm Central Standard Time. Of course, launch occurred 2 hours, 40 minutes late at a Ground Elapsed Time of 11, - of a Central Standard Time rather, 11:33 pm. As a result of the late launch time, the Translunar Injection, that's up through Translunar Injection, also slipped 2 hours, 40 minutes. We would expect that the Translunar Injection, which is targeted to make up the difference, will get us back on the nominal Flight Plan time by the time the spacecraft arrives at the Moon. In other words, arrival time at the Moon would be at the same Central Standard Time as called for in the Flight Plan at about 1:49 PM Central Standard Time, December 10. But, the Ground Elapsed Time would be about 2 hours, 40 minutes earlier than that provided for in the Flight Plan, the arrival being at about 86 hours, 14 minutes Ground Elapsed Time. The 2-hour, 40-minute difference being accounted for in a speedier arrival time at the Moon, a Translunar Injection burn being targeted just slightly longer than would have been the case in a normal launch. The spacecraft getting to the Moon in a total elapsed time 2 hours, 40 minutes less; in effect, making up for lost time from the late launch. In order to get the Flight Plan back in agreement with the Ground Elapsed Time, the GET, or ground elapsed clock, will simply be moved ahead 2 hours, 40 minutes between now and the time spacecraft arrives at the Moon. So, that by the time Apollo 17 is inserted into lunar orbit, the GET will once again agree with the Flight Plan GET and of course, the Central Standard Time of arrival will be the same as was originally planned by virtue of a speedier trip time. As a result of the late lift-off, it was not possible to program television coverage of the transposition and docking. This was because of a shift in the orbital ground track moving the ground track away from the needed Manned Space Flight Network coverage for television. We simply didn't have an adequate ground station to receive the television signal from the spacecraft. There has been one recurring problem that is yet unexplained. That is in the displays and control system. The crew reported on several occasions that Master Alarm was occurring. The Master Alarm manifests itself in a form of a light that flashes in the Command Module. There are three of these lights and also a tone that comes on and a normal procedure is when the Master Alarm light comes on and the tone sounds, the crew then looks at another matrix of lights to determine precisely where the problem is. However, when looking at this matrix of lights none of them were lighted, indicating that some spurious signal had ignited or lighted the Master Alarm light and that there was in fact no problem in the systems. There is at this point no explanation for the problem. However, engineers here in the Control Center, are looking into the past history of Panel 2, which is the panel on which a number of switches are located, which have triggered this Master Alarm, to see if there is a history of Panel 2 that would indicate a possibility of some momentary short in the Caution and Warning system which could give a Master Alarm. The problem at this point is an annoyance, but does not appear to be a serious problem. All other spacecraft systems are performing normally, and the trajectory to the Moon is almost precisely as planned at this point. We do not anticipate a change of shift press briefing. The White team will be coming back on at the regular Central Standard Time 4:00 pm tomorrow. And in light of this rather short turnaround, we're going to forego the change of shift press briefing. At 5 hours, 36 minutes; this is Apollo Control, Houston.
005:30:01 Cernan: Bob, I can assume that from what you said there will be - probably not be a midcourse 1?
005:30:02 Overmyer: That's exactly what we're working towards, Gene. And I - I'm sorry I didn't convey that feeling to you a little earlier. There's no reason for midcourse 1 right now.
005:30:03 Cernan: Okay. Because we prefer to press on and get the suits off and hit the sack rather than make it, unless we have to.
005:30:04 Overmyer: That's for sure. Roger. The earlier data showed us midcourse 1 would have been less than 3 feet per second, and we wouldn't have done it. And the data's been fluctuating, but they're smoothing it out, and it's still holding that way; so we won't be doing it, probably.
005:30:05 Cernan: Okay. Very good.
005:30:06 Schmitt: Bob, I'm looking over Gene's shoulder here at the Earth, and it must be an awful clear day for the so-called convergence zone across Africa. Gene, I think, Indicated, as it looked to us as we crossed it earlier, most of Africa is clear. Only some - probably are broken and scattered clouds - cumulus in the east central portion that are running along the line of - north/south lines.
005:30:07 Overmyer: Roger.
005:30:08 Schmitt: Looks like a major circulation system off the southern tip of Africa, as Gene mentioned, plus one west of that, 20 or 30 degrees of longitude. Make that east of that.
005:30:09 Overmyer: Roger.
005:30:10 Schmitt: And, southwest of the - make that south southwest of the tip of Africa at Cape Good Hope, there looks like an incipient circulation system developing about half way between the coast of Antarctica and Africa. If I had to guess, it's going to swing up north towards the Cape and - and then swing west. The whole pattern, [garble] it looks like now, is a fairly equally spaced cyclones that are sort of circling around the Antarctic continent, as we can see it now.
005:30:11 Overmyer: Roger, Jack.
005:33:50 Schmitt: But I would guess that South Africa is going to have good weather for several more days, at least. And if the pattern is - is apparent in the clouds we see is correct, the last disturbance I mentioned probably is going to pass south of the Cape also,
005:33:51 Overmyer: Roger. Understand.
005:33:52 Schmitt: As we were going - over our daylight around the Earth in orbit, it was very clear looking at the various clouds, Bob, what were high clouds and what were low clouds, particularly when you had them together. The high clouds cast very distinct shadow patterns on the lower ones and, very commonly, had entirely different orientations -pattern orientations. The low ones seem to be more associated with arcuate front patterns; whereas, the high clouds were generally transverse to that, roughly north/south directions. That's not completely general observation, but I noticed it several times.
005:33:53 Overmyer: Roger. Understand.
005:33:54 Overmyer: I just noticed on the plot board here, it looks like you're come up on 20,000 [nautical] miles out, right about now.
005:35:27 Schmitt: It feels like about, 20,000 [nautical] miles.
005:35:27 Overmyer: Okay.
Comm break.
