Category Archives: astronomy news

A Distant Starry City

The Lion’s Treasure

The spiral galaxy NGC 3512, as seen by the European Southern Observatory's Very Large Telescope in Chile. The galaxy is about 35 million light-years away and spans an area of space 50,000 light-years across. Courtesy ESO.

I like to look at pictures of galaxies. They always trigger in my mind questions about what kind of life must exist on planets around their stars. Since we’ll likely never know (at least in our lifetimes) about beings in other galaxies, it’s a great way to think about starry empires and the civilizations that support them. As a science person, I look at galaxies and immediately start cataloguing in my mind their structures, which gives me some idea of their evolutionary history— that is, what they went through to get to the shape we see them in—and also how much star-forming activity is occurring in the arms. Galaxies are treasure houses of star formation, star death, and the materials for new stars, planets, and life.

This galaxy, NGC 3521, is what astronomers call a “flocculent” spiral galaxy. That means its spiral arms are fluffy with clouds of gas and they are dotted with star-forming regions.  The areas where new stars are being born are mostly blue in color because of the hot young ultraviolet-bright stars they contain. The reddish areas contain older stars, and the dark lanes are those clouds of gas and dust. There could be stars forming inside those clouds and in a few tens of thousands of years, bright blue splotches will light up more regions of the dust lanes.

The core of this galaxy is really quite compact—meaning tightly bound together. There are likely millions of stars in that little region, and possibly a black hole.  All in all, this is a busy galaxy—bustling with star formation, and with the creation of many stars, very likely it has a population of planets in orbit around some of those stars.  If so, I expect that this treasure of a galaxy in Leo also has some life forms in it—maybe some of them are looking at pictures of our galaxy and wondering the same things about the Milky Way.

Planet or Not…

Pluto Has Moons

The Pluto system. Courtesy STScI/NASA/ESA

That distant world called Pluto has surprised astronomers again, yielding up yet another moon.  Pluto’s largest moon is Charon and was discovered in 1978.  Two more — Nix and Hydra — were found in 2005. The new one, called P4 (for now), is quite small, somewhere between 13 to 34 kilometers across, and small enough that it was probably missed in earlier images of the system taken by Hubble Space Telescope. This latest HST image was taken as part of  a search for ring material around the distant dwarf planet, in support of the New Horizons mission, which is en route to Pluto.

So, how would Pluto, itself a small world like many others in the outer solar system, get moons?  The current thinking is that a collision between Pluto and another world early in the history of the solar system would have flung material out into orbit. Eventually, the pieces and parts would have coalesced back together, forming the family of moons we see today.

When I read this story, the first things I wondered were “Why search for rings around Pluto?”  and “Where would the material for Plutonian ringlets come from?”  A long-ago collision would have provided material for rings, but by now, that material would have been cleared away or coalesced into moons, such as Nix, Hydra, P4 (and maybe even Charon?).  To maintain a ring system, you need a constant source of material being tossed out to space.  At Pluto, that source may well be material “chipped away” from the icy surface by the impacts of tiny micrometeoroids.  That would provide chips of ice to form a faint, thin ring. If it exists, it hasn’t yet been detected. But, HST would be the best instrument we have at this time to find the ring.  Once New Horizons gets there, it may well “see” the ring, if it exists.

I like it when HST finds things like this. It’s a continuing reminder that the venerable telescope has a lot of life in it yet; and will keep surprising astronomers with new finds.