Saturday, October 29, 2005

Naming the moon

I've been told I have a love affair with the moon. And I believe it. Mars comes to its closest approach tonight, in less than an hour from now, and I'm asking my wife what she thinks the moon should be named. She suggests something Japanese.

Actually I did try to take a picture of Mars tonight, during a rare break in the clouds. Results unsatisfactory. More to come later.

In the meantime I've started a thread at the Bad Astronomy and Universe Today forums, asking for suggestions on naming the moon. I'd love to hear your opinion.

And do I have a name for the moon? None. Not yet.

A photograph I took on August 25th, probably the best I have:

Monday, October 17, 2005

Venus at the kitchen window



From earlier tonight.

At the Empire State Building



Saturday, October 15, 2005

Clouds can be nice, too

I saw the sun today after 9 days of clouds, fog and rain here in New York. I can remember longer cloudy periods, but none so intense.



Those were clouds during a sunset in Greenpoint last October. The brilliant red, they tell me, is due to New York's smog.


This was the same scene, more or less, later that month on Thanksgiving morning. Within twenty minutes almost all the clouds had gone.


And this was the full moon the evening of the next day, as seen from Great Barrington, MA. I caught it when it was due East, which tells me that the photo was taken at 7:59 pm, though I have no other way of knowing.

This happened to be the first time I ever saw Titan, the big moon of Saturn. My father-in-law got out his birdscope (magnification of 75x), and the whole family got to see Saturn's rings. It was a terrific evening all around.

Great Barrington was the place where I took a 10-day solitary retreat, shortly before my wedding last year. I was new to astronomy and completely in love with it; I hardly did anything else that week. I wrote 100 pages in my journal about very basic topics, like why and how the sun comes up in a different place every day. I had only brief access to the internet, and I hardly knew any astronomy sites, so I was trying to figure out for myself things that these days I just look up, like the nightly position and identities of Jupiter's moons. I had a birdscope but no telescope, and for much of the time I had no globe of the earth. It was a great experience trying to understand the universe with one's wits and a few instruments. It really gave me a sense of how far our species has come, and how much work was involved -- not to mention mistakes -- in coming to know what we know now.

I got religious about studying the moon's waxing face that week, and clouds were a big deal for me every time they appeared. Two days passed without a glimpse of the moon or anything else, and then this excerpt from my journal:

Great Barrington
June 1, 2004
9:52 pm
In the murky, turbulent, dark clouds I caught patches of strong white light about 20 minutes ago, and I knew the moon was there, well behind its transit of two days ago -- no more than 35 degrees above the SE horizon this time, and nearly turned sideways from my angle. Very eerie scene. At first nothing but white light shone through, and then it would be covered again by clouds, which rolled in all 4 directions and kept opening and closing. Then the moon began shining through, with dark clouds abating but thin and black wisps, or cloudy mists, gliding quickly over the disk.


In my 8x21's I could see the point where Mare Frigoris "spills" its western flank into the Ocean Procellarum, which is now fully visible. To the sea's left, just S of the equator, I could see Grimaldi (crater or sea?), near the western edge of the disk. In the bird scope I could see more, and for a brief moment the clouds revealed a disk so bright that my eye hurt; and many craters, moreover, became hard to distinguish. When the moon is that bright, craters with rays are the most apparent -- Tycho especially. I thought I caught a faintly outlined Longomontanus, while Clavius looks like it's out of view for now, though I can't be certain (and the disk's edge is shimmering as thin clouds pass over). I could also see two craters to the W of Grimaldi (adjacent to it) that are both on my map, though unnamed; on my map there is but a thin sliver not yet revealed.

It's covered now; and nothing else is visible. Not cold tonight at all, and the country is peaceful.

Friday, October 07, 2005

What are planets and moons?

The recent discovery of a planet which has been [nick]named Xena, more distant and larger than Pluto, is stimulating a widespread discussion over the definition of a planet. I've suggested that Pluto should be demoted from the status of a planet, but I find that when I try to define a planet, there is no real need to demote Pluto. I'd like to describe why, but I want to emphasize two things. First I'd like to approach the problem by trying to defining "moon," which is a closely related concept. And I'd like to emphasize the question of time, namely how our categories need to accommodate not just change in our knowledge base as we explore and discover new things, but also dynamic change in the universe.

Let me note right at the start that there are many terms in astronomy which express old concepts but are no longer accurate. We speak of bodies rising and setting. We say that there is a sun and that there are stars, but only in relatively recent times have we started thinking of our sun as another star, or speaking poetically of the stars as other suns.