005:37:28 Schmitt: Bob, I have the first hint of contamination on window 5. It's covering, probably, the central - well, I'd say, - roughly around - it's square about - 7 inches in - on a side with a very thin film that's catching the sunlight; and slightly iridescent, but also very finely granular - very finely granular. You can just barely tell what it is, actually.
005:38:09 Overmyer: Roger. Understand.
The windows in the Command Module are numbered 1 to 5 starting at the commander's side.
The numbering system for the Apollo Command Module
This photo of Command Module America taken in lunar orbit shows the numbering system for the spacecraft's five windows.
Window five is therefore on the LMP's side, furthest to the right as seen from their couch positions.
005:38:11 Schmitt: Looks like very uniform in thickness right now.
Long comm break.
005:46:55 Schmitt: Bob, this is Jack. We've got a UCTA dump scheduled, or is possible, at 6 o'clock. There's nothing sacred about that time, is there?
005:47:11 Overmyer: Nothing at all. Whenever you're ready, just go ahead and dump.
005:47:15 Schmitt: Okay.
Comm break.
005:48:48 Schmitt: Bob, one of the things that we missed in our training is a good geography lesson, and particularly on Antarctica. I got the monocular out, and apparently the dark band that Gene - Ron mentioned as interface between the continental water is that between the pack ice and the water. And you can, by very subtle changes in the apparent smoothness of the ground, probably make out where the actual continent begins and the pack ice ends. There are a few exposed ranges, I guess it's midsummer down there now, and you can make out the snow-free areas scattered at least in the northern portion of the continent.
005:49:47 Overmyer: Roger. Did you get any pictures of that, Jack?
005:49:50 Schmitt: Oh, yes. We got some pictures earlier. I'm going to get another one here in a minute. I'll tell you, if there ever was a fragile-appearing piece of blue in space, it's the Earth right now.
005:50:03 Overmyer: [Laughter.] Roger.
005:50:06 Schmitt: And we got a Master Alarm.
005:50:08 Overmyer: Okay. We copy that.
005:50:11 Schmitt: And there's one in the LEB.
005:50:14 Overmyer: Okay. Good data point.
005:50:18 Schmitt: And there are no caution lights.
005:50:21 Overmyer: It came right at accumulator cycle, along with the high O2 flow again.
005:50:26 Schmitt: Yes, I just checked the time, and I think you are right on that one. Well, we gave you your LEB data point.
005:50:39 Overmyer: Yes, sir.
005:50:49 Schmitt: The problem with looking at the Earth [laughter] particularly Antarctica, is it's too bright.
005:51:00 Overmyer: Understand.
005:51:02 Schmitt: And so I'm using my sunglasses through the monocular, which is not the best [laughter] viewing platform. I think I can see some of the areas of the Dry Valley, but, again, I'm not too sure of my geography Bob. There are clouds over the continent, I believe, but, of course, they're just as white as the snow, and you only see differences in texture brought out by - probably varying photometric return because of fairly low sun angles down there.
Schmitt, from 1973 Technical debrief: "Partly, I used my glasses because they do have a small correction for my astigmatism, and that did increase the resolution with which I could view the surface. Looking at the Earth and translunar coast with the sunglasses, I often did that for the correction. I used the binocular and the sunglasses and it did seem to help the resolution of viewing cloud patterns and geographic locations. When I used the sunglasses they seemed to be very adequate in terms of the level in which they reduced the brightness. As soon as I looked in the cabin to look at instruments and this sort of thing, the glasses did inhibit the observation of those instruments and the lettering on the panels, and I would push them up on my forehead for cabin work."
005:51:41 Overmyer: Roger.
005:51:47 Schmitt: But you can see patterns of what I believe is pack ice - leading off from that sharp interface that was talked about earlier. And those patterns seem to merge directly with the patterns of the clouds as if the - at least near the continent - the oceanic currents are controlling the air currents, up to a point, along with the movement of the pack ice.
005:52:24 Overmyer: Roger.
005:52:25 Schmitt: I'm distinguishing the pack ice from clouds mainly by the angularity of the patterns within them. There is no good clear color or albedo distinction. So, I could - I could be looking entirely at clouds, but I suspect there are some pack ice patterns, too. I'm not keeping you awake, am I, Bob?
From the ALSJ - Throughout the outbound journey, they had a good view back toward Earth. Schmitt, in particular, provided lengthy and detailed weather reports, complete with predictions. His first report, given while Cernan and Evans were getting out of their suits, went on for a full half hour and, as the Earth turned beneath them, he could update his predictions for various parts of the world. Later in the mission, CapCom Gordo Fullerton told him, 'You're a regular human weather satellite.'
005:52:53 Overmyer: No, sir. Just keep talking; we're listening. And I'm sure not much of the world is listening, but this will all be recorded, and you can read it all when you get back and think it through and tie it up with the pictures. And I'm sure there's going to be people interested in this. And we're interested ourselves; just keep talking.
005:53:11 Schmitt: All I want to do is read what I say.
005:53:14 Overmyer: Roger. If I had a little more geology training, I'd be asking you some better questions. I'm afraid, right now, I can't think of anything to ask you.
005:53:21 Schmitt: Well, I can't - I really wish I knew that geography. I don't know - I wish I'd thought of bringing a good map of Antarctica. Could somebody do a little researching for me and see if they could tell me if we're - have a Little American view - say on the eastern edge of the continent?
005:53:48 Overmyer: Roger. We'll see if we can get some Antarctica geographers around.
005:53:53 Schmitt: Yes, I'd like to - and, also, whether or not they think the Dry Valley area is visible to us. Let's see, there's some - some of the people over there in Bill Bennett's group, I think, have a little Antarctic experience, or used to. They might be able to help you out.
005:54:10 Overmyer: Okay. We'll see what we can track down on it.
005:54:13 Schmitt: Don't use up a lot of people's time on it, but - but I'd be interested.
