You could spend each day of your life staring at a different galaxy, and you’d never even come remotely close to seeing even a tiny percentage of all the galaxies in the Universe. Of course, nobody knows for sure exactly how many galaxies there are. But there might be up to two trillion of them. If you live to be a hundred, that’s only 36,500 galaxies that you’d look at. Puts things in perspective.
But science and astronomy transcend the life-span of any single individual human. Astronomy is a species-wide endeavour. And to serve that endeavour, we keep developing better and better telescopes and technology. One of astronomy’s premier instruments is the Hubble Space Telescope, even after all these years of stalwart observing.
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NGC 4237 is a spiral galaxy, though it’s hard to tell at first glance. It’s actually a specific type of spiral galaxy called a “flocculent” spiral galaxy. Aren’t you glad you looked that word up?
Flocculent basically means “fluffy.”
A flocculent galