jartsa said:
1: Does an observer, standing on the moon, see a brick, that is falling straight down, to contract?
2: Does an observer, standing on the moon, see a light pulse, that is falling straight down, to contract?
What's your motivation for asking the question?
If you're trying to understand SR better, dragging GR into it isn't really a good way to proceed. You're much better off handling the simpler case in flat space-time where there's no gravity to confuse the issue.
If you're trying to understand GR better, it would be a good idea to sketch exactly how you propose to measure the length of the object remotely. I can warn you in advance that the notion of "distance" in general relativity is ambiguous, mainly due to differing notions of simultaneity. Some people understand the warning, some don't, and I get a bit frustrated trying to explain the problem to those who don't. This is really a SR issue, by the way, but it's an important one to understand before you try to tackle GR.
I can tell you how in general I would go about "setting up" the problem. The first step is to decide what notion of simultaneity you want to use, and why. So I would start by assuming that the moon is the most significant gravitating body, and that we can ignore the Earth. Right away, I can see a possible conflict with your question, perhaps you didn't intend the moon to be the most significant gravitating body? In that case, the issue of how to determine the notion of simultaneity would require some thought. If the moon is the most significant source of gravity, however, there is an obvious way to proceed, that is to use a clock synchronization scheme compatible with "static observers". It's less obvious how to proceed if the moon is not the most significant source of gravity.
Once you have decided on the notion of simultaneity you're going to use, the simplest procedure is to construct a spatial geodesic curve. (Not a space-time geodesic, but a spatial geodesic!). Constructing this geodesic will require you to use the metric induced on your spatial hypersurface by your space-time geometry. Constructing the geodesic will require some knowledge of the geodesic equations, and how to solve them. Solving them directly is usually difficult, and taking advantage of conserved quantities via means of Killing Vectors or some equivalent procedure, is highly recommended.
Next you need to confirm that the problem that you've set up is really one-dimensional. If it is, then you mark on this spatial geodesic curve the position of the front end of the rod, and another mark for the rear end of the rod, "at the same time", according to your notion of simultaneity. If both ends of the object aren't on a single curve, then your problem isn't one dimensional. But let's assume that it is. Then the length along the curve (the spatial geodesic) between the marks on the front and rear will be the "length of the rod".
I'm afraid I can't give an exact formula for the result you'd get if you followed this procedure, I'd actually have to work it. My own view is that the exercise of thinking about what you want to measure is considerably more helpful than going through the detailed calculations of calculating the number. Furthermore, if you don't understand what all the steps I've outlined mean (and some of them might require a certain amount of expertise), just giving you the number won't really accomplish much.