005:54:18 Overmyer: Roger. It's getting pretty empty around here. It's 5:00 in the morning, so - [laughter]
005:54:25 Schmitt: Okay. There is a good strong northern hemisphere cyclone up near India, and I think Gene mentioned that. It, I think, was one I saw in some of the forecast sheets as a dissipating hurricane or typhoon. I'm not sure which it is there. I guess it's a typhoon. And I see something here that I noticed in Earth orbit, Bob. That as you approach the terminator - and now I'm looking at the eastern terminator - have to keep all my directions straight here - yes, eastern terminator. The clouds - those associated with the cyclone over India and one that's - appears to be due south of there - maybe 30 degrees of latitude - have a gray appearance. The - instead of the brilliant white of other clouds as you approach the terminator, those - at least the high level clouds are gray. Now, when we were going over them in orbit, the lower level clouds were still white, and I think I can see a hint of that right now. The Sun gives a strong light reflection off of the buildups in the low-level clouds; whereas, the high-level and probably layered cirrus and maybe some of the intermediate level stratus tend to look gray because of grazing Sun, I suspect.
005:56:26 Overmyer: Roger. You mentioned something in Earth orbit that kind of intrigued me. You mentioned seeing the rainbow, and we were trying to figure out how you saw a rainbow up there. And you were in orbit already at that time. Do you remember that?
005:56:41 Schmitt: Well, - we're not - we were speaking of the merits of the sunrise.
005:56:46 Overmyer: Okay. Roger.
005:56:50 Schmitt: - having a banded color appearance that varied as you approached sunrise. I can't remember what we - I think we put some of that on tape, and we were probably LOS at the time. But the banded character of the sunrise in the atmosphere was very, very marked. There was a gray-blue upper layer followed - that merged or graded into a brilliant blue intermediate zone that was just above the cloud levels. And within the clouds, you got a orange to yellow band, getting more yellow as the Sun rose, that was broken by the dark patterns of the buildups.
005:57:54 Overmyer: Roger. Good show.
005:57:59 Schmitt: The interesting thing was the continual glow on the horizon we had, even at night, on the darkside pass - and that glow was in the atmosphere because I could see stars rise over the horizon in it and then pass on through it.
005:58:19 Overmyer: Roger. You were talking - the airglow, I guess, is the phenomenon most of the guys had seen before. It's kind of Interesting, Yes?
005:58:25 Schmitt: Yes, that's - that's right. It's interesting - I guess standard airglow, but it is very striking that it's a continuous thing even in the dark pass.
005:58:36 Overmyer: Roger.
005:58:42 Schmitt: I think I did see the eastern tip of South America, now.
005:58:56 Overmyer: Roger. You're starting to back up now, coming the other way. So you're still over Africa, according to our chart here, but you're backing up towards the - South America.
005:59:07 Schmitt: Yes, I can see the part of South America that Wegener thought that fitted in with the bend in Africa some many decades ago and started people thinking about moving continents around on the crust.
Jack is referring to Alfred Wegener, a German scientist who, upon hearing about similar fossils being found on either side of the Atlantic Ocean, noted at the close fit of Africa's western coastline with the eastern coast of South America. In 1915, after he had amassed more evidence of a similar nature, he put forward the theory of continental drift and suggested that 300 million years ago, Earth's landmasses had been together in a single supercontinent. Wegener's work led to our current understanding of plate tectonics. As will be clear from Jack's comment below at 006:11:21, he is one geologist that in 1972 still needs to be convinced that plate tectonics is a major mechanism within Earth's crust. However, the view from far out in space is beginning to sway him.
005:59:25 Overmyer: Roger. Jack, how'd the PGA doffing go? Most of you - are you all out of the PGAs now?
005:59:38 Schmitt: That's in work. We're taking it slow and easy up here, Bob.
005:59:41 Overmyer: Roger. Understand. I'll just be curious to see if they all fit in that bag.
005:59:48 Schmitt: I think you'll find that Ronald Evans will also be curious about that. He's already making comments.
005:59:56 Overmyer: Roger.
006:00:03 - This is Apollo Control at 6 hours. As Jack Schmitt gives the description of the Earth, Apollo 17 is 22,868 nautical miles [42,352 km] from Earth; velocity, 12,520 feet per second [3,816 m/s].
006:00:17 Schmitt: Bob, you certainly do have a very clear intuitive impression, although the evidence is hard to pull together, that the - any frontal systems that move off the Antarctic continent do not take on any well-defined character until they get into the moist regions of the ocean. And when they do, they seem to pick up an arcuate circ - circulation that, in the view we have, seem to get fairly regularly spaced cyclone patterns that lie between the Cape of Good Hope and northern portion of Antarctica. And these - circulations of the cyclones follows roughly an east/west pattern, and the curve - and the arcs of the fronts are more north/south than - let's say northwest, swinging around to the south.
006:01:30 Overmyer: Roger.
This circulation pattern that runs around the Antarctic continent is responsible for limiting the amount of heat that gets delivered to the South Pole from Earth's warmer regions. In the north, the interplay of Oceans and continents has the effect of sending heat to the pole via the Gulf Stream and the North Atlantic Drift. This helps to make the Arctic substantially warmer than Antarctica
006:01:30 Schmitt: All of them - all of them very - very nicely defined as southern hemisphere cyclones. There - about four of those visible swinging around - oh, I guess, that's latitude - I'm having to guess here, but I'd say latitude 50 to 60 south.
006:01:55 Overmyer: Okay; 50 or 60 south on that, huh?
006:01:58 Schmitt: Yes, I have to look at the map here in a minute and see if that puts me between Antarctica and the Cape.
006:02:03 Overmyer: Roger.
006:02:08 Overmyer: Well, the tip - the tip of Africa there is at about 32 south.
006:02:14 Schmitt: Well, that sounds like a pretty good guess, then. It looks like the intertropical convergence zone over Africa is starting to get more and more clouds in it now. I suspect as midday approaches, which is what we're seeing there, we can expect to see more and more moisture indications.
006:02:39 Overmyer: Roger. They're - they're probably about noontime right there right now. It's 11:36 at the zero meridian at Greenwich, so it's just a little bit before noon right in that area you're talking about.
006:02:51 Schmitt: Yes, some of those masses of what I suspect are cumulus buildups - well, not really. They don't look like they're as concentrated and localized. More like just masses of fairly dense clouds that are developing in that band of green that crosses the lower portion of Africa.
006:03:17 Overmyer: Roger.
006:03:55 Schmitt: Stay tuned for the next instalment on the Earth. I'll try to get out of this suit.
006:04:01 Overmyer: Okay. Just take it easy, Jack, and we'll be listening.
006:04:06 Schmitt: Man, I've never taken it so easy in my life. I'll tell you, Bob, I couldn't have believed this would be an experience like it is now.
006:04:15 Overmyer: Roger.
006:04:21 Schmitt: Every time you turn around, there is something else to see and wonder what's causing it. Whether it's a particle zipping across the window, or one zipping across the cabin, or spring mechanics here in zero g; there's always something going on.
006:04:37 Overmyer: Roger.
006:07:05 - This is Apollo Control at 6 hours, 7 minutes. No midcourse correction number 1 will be performed. The value of the maneuver that would be required is less than 3 feet per second [0.9 m/s] and midcourse correction number 1 will not be performed by Apollo 17. The spacecraft is now 23,682 nautical miles [43,859 km] from Earth; velocity, 12,301 feet per second [3,749 m/s].
AS17-148-22729 - The nearly full Earth at a distance of approximately 44,800 km (based on photo analysis). First in a sequence of five images taken slightly later than the Blue Marble series and, upon close examination, appears to be the sharpest - JSC scan
AS17-148-22730 - The nearly full Earth at a distance of approximately 44,950 km (based on photo analysis). Second in a sequence of five images taken slightly later than the Blue Marble series - JSC scan
AS17-148-22731 - The nearly full Earth at a distance of approximately 45,000 km (based on photo analysis). Third in a sequence of five images taken slightly later than the Blue Marble series - JSC scan
AS17-148-22732 - The nearly full Earth at a distance of approximately 45,000 km (based on photo analysis). Fourth in a sequence of five images taken slightly later than the Blue Marble series - JSC scan
AS17-148-22733 - The nearly full Earth at a distance of approximately 45,000 km (based on photo analysis). Fifth in a sequence of five images taken slightly later than the Blue Marble series - JSC scan
006:09:55 Schmitt: Bob, if I'm not waking you up, an observer from another planet certainly - probably could decide that we have such things as clouds and at least large thunderstorms because right at the terminator you get a brightening of the sunlit side and a long, long shadow out to the - out to the east that is reminiscent of what we saw in the early days looking at the Moon at the terminator.
006:10:37 Overmyer: Roger.
006:10:40 Schmitt: However, in the next pass around, I'll bet you wouldn't see them.
006:11:21 Schmitt: I've never been a big - Well, I didn't grow up with the idea of drifting continents and sea-floor spreadings, but I tell you, when you look at the way the pieces of the - of the north-eastern portion of the African continent seem to fit together, separated by a narrow gulf, you could almost make a believer of anybody.
006:11:22 Overmyer: Roger. It's beginning to look like the globe that you might buy down at the store, huh?
006:11:57 Schmitt: Oh, I don't think so, Bob. [Laughter.]
006:11:59 Overmyer: Okay.
006:12:01 Schmitt: I don't think we'd better put this one up for sale. Somewhere there might be somebody who would like to buy it.
006:12:27 Overmyer: Say, Jack. We noticed the O2 flow has dropped down now. We're wondering, did you all close the waste storage vent valve?
006:12:36 Schmitt: I don't think so; let me check on that. It might have gotten closed inadvertently in this game we were playing down in the LEB.
006:12:55 Schmitt: Ron says it's still on Vent.
006:12:58 Overmyer: It's on Vent. Roger.
006:13:07 Overmyer: Okay. We're noticing the flow is coming back up slowly; so something caused it to drop, and it's coming back up.
006:13:15 Schmitt: Okay.
Long comm break.
006:17:41 Overmyer: 17, Houston.
006:17:44 Schmitt: Go ahead.
006:17:45 Overmyer: Jack, just to ease those words I said before, we looked at the schematics here a second, and you'd be dumping urine out of that same line as that waste vent, and that would probably cause the pressure to build up enough to slow the O2 flow. And we noticed that the O2 flow is climbing back up to where it belongs.
006:18:08 Schmitt: Well, that's clever. Okay.
006:18:11 Overmyer: Didn't mean to worry you there. Shouldn't have said it, I guess, before we looked at the schematic.
006:18:18 Schmitt: Oh, I really hadn't started to worry about it yet, Bob, so no sweat.
Long comm break.
006:22:15 Schmitt: How'd the S-IVB work go Bob?
006:22:24 Overmyer: They just finished their second burn, and it's targeted right where they want it. Just working perfectly.
006:22:34 Schmitt: Where were they going to put that one? I guess I lost track of that.
006:22:52 Overmyer: 7 degrees south and 8 degrees west, Jack.
006:22:57 Schmitt: Say again, you cut out on the first.
006:23:00 Overmyer: Okay; 7 degrees south and 8 degrees west.
006:23:09 Schmitt: Okay. That ought to be interesting.
Long comm break.
The S-IVB is targeted to impact the Moon near the craters Ptolemaeus and Lalande in order to provide a calibrated shock event with which the suite of seismometers already emplaced by Apollo's 12, 14, 15 and 16 can probe the lunar interior.
006:23:29 - This is Apollo Control at 6 hours, 24 minutes. The S-IVB maneuver that was just being discussed was performed with the Auxiliary Propulsion System; just completed Delta-V of 13 feet per second [4 m/s] to tune up the trajectory for S-IVB impact at the desired location on the lunar surface of 7 degrees south, 8 degrees west. That's approximately 200 kilometers east of the Apollo 14 ALSEP site where the seismometer is located. That impact is expected to be picked up by the other seismometers on the Moon, the other Apollo lunar surface experiment seismometers. Booster systems engineer is now maneuvering the S-IVB stage, the third stage of the launch vehicle to a solar heat control attitude. This is to minimize the heat into the instrument unit. They will then track the stage for a considerable length of time and determine whether another corrective burn will be required. At 6 hours, 25 minutes into the mission; this is Mission Control, Houston.
006:27:06 - This is Apollo Control at 6 hours, 27 minutes. Booster systems engineer has just reported to the Flight Director that the S-IVB stage is in good shape, with 14 hours life time remaining. The limiting factor on the S-IVB is the battery life. Fourteen hours of battery life remaining on the S-IVB.
006:28:47 Cernan: Hello, Houston; how do you read CDR?
006:28:52 Overmyer: Read you loud and clear, Gene.
006:28:55 Cernan: Okay.
006:29:31 Schmitt: Bob, LMP's going off the air for a little while.
006:29:34 Overmyer: Roger, Jack.
006:29:39 Schmitt: It sounded like a sigh of relief.
006:29:41 Overmyer: No, sir. Been enjoying listening to you; keeping - keep me awake down here.
006:29:48 Schmitt: You had a long day.
006:29:49 Overmyer: Not as long as you've had.
006:29:52 Schmitt: I've just been lying around, floating around.
006:29:56 Overmyer: You make it sound so good.
006:30:00 Schmitt: Piece of cake. I'll talk to you in a little while.
006:30:05 Overmyer: Yes, sir.
Long comm break.
006:33:26 - This is Apollo Control at 6 hours, 34 minutes. Apollo 17, now 26,553 nautical miles [49,176 km] from Earth; velocity, 11,606 feet per second [3,538 m/s].
006:39:55 Evans: Houston, Apollo 17.
006:40:00 Overmyer: Go ahead, Ron.
006:40:03 Evans: Okay; we had another Master Alarm, and I just glanced up and it was the Main A Undervolt light that was on, just for a second.
006:40:18 Overmyer: Okay. Ron, we didn't see anything at all on Main A down here. We did have an Accumulator cycle again. Don't know if that ties in or not.
006:40:28 Evans: Well, the Main A Undervolt - I just happened to be looking right at the panel and the Main A Undervolt light blinked on for a second. And, of course, obviously, Main A is up now.
006:40:45 Overmyer: Roger.
006:41:45 Overmyer: Ron, Houston here. We've checked the back room and the high-speed charts and that and don't see any glitch on Main A at all on our data down here.
006:41:57 Cernan: Okay, Bob.
Very long comm break.
006:48:59 - This is Apollo Control. It's 6 hours, 49 minutes. Apollo 17 is 28,232 nautical miles [52,286 km] from Earth; velocity, 11,291 feet per second [3,441 m/s]. We're continuing to operate at present on the normal GET of the Flight Plan, normal Ground Elapsed Time. Under that schedule the crew's rest period will begin about 9 hours and 15 minutes into the mission. If, however, the crew completes the activities that are scheduled in the Flight Plan early, the rest period will probably begin early if they so desire. However, at the present time we are continuing to operate on the GET of the Flight Plan. At 6 hours 50 minutes, this is Mission Control, Houston.
007:06:58 - This is Apollo Control at 7 hours, 7 minutes. Apollo 17 has just passed the 30,000-[nautical-]mile [55,560-km] mark on its journey to the Moon. Now, at 30,039 nautical miles [55,632 km], velocity continuing to decrease now 10,932 feet per second [3,332 m/s].
007:10:10 Evans: Houston, 17. That was O2 Flow, High.
007:10:14 Overmyer: Roger. We copied that one. We saw it. Just about ready to call you when you called us just now.
007:10:23 Evans: Okay. Mighty fine.
Very long comm break.
007:14:51 - This is Apollo Control at 7 hours, 15 minutes. Astronaut Bob Parker is now relieving Astronaut Bob Overmyer at the CapCom console and the commander of the backup crew, Captain John Young, has just left the control room. He has been sitting at the CapCom console with Overmyer since returning from the Cape early this morning. So the next CapCom voice you will hear will be that of Bob Parker.
007:34:01 - This is Apollo Control at 7 hours, 34 minutes. Apollo 17 now 32,697 nautical miles [60,555 km] from Earth; velocity, 10,457 feet per second [3,187 m/s]. The crew a little over midway in the scheduled meal period in the Flight Plan.
007:49:58 Schmitt: Houston, 17.
007:49:59 Parker: Roger. Go 17.
007:50:03 Schmitt: That little Master Alarm there, I can't be absolutely positive, but out of the corner of my eye, I think it was the Suit Compressor light that glitched.
007:50:15 Parker: Okay. We copy that. You - we believe down here it was the High O2 Flow.
007:50:22 Schmitt: Well, they're pretty close. I thought it was red and I thought, okay; that's good. That's the right time, I guess.
007:50:29 Parker: Okay; because we'd just called it out. I was just read for you 5 seconds before you called me.
007:50:36 Schmitt: Very good, Doctor.
007:50:39 Parker: Roger. And Stoney is back in Houston on the console.
007:50:42 Schmitt: That's hard to believe. What are you doing back here? We're - we haven't even had time to go to sleep.
007:50:46 Parker: Well, I tell you, it's a tale that's hard to believe. It's almost as miraculous as your escape from the pad tonight.
007:51:06 Schmitt: Did you enjoy the launch?