We speak of the moon, but now we know that our moon is just one among many. Jupiter has four moons, discovered by Galileo, and today we call them the Galilean satellites. When Sputnik launched, we called that satellite the first artificial moon. But increasingly we think of everything in the universe as either bound up gravitationally with other bodies or in actual orbits. The earth, Halley's comet, our sun, and perhaps even the Milky Way galaxy are all satellites of something larger.

Our common sense is that "moons" orbit planets, but since the latter term is ill-defined, I'm not sure we really know anymore what a moon is. But let's say that stars should not be classified as moons. Can we restrict the term "moon" to bodies where gases have never collapsed into nuclear fusion? Jupiter and Earth are two such bodies. So let's restrict the term further to bodies that do not orbit stars or former stars. Well, our Moon orbits the Sun. The latter's gravity acts on the Moon and is enough to keep it, along with Earth, in solar orbit. Astronomers sometimes speak of the Earth and Moon as a double planet system, because they orbit around a focal point located deep inside the Earth, close to the geometrical center of the Earth but not quite there. If the Moon were much larger, the focal point would lie between the surfaces of the two planets: then we would have to decide whether indeed to call them two planets, or to call the more massive one a planet while naming the other a moon. We need to restrict the definition further.

Let me suggest that a moon is a body which orbits a focal point inside the "surface" of at least one body that is non-stellar (by a stellar body I mean an object in which gases are, or once were, igniting in nuclear fusion). If the said focal point lies outside another body's surface or atmosphere (note that the latter's boundaries may have to be defined arbitrarily), then we may speak of a double-body system, rather than a body and its moon.

Suppose that a small body like a comet were to pass by our Moon and be captured into lunar orbit. We would call it a moon of our Moon. The new moon fits the above definition: it is orbiting a focal point inside at least one body that's not a star (it also happens to be in orbit around the earth, and in an orbit around the sun). The original moon retains its status as a moon, because it continues to fit the definition. A capture, unless it changes the original body in some drastic way, should not change the definition of that body. Now, the earth will have two moons: unless drastically changed, Earth will retain its definition, whatever that may be. But Earth will not be called a moon, because it does not orbit at least one non-stellar body. Its primary orbit is around a stellar body. Is that the definition of a planet? That it orbits primarily a stellar body? I think it is, so long as the orbiting body is not itself a stellar object. But I'd like to get at this by exploring one more issue: change.

A capture of an asteroid or comet seems like an unlikely event. But in the early solar system, such events probably occurred. Mars and the gas giants seem all to have captured smaller bodies at undetermined moments in solar system history. We hear today of asteroids passing "dangerously" close to the Earth-Moon system (we even think our moon formed from a collision of a former planet with earth), and though our aged and stable solar system may not be producing captures and collisions now, there is nothing in the law of physics preventing such a thing. There is much perhaps in our models of solar system formation that would argue against the probability of such a thing, but there are many solar systems in our galaxy, all of which will probably challenge our models of how solar systems form.

And even if we stick with our own, let's look at the big picture. In the early years, planets, moons, comets and all the rest were moving around in a riotous roullette; and when the sun begins expanding a few billion years from now, much of the current stability will again be disturbed. The histories of solar systems may contain, what is to our minds, long periods of unstable conditions in which it is not possible to say which bodies are the planets, how many moons they have, which bodies still retain large masses of gas and which ones are "terrestrial", etc. Orbits and masses are variable for much of the life of a solar system.

I think we'd be better off speaking of planets that are currently of a certain class or type: this planet over here currently has its gases and looks like a gas giant; that one over there retains gases but is in an elliptical orbit, and looks like a comet-type planet; another is a terrestrial-type planet with some gases; these others are irregularly shaped planets, of the asteroid-type; still others are Kuiper-type planets; and finally there are what we call Moon-type planets, orbiting not the star primarily but another planet. And for all of these we say, "currently", or "now."

The issue of change seems critical to me because our short lives, and our short history on the earth, makes the universe appear static to us, when actually it is not. It is alive with constant activity, much of it unstable or nascent -- and our stable conditions at this point in time, in this corner of space, make us still less aware of the universe's essentially dynamic character.

A planet much larger than Jupiter might live what we would consider a long time, several million years perhaps, before igniting into a sun. What we called its moons, if it had any, would cease to be moon-type planets (i.e., planets orbiting other planets), and would then become planets of another kind, depending on what the stellar fusion did to them (it could destroy them).

