“Let the great world spin for ever down the ringing grooves of change.” -Alfred Lord Tennyson
Welcome back, for another Messier Monday here on Starts With A Bang! Each Monday, we’ve been taking a look at one of the 110 Deep-Sky Objects that make up the Messier catalogue, a mix of clusters, nebulae, galaxies and more, all visible from most locations on Earth with even the most basic of astronomical equipment.
When you think of our local group of galaxies, you probably think of the Milky Way and Andromeda, and then “everything else” as an afterthought. I can hardly blame you for that; at only 2.5 million light years, it’s the biggest, brightest extended object in the night sky. With an estimated one trillion stars, it’s the biggest galaxy in our neighborhood, followed by the Milky Way at number 2.
But did you ever wonder what the third largest galaxy in our neighborhood is?
Believe it or not, there’s another galaxy within our local group that’s actually (barely) visible to the naked eye: the Triangulum Galaxy, also known as Messier 33. Here’s how to find it, but only on nights where there’s low light pollution. (I.e., not tonight, when there’s a full moon!)
Early in the night, the bright clusters Hyades (highlighted by Aldebaran) and Pleiades are prominent, with Jupiter presently between the two. If you draw an imaginary line connecting Aldebaran to the Pleiades and continue, it will take you across the sky towards the bright star Mirach (in the constellation of Andromeda), not so far away from the bright “pair” Hamal and Sheratan (in Aries).
But the small constellation Triangulum is found in there, and practically midway between the Hamal/Sheratan pair and Mirach is a very faint object just barely visible to the naked eye. It’s the only Messier object in this constellation, and whether you can see it or not is a great test of how dark your skies are.
In skies darker than the suburban/rural transition (a “4″ or lower on the Bortle scale), you’ve got a great shot at finding it! Through a good pair of astronomy binoculars, a small “ring” of five stars appears to encircle this deep-sky object, and — although it will be mind-numbingly faint — you’ll never forget it if it appears for you.
Why’s that? This is a real “small wonder” of a galaxy. With just 40 billion stars, it’s only 10% as massive as our Milky Way, but appears as the second-brightest galaxy in the sky because it’s so close! At just 2.8 million light-years distant and inclined at 54° to our line-of-sight, it gives us the best “face-on” view of any close galaxy!
The only drawback is that it’s so close that low-magnification viewing is practically a necessity! But if you build up your observations over long enough time periods, you can develop a clear, spectacular view of our next-door neighbor!
Because it’s so close, we’ve not only seen some spectacular views of M33, we’ve also learned a ridiculous amount about astronomy from it. There are the red areas, which are indicative of star-forming, ionized regions of space, sweeping spiral arms, along with billions and billions of stars.
The many variable stars in this galaxy are well-studied enough that our figure of 2.8 million light-years is pretty robust for its distance.
It’s over 40 times as large and 6000 times as bright as the Orion Nebula, with about 200 prime candidates for a spectacular Type II supernova! If this star-forming region were located in our neighborhood of the Milky Way, it would outshine every star and planet in the night sky.
But — as is often the case — there’s a ton to be learned from looking in a multitude of wavelengths.
From the visible light images, we learn that there’s practically no bar in the center of this galaxy, and from the motions of individual stars, we also learn that there’s no supermassive black hole in there, either. In fact, if there is a massive black hole, it’s less than
three thousand 1,500 solar masses, whereas supermassive black holes normally range from a few million to many billions of solar masses.
But there are some amazing things happening.
The Spitzer Space Telescope shows us this galaxy in the infrared, and highlights extended dust far past where the spiral arms are. Reconstruction of faint IR signatures shows that there was once a gravitational encounter between M33 and the great Andromeda galaxy, and we now think that ourselves, Andromeda and the Triangulum galaxy will all eventually merge together, with the most probable outcome being a merger of Andromeda and the Triangulum galaxy maybe a billion or two years before the Milky Way-Andromeda merger we’re all looking forward to.
This Ultraviolet view, from GALEX, shows the location of bright, young blue stars, which the Triangulum Galaxy is full of! The spiral arms are clearly traced out in the Ultraviolet, but the central “bulge” that we’re so familiar with in our own galaxy seems absent.
In fact, there is no central bulge in this galaxy, but something fishy is happening in there. And that’s something we only know thanks to our X-ray eyes.
There’s an ultra-luminous X-ray source coming from the center of the Triangulum galaxy, which is the most luminous X-ray source in the entire local group! This sort of X-ray source very close to the center of a galaxy is thought to be extremely rare, and yet, out of the three major galaxies in our local group, there it is.
Unlikely events happen all the time in the Universe, and we have the chance to enjoy one right here in our own backyard.
Including today, we’ve taken a look at the following Messier objects:
- M1, The Crab Nebula: October 22, 2012
- M8, The Lagoon Nebula: November 5, 2012
- M13, The Great Globular Cluster in Hercules: December 31, 2012
- M15, An Ancient Globular Cluster: November 12, 2012
- M30, A Straggling Globular Cluster: November 26, 2012
- M33, The Triangulum Galaxy: February 25, 2013
- M37, A Rich Open Star Cluster: December 3, 2012
- M41, The Dog Star’s Secret Neighbor: January 7, 2013
- M44, The Beehive Cluster / Praesepe: December 24, 2012
- M45, The Pleiades: October 29, 2012
- M48, A Lost-and-Found Star Cluster: February 11, 2013
- M53, The Most Northern Galactic Globular: February 18, 2013
- M60, The Gateway Galaxy to Virgo: February 4, 2013
- M67, Messier’s Oldest Open Cluster: January 14, 2013
- M78, A Reflection Nebula: December 10, 2012
- M81, Bode’s Galaxy: November 19, 2012
- M83, The Southern Pinwheel Galaxy, January 21, 2013
- M97, The Owl Nebula, January 28, 2013
- M102, A Great Galactic Controversy: December 17, 2012
Come back next week for another Messier Monday, where we’ll spotlight our twentieth Messier object since we started this series! And for those of you who want some fantastic international news, Starts With A Bang fan Olaf van Kooten has begun translating our Messier Mondays into Dutch over at astroblogs.nl, because the joys and wonders of the Universe should be freely available for everyone to enjoy!