007:51:08 Parker: Beautiful.
007:51:20 Schmitt: You've seen one night launch, you've seen them all. Huh, Parker?
007:52:15 Evans: We go to SCS. Okay.
007:52:36 Evans: Never know if this is it or not but we'll try it.
007:52:52 Evans: Dust whipping all over the place. The stars in there...
Comm break.
007:54:33 Evans: [Garble] Yes, let's do it a little better now.
Comm break.
007:56:44 Schmitt: [Garble] Bob, mag November November is 130 now. And I just took another set of Earth pictures.
007:56:57 Parker: Okay. Copy that. November November at 130.
This frame count means that images 22734 to 22736 have just been taken. In these images, Earth appears distinctly less 'full' than it was when the Blue Marble images were taken less than three hours ago. Despite the spacecraft's west to east trajectory, which is taking them away from the Earth-Sun line, Earth's rotation has caught up with them and Africa has turned more into view now as it approaches the sunset terminator. They are still shooting with the 80-mm lens on the Hasselblad but when they return to photographing Earth after their rest period, they will switch to the 250-mm lens.
AS17-148-22734 - Earth at a distance of approximately 63,500 km (based on photo analysis). Africa, South America and Antarctica - JSC scan
AS17-148-22735 - Earth at a distance of approximately 63,500 km (based on photo analysis). Africa, South America and Antarctica - JSC scan
AS17-148-22736 - Earth at a distance of approximately 63,650 km (based on photo analysis). Africa, South America and Antarctica - JSC scan
007:57:07 Evans: And, Houston, 17. You copying the torquing angles now?
007:57:15 Parker: Roger. Stand by.
007:57:21 Parker: Okay. We have them, and you're Go to torque them.
007:57:25 Evans: Okay. I'll torque it at 58:10.
Ron has completed his third realignment of the spacecraft's guidance platform using program 52. For this, the two stars he sighted upon were 4 Achernar (Alpha Eridani) and 7 Menkar (Alpha Ceti). These sightings showed that the platform, which is still aligned to the orientation of the launch pad at the time of launch, had drifted out by -0.134° in X, -0.018° in Y and +0.175° in Z. Ron's sighting accuracy was 0.01°, a comparison between the actual angle between these two stars and the angle that Ron's sightings produced.
007:57:58 - This is Apollo Control at 7 hours, 58 minutes. Ron Evans is realigning the inertial platform that was scheduled on the Flight Plan for 8 hours, 15 minutes. That indicates that they are running 15 to 20 minutes ahead of the Flight Plan. Jack Schmitt is obviously taking some pictures. He gave Bob Parker a report on a film magazine that he was using.
007:59:01 Evans: [Garble] REFSMMAT.
REFSMMAT is an acronym for Reference to a Stable Member Matrix. In simpler terms, it is a numerical definition of an orientation in space, to which the guidance platform should be aligned. It is defined with respect to the celestial sphere around the spacecraft. Having been aligned per the 'launch pad REFSMMAT' thus far in the mission, Ron is going to realign the platform per a new REFSMMAT, one that is appropriate to their intention to continuously roll the spacecraft side-on to the Sun to moderate temperatures across its skin. The data that comprises the REFSMMAT needs to be uplinked into the computer's 2 kilobytes of erasable memory. To achieve this, the crew will throw a switch that gives Mission Control access.
007:59:04 Parker: And, 17, we have a preferred REFSMMAT standing by if you want to give us Accept, and we'll send it up before you do your second P52.
007:59:14 Evans: Okay, you have P00 and Accept now.
007:59:19 Parker: Roger. Understand we have updata. It's coming at you. And, Ron, while we're sending it up to you, we'll also send you an update on the zero trunnion bias, as per the Flight Plan.
007:59:37 Evans: Okay. Mighty fine.
008:00:09 Evans: Somewhere. There it goes.
008:00:32 Evans: There they are, right there.
Long comm break.
008:02:36 Parker: Okay, 17 - Ron, you can go to Block now. You've got your PTC REFSMMAT. You're free to do a P52 option 1 if you want. And, be advised we are suspicious from time to time you may have an open mike there.
008:02:51 Evans: Okay. Thank you, Bob.
Long comm break.
008:10:05 Evans: Okay, Houston. Those are the differences in the gyro torque and I'll torque it - oh, 11, I guess. Eight [garble] 11.
008:10:14 Parker: Okay. Copy that.
Long comm break.
008:12:07 - This is Apollo Control at 8 hours, 12 minutes. Apollo 17 now 36,353 nautical miles [67,326 km] from Earth; velocity, 9,878 feet per second [3,011 m/s].
008:13:32 Parker: Apollo 17, Houston. Over.
008:13:35 Cernan: Go ahead.
008:13:37 Parker: Roger. We've been discussing the question of what your sleep configuration is going to be in terms of headsets or not, particularly with reference to all of these various Master Alarms. And I guess we'd feel better if one of you guys slept with his headset on. We were curious as to what your plans are.
008:14:01 Cernan: Bob, since I've got to wear the biomed anyway, I might just as well go ahead and keep it on.
008:14:07 Parker: Okay. The other option is for us, if we were trying to get hold of you, is to put the Klaxon up. But we're a little - un-in-favor of that, because of the possibility of one of these spurious things waking everybody up that way.
008:14:22 Cernan: Yes, I'll go ahead and keep it on and see how it works out for a while.
008:14:27 Parker: Okay. We copy that. And, when you guys are ready, we have a couple of - we have three items to read up to you, three updates in the Flight Plan.
008:14:52 Schmitt: Okay. Go ahead, Bob.
008:14:53 Parker: Okay. The first's in the Flight Plan itself, and it's the quads for the PTC spinup, and they'll be Alpha and Bravo.
008:15:19 Schmitt: Okay. For PTC spinup, quads Alpha and Bravo.