Other factors have restricted our vision of what planets are. Early in human history we saw only lights in the sky and called them stars, with some of them marked off as wandering stars, or planets. Modern science revealed that these wanderers were worlds of great size, comparable to our own world. But we have not seen them in their full glory -- or rather, we have only begun to see them as great, fascinating worlds. Until very recent human history, other planets, and even our Moon, have not pressed upon our consciousness as anything more than lights larger than the stars; they were reputed to be much more, but the details have been slow in coming. Earth-based photographs have started to change our impressions, as have visits by planetary probes; and critically, so have the photos from Hubble. Meanwhile, ground-based telescopes have gotten larger, and more accessible. Now we're starting to realize that all these bodies, even little asteroids and comets, are worlds of size and great interest. And when we visit them personally, our consciousness will regard them with greater equality, as non-stellar worlds.

The more I regard and study the Moon, the more I tend to think of it as a planet. It switches places with Earth twice every month as the third rock from the sun. It is sometimes called a failed planet, but it only failed to become an Earth-type planet. It is quite a massive world when seen in some of the best composites of Apollo photographs from the lunar surface; and it is an interesting world with the same planetary structure (core, mantle, crust) as Earth, and a similar historical process (up to a point). The Moon once had flowing lava and an atmosphere: at one time we may have had to include such a world in a different category of planet, closer to ours. Planets, even in a stable solar system, evolve enough to change categories -- or to push us to change our categories.

In sum, a moon is any object which orbits a non-stellar body; a planet is any object, but not a star, which orbits a stellar body.

Thursday, October 06, 2005

Morning Moon Conjunction


This is the photo now appearing in Night Sky magazine. Venus and Jupiter are near the moon, with Jupiter closer. I took it last November 9 at dawn, from our roof in Greenpoint. I wrote very little in my observation journal:

November 9, 2004
7:02 a.m. (26 minutes past sunrise)
Our moon arrived at Jupiter today, so close (just half my 9x63 aperture) that no Galilean satellites were visible (they were IG/CE). Venus and Jupiter now take up almost a full length of my aperture. This is the closest that the moon will get to either planet this month (1.5 degrees perhaps). I took many photos, most from my window, and ventured for only 2 or 3 minutes onto the roof, so cold has it become. Very beautiful sight.

Wednesday, October 05, 2005

The Spider and the Fly


This fly was a resident of Great Barrington, MA when I photographed it. It lay very still for its portrait, and we wondered if it was dead, but it did fly away after a minute or two. Maybe it was on its last legs.


That's the full photo. Compare with the photo below, which appears in Michael Light's coffetable book, Full Moon.


That's the lunar module Challenger, sitting on the moon in December 1972, during the last of the moon missions, Apollo 17. Geologist Jack Schmitt took this picture with a 500-mm lens while almost 2 miles away from Challenger, which is about 23 feet high. The mountain in the background, the South Massif, of which we can see two white slopes rising steeply, is another 5 miles back. Even the darker embankment between Challenger and the white slopes lies nearly 4 miles behind the lunar module!

The remains of Challenger are still sitting there in the Taurus-Littrow Valley, which was formed when a large meteor struck the moon nearly 4 billion years ago and left mountains on all sides.

The photo captures the full width of the valley. I downloaded it from a website that has a great archive of Apollo photos. On the web there's also a 360-degree panorama of the valley.

Below is a photo of the valley from lunar orbit. I've marked off the spot where Challenger later landed (near the middle of the plain), and the spot where the photo above was taken (at the foot of the mountains to the right).



The first lunar module produced, for Apollo 9, was nicknamed Spider. The most famous of the spiders was the Eagle, seen here with Buzz Aldrin.

Now have a close look at the next photo, from yet another mission.

This is David Scott, the commander of Apollo 15, in the summer of 1971. The mountains behind him, known as the Swann range, are 10 and 1/2 miles away.

The distances in these photos are so deceptive, as the astronauts reported experiencing during their visits. It makes the Apollo photos doubly interesting; you don't know exactly what you're seeing, at first sight. Before reading Michael Light's book, I had always assumed the mountains in Apollo photos were hills. But there are no familiar objects on the moon to give a sense of perspective.

A few weeks ago I was showing my 9-year-old nephew some Apollo photos. I explained that if you were to look at a mountain on earth, you would see valleys, rivers, forests, roads, and perhaps clouds in front of it. That's how you'd know that the mountain was very distant. Remove all those things, and there's no way to know. You could make your way toward an apparent hill and find yourself walking a very long time. The plain in front of you would open up endlessly, tirelessly offering up craters and boulders, and more ground, until you arrived at the base of a 15,000 foot mountain.

I remember being deceived by distances in the Sinai desert, where there are comparatively few objects to give perspective -- fewer than in the American Southwest, which is less deceptive. But the Moon must be something else.