Spacelog Apollo 11

That's affirmative.

11, Houston. Do you read?

Roger. We read you. It seems to be rather marginal on the high gain.

Roger. We concur.

Houston, Apollo 11. Could you give us a time of crossing the prime meridian 150 west? Over.

Roger. Stand by about a half a second, here. Okay. Your time of crossing the 150 west meridian will be 77 50 05. Over.

Thank you.

11, this is Houston. We have about 6 minutes remaining until LOS, and in order that we may configure our ground lines, we'd like to know if you're still planning to have the TV up with the beginning of the next pass. Over.

Roger, Houston. We'll try to have it ready.

This is Houston. We are inquiring if it is your plan to. Over.

It never was our plan to; but it's in the flight plan, so I guess we'll do it.

Houston. Roger. Out.

11, Houston.

Roger. Go ahead.

For use in connection with the prime meridian crossing, you have an orbital period now of 2 hours 8 minutes and 37 seconds. Over.

Thank you.

Apollo 11, this is Houston. A little over 2 minutes to LOS. All your systems parameters and orbit are looking good from the ground. We have AOS on the other side at 78 23 31. Over.

Roger. 78 23 21.

Roger. That was 31 on the end.

Apollo 11, this is Houston. Over.

This is Apollo 11. Are you picking up our signals okay?

Apollo 11, this is Houston. Affirmative. We are reading you loud and clear on voice and we have a good clear TV picture, a little bright crater in the —

— No, no, no —

— the bottom of the picture. I guess that's the spot on the tube.

I'm sorry about that one.

And if you give us P00 and ACCEPT, we will uplink our new state vector and target load to you.

Okay.

Houston, Apollo 11. One of the larger craters on the back side—I noticed a small, dark speck on the outer wall and I put the monocular on it. I was able to see—oh, an area maybe a quarter of a mile in diameter. It was really a freshlooking dark colored pit, and that seems to be in contrast with all the other fresh little craters or holes that you can perceive on the walls of any of these craters. Around this particular one there seems to be two or three of these—especially the one that caught my attention. Quite remarkable. Over.

Roger. Do you have a location on that one?

No, not a precise one. I've got several pictures of it, though.

Roger. We copy.

We're getting a beautiful picture in down there now, 11. The color's coming in quite clearly, and we can see the horizon and the relative blackness of space, and without getting into the question of grays and browns, it looks, at least on our monitor, sort of a brownish gray.

That's a good, reasonable way of describing it. It appears to me as though it made a difference just sitting back in the tunnel and gazing at all windows; it makes a difference which one you're looking out of. For example, the camera right now is looking out the number 5 window, and it definitely gives a rosier or tanner tinge, especially when you look straight through it and not at an angle. Over.

Roger.

And if you rear back 95 or 100 degrees …

… Still holding … Okay.

Say again, 11?

I'd say we're about 95 degrees east, coming up on Smyth's Sea.

Roger. And for your information, we show you at an altitude of about 92 miles above the surface right now.

Okay.

Houston, Apollo 11. Could you observe a difference in the N₂ pressures before LOI? It seems to me as though the two were not equal on the … B tank was a little low on pressure. Over.

I'm flying it in SPS minimum impulse, Houston, and it's rather difficult to keep it on a constant data. The LM wants to wander up and down. I'm not sure if it's in response to MASCONN's or what, but I can get it completely stabilized in DATA and let it alone, and in another couple of minutes it will have developed its own rate.

This is Houston. Roger.

Houston, we'll be moving shortly from the side window to the hatch window, and we'll try and pick up some of the landmarks that we'll be looking at as we approach the powered descent. Over.

11, this is Houston. Roger. And we're through with the uplinks; the computer is yours. You can go to BLOCK and we'll have the information on nitrogen for you shortly. Over.

Roger. Copy.

Okay, Houston. Several minutes ago I was exactly steady on data, and since then I have been moving toward the LM, pointed straight down toward the radius vector, and that's been despite a number of down minimum pitch impulses.

Roger.

We're about 88 degrees east, I would estimate.

We show you about south of the—southwest of the crater Jansky right now.

Smyth Sea doesn't look much like a sea. It—The area which is devoid of craters, of which there's not very much, is sort of a hilly looking area. It's not like the maria at all.