008:15:24 Parker: All right, we just took that back. It should be Bravo and Delta for spinup; Alpha and Bravo only for damping. Copy Bravo and Delta for spinup; Alpha and Bravo for damping.
There are four packages of thrusters arranged around the Service Module and they are labelled A to D. Each carries four little rocket engines, hence the name 'quads'. To damp the rotational motions of the spacecraft, single thrusters are fired and only those on adjacent quads, A and B will be used. Then when it comes time to execute the spin-up of the spacecraft, opposite pairs of thrusters will be used to minimise any translation forces. Hence the use of quads B and D. Part of teh decision of which quads to use is the need to share out the consumption of each quad's propellant tanks.
008:17:04 Parker: And, 17, if you have that, I have two others. One's the Flight Plan Supplement Book, and the other one is in the G&C Checklist.
008:17:16 Schmitt: Okay. Go with the Supplement.
008:17:18 Parker: Okay. In the Flight Plan Supplement, we have an E-Load update on page 1-43. Say; 1-43 - can give me a call when you get to that page?
008:17:42 Schmitt: Okay, Bob. I'm there.
008:17:44 Parker: Okay. Under line - it's 30704, column Bravo - you'll find currently 33550. And let me give you a word of warning. When we change this, we'll be changing it again around 67 hours. These are primarily due to the launch delay. And we'll give you another GET update of this sort later on. The new number to replace 3...
008:18:15 Schmitt: Bob...
008:18:15 Parker: Go ahead.
008:18:17 Schmitt: Let me get a pencil, please.
008:18:17 Parker: Okay.
008:18:18 Schmitt: I'll use that instead of a pen.
008:18:20 Parker: Okay.
Comm break.
008:19:21 Schmitt: Go ahead.
008:19:22 Parker: Okay. Under - Again, I remind you, 30704 column Bravo, which was 33550, is now 34761. The line just below it, which is 05, also in column Bravo, is 15403. Over.
008:19:51 Schmitt: Okay, Bob. For 30704 Bravo, 34761; and for 31005 Bravo, 15403.
008:20:04 Parker: Okay. Very good. And the next one is in the G&C Checklist under the P37 block data. And to help you find it, that's on page 4-23.
008:20:39 Evans: Okay. Go ahead.
008:20:41 Parker: Okay. On the lift-off plus 15, be the first block. It's 01500, 3893, minus 174, 05756. The second block for lift-off plus 25 is 05 - Pardon me, start over again there; 02500, 6651, minus 175, 05725. Over.
During Earth orbit, the crew were given a block of data to perform a return to Earth manoeuvre at 9 hours if needed. That time is almost past so further similar PADs are read up that also use P37. These refer to ignition times of 15 hours and 25 hours into the mission.
008:21:37 Evans: Okay, Houston; Apollo 17. First one would be 01500, a Delta-V of 3893, minus 174, and GET 400K is 05756. The other one is Tig of 02500, Delta-V of 6651, longitude of minus 175. GET of 400K is 05725.
008:22:14 Parker: Roger. Good readback.
008:22:32 Schmitt: Okay, Bob. This is Jack. I'm going to be moving into the pre-sleep checklist here. Are there any things you want to change or alter in that? Are you ready for the waste - Waste Stowage vent to be closed?
008:22:49 Parker: Roger, 17. We're ready for the vent valve to go closed. Waste Stowage Vent to Closed. And we have no anticipated changes, at the present time, in the Flight Plan, Jack.
008:23:05 Schmitt: Okay, I'm just looking at 1-29 in the pre-sleep checklist and - wondering if there was anything there.
008:23:19 Parker: Stand by, Jack. [Long pause.]
008:24:00 Parker: Okay, 17. For antenna management tonight we'd like you to select Omni Bravo at the current time, and stow the High Gain Antenna. And we'll take care of managing our antennas from here on.
008:24:19 Evans: Okay. We'll give you Omni Bravo and stow the High Gain.
008:24:25 Parker: Okay. [Long pause.]
008:24:53 Parker: And, Jack, we indeed do not have anything to add to the presleep checklist tonight.
008:25:06 Schmitt: Okay. [Pause.]
008:25:14 Schmitt: And - with your concurrence, I'll take the H2 Fans all to Auto now.
008:25:22 Parker: Stand by.
008:25:26 Parker: Roger. We're ready for that. All to Auto.
008:26:28 Parker: Okay, Jack. I guess that you - we're not quite sure what you said or meant there - or what - what it is. In the Flight Plan itself, we want H2 Heaters 1 and 2 to Auto, and we want H2 Fans, on tank 3 only, to Auto. They're three there for H2 tank 3.
008:26:53 Schmitt: Okay. You're teaching me to read carefully early, aren't you?
008:26:57 Parker: We're trying. The 1 and 2 Heaters will be in Auto and 3 Fan will be in Auto.
008:27:04 Schmitt: That's the way it is now, and consider the fans have been cycled.
008:27:08 Parker: Roger.
008:27:12 Schmitt: According to the checklist, you might look at the third line on 1-29, and look at the H2 line on the Flight Plan, and see why I was confused.
008:27:37 Parker: Roger. We were just discussing whether or not there was a fan or fans in each tank.
008:27:44 Schmitt: That ought to keep you awake this morning.
008:27:47 Parker: Going to take something.
008:27:54 Schmitt: What I was really trying to do, Bob, was get out of chlorinating the potable water, but you wouldn't bite.
Comm break.
008:28:14 - This is Apollo Control at 8 hours, 28 minutes. Apollo 17 now 37,832 nautical miles [70,065 km] from Earth; velocity, 9,667 feet per second [2,947 m/s]. Apollo 17 crew in the period now in the Flight Plan where they're making preparations for their rest period. Getting the systems in the proper configuration for a sleep period. The spacecraft has been maneuvered to the Passive Thermal Control or PTC mode - attitude, rather. And just prior to the rest period the crew will spin up the spacecraft for thermal control during the rest period. The spin rate will be slow or approximately 3 revolutions of the spacecraft per hour but it will keep the thermal balance on the spacecraft. At 8 hours, 30 minutes; this is Mission Control, Houston.
008:30:43 Parker: Apollo 17, Houston. Over, Jack.
008:30:48 Schmitt: Go ahead. Over, Bob.
008:30:50 Parker: Okay. We're going to give you a little High Gain Antenna practice here. We'd like to pick up with the High Gain Antenna again so that we can get your PTC or can watch your PTC develop. We'd like you to go to a Pitch of 40 and Yaw of 275 on the High Gain. That's 40, Pitch: 275, Yaw; and Manual and Wide. Over.
008:31:27 Schmitt: Okay. You want the High Gain selected, I presume.
008:31:29 Parker: That helps, yes.
008:31:33 Schmitt: You got it.
008:31:35 Parker: Roger. Our apologies.
008:31:44 Schmitt: Oh, I don't expect that'll be the last time you have to apologize. I think we're running about even now.
008:32:06 Schmitt: You're missing quite a view, Bob. Sorry you're not here.
008:32:12 Parker: That makes two of us. Weitz just said, 'That makes three of us'.
008:32:31 Schmitt: What are you trying to tell me?
008:32:36 Parker: Look out.
008:32:39 Schmitt: Who's your friend off on your right, tonight?
008:32:45 Parker: Wally Moon, would you believe?
008:32:50 Schmitt: Say again?
008:32:51 Parker: Wally Moon.
008:32:52 Schmitt: Oh, a Moon, huh? Why don't you ask him what he's reading at H2 tank 3 quantity?
008:33:05 Parker: Okay. I'm asking him.
008:33:16 Schmitt: In percent.
008:33:21 Parker: Okay, 17. On tanks 3 of H2, we're reading 84.38.
008:33:30 Schmitt: Okay, it looks like we're reading almost the same nowadays.
008:33:37 Parker: That's good.
008:33:39 Schmitt: I thought we launched a little bias, but I guess that's gone now. We're a little higher than that.
Comm break.
008:35:27 Parker: And, 17, Houston. We're seeing your rates are quite low enough to start the spinup to PTC.
008:35:45 Evans: Okay. We'll see if we can't get it right this time.
Comm break.
008:38:35 Evans: Houston, 17.
008:38:36 Parker: Go ahead, 17.
008:38:38 Evans: Does it make any difference with the plus or minus roll there with the - now that you aren't going to use the High Gain?
008:38:51 Parker: Okay. Well, the Flight Plan says minus roll, why don't we do it that way?
008:38:58 Evans: Oh, okay.
008:39:01 Parker: And after you start the roll, 17, we'd like to go back to Omni Bravo and stow the High Gain.
008:39:09 Evans: Okay.
008:39:11 Parker: We only needed the High Gain to just keep a good check on your rates.
008:39:32 Parker: And, 17, that means stow the High Gain after you - after the startup. We'd like to watch the startup itself.
008:39:40 Schmitt: Okay. I was just going to ask you when.
008:42:20 Parker: Okay, 17 - We're ready for High Gain to stow and select Omni Bravo.
008:42:29 Schmitt: Okay.
Long comm break.
008:49:35 Parker: 17, Houston. We gather you're ready for sleep, almost. One thing we'd like to check at the end here is your O2 heater configuration. Over.
008:49:48 Cernan: Okay. Go ahead, Bob.
008:49:50 Parker: Roger, Gene. Can you give us your O2 heater configuration?
008:49:54 Cernan: Okay. We've got 1 and 2 in Auto, and 3 is Off.
008:50:00 Parker: Okay. We'd like those per the Flight Plan; 1 and 2 to Off, and 3 to Auto.
008:50:08 Cernan: Okay; 1 and 2 to Off and 3 to Auto.
008:50:12 Parker: Okay. And do you have a final change or update on the film status - beyond that 130 that Jack gave us?
008:50:21 Cernan: Stand by 1.
Long comm break.
008:55:05 - This is Apollo Control at 8 hours, 55 minutes. As the crew of Apollo 17 prepares for a 5¾-hours rest period, the spacecraft is 40,165 nautical miles [74,386 km] from Earth; velocity, 9,349 feet per second [2,850 m/s].
008:58:04 Parker: And, 17, your PTC is looking real good so far.
008:58:10 Cernan: Okay. That number on that mag is still 130, Bob.
008:58:13 Parker: Okay. I copy that, Gene.
008:58:16 Evans: And Alpha Alpha, that 16-millimeter mag, is about 25 percent left.
008:58:23 Parker: Okay; copy that as well.
008:58:35 Parker: And I guess as soon as you change the LiOH canister, if you have or haven't, and charge Battery Bravo, then we're ready for you to go to sleep at your leisure. Configuring your comm, remember the Squelch, Enable, and the Voice, Off, when you get ready to go to sleep.
008:59:31 Parker: Roger, Apollo 17. We copy the film update, and we're ready for you to go to sleep once you've got the LiOH canister changed, if you haven't. And remember also the charge on brady - Battery Bravo. After that, it's just the comm configuration, Squelch, Enable, and Voice, Off, when you get ready to go to sleep.
008:59:31 Schmitt: Bob, You're cut in and out. Stand by. We'll talk to you in a minute.
009:00:00 Parker: Okay, I think we're losing an Omni here.
Very long comm break.
From the ALSJ - Nine hours into the mission, they were ready to sleep. Cernan wore a headset in case Houston needed to talk; and he also wore biomedical sensors so that the flight surgeon could watch his heart rate and other vital signs. On this first night, none of them got more than about three hours of sound sleep but, for the next few days, the work load would be relatively light and there would be plenty of time to get adequate rest.
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