Roger. We copy that about the sea, and it looks like you were just giving us a view of the crater Neper, the large crater on the left, and Jansky on the right.

We think you're close, but no cigar.

11, this is Houston. Would you care to comment on some of these craters as we go by?

Roger. We're approaching the approach path to ignition. This is equivalent to 13 minutes before ignition, and we're at about 83 degrees, I guess—83 degrees east. That correspond to location you're holding there presently?

Roger. We're showing your present position as about 77—76 degrees east looking back towards the east.

Hey, you should be looking back at Smyth Sea now.

Roger.

Okay.

Houston, what you're seeing in the middle of the screen now is the crater Schubert and Gilbert U is in the center right now; and this comes up at about—a little over 12 minutes before power decent. Instead of me looking—Instead of looking back at it, we'd be looking straight down at it in descent.

Roger.

And we show you at an altitude now of about 110 miles; and, of course, you'll be considerably lower at the initiation of powered descent.

Okay, Houston. Look at register 3 on the DSKY data. This data is increasing toward my desired of 315; and I'll let the hand controller alone here, and I'll bet you it reverses itself.

Roger, 11. We're watching the DSKY now, and it's still coming in beautifully on the TV.

Okay. There's—on the right side of the screen at the present time, there's a triple crater with—with a small crater between the first and second; and the one at the bottom of the screen is Schubert Y. Zoom in; it does have a central peak in Schubert Y. Actually, several of them, and you can observe those plus the rim craters at the bottom of your screen.

Roger. We're seeing the central peak quite clearly now.

Okay. We're zooming in now on a crater called Schubert N. Schubert N, very conical inside walls and the bottom appears to be nearly flat.

Look at data on the DSKY. It's stabilized and is holding steady now.

Roger.

Looking out the window I can see a number of small craters on the bottom of Schubert N.

We're coming up on the Foaming Sea where I'll be doing some P22 marking on a crater of my choice, name of crater, Camp.

Okay. We'll be watching for Neper.

And notice register 3 has reversed itself, and it's heading back the other way now without any pitch thruster firing.

Roger, Mike. We confirm that you've changed the direction of your pitch rate.

Generally speaking —

The crater —

— The tendency seems to be to pull the LM down toward the center of the Moon there as in a gravity gradient experiment.

Roger, 11. We copy —

It may have something to do with MASSCON's or it may —

Roger. We copy …

…

It may have something to do with MASSCON's or it may just be the peculiarity of the DSKY display.

Okay. We've observed the behavior of your DSKY, and I think we've got the data here to work on it. Let us grind around a little while on it, and we'll report back to you, probably in a REV or two.

Okay. Well, in the meantime, I'm going to pitch down toward 315.

Roger.

Three craters—three horizontal craters that you now have in the field of view are immediately underneath the ground track. The right hand is the largest crater that you see, Dubiago P.

Roger. We concur on the identification of that crater.

And we show you coming up on landmark Alfa 1 here shortly.

Roger. Mike's having his first look at Alfa 1 at the present time.

Yea. It's a very bright crater. It's not a large one but an extremely bright one. It looks like a very recent and, I would guess, impact crater with rays streaming out in all directions which should make my—Correction—the Foaming Sea easy to see coming up on it now. Crater Camp is one of the smaller ones out on the—on the floor of the Foaming Sea.

Here we show you over the Sea of Fertility now, and we ought to have Langrenus down south of track a few degrees, about 9 degrees south of track.

Now the crater that's in the center of the screen now is Webb. We'd be looking straight down on it at about 6 minutes before power descent. It has a relatively flat bottom to the crater, and you can see maybe two or three craters that are in the bottom of it on the western wall, the wall that's now nearest the—the camera. Near the bottom of the screen, we can see a dimple crater, just on the outside. And then coming back toward the bottom of the screen and to the left, you can see a series of depressions. It's this type of connected craters that give us most interest to discover why they're in the particular pattern that they're in. I'll zoom the camera in now and try and give you a closer look at it.

Roger. We're observing the dimple crater now. The central peak we can see on the Orbiter photos doesn't seem to stand out very well here.

Well, they're not central peaks. They're depressions in the center.

Roger.

And you'll notice on the pitch thruster activity, I've still—I've put in a dozen minimum impulses in pitchdown, and I'm still far from correcting back to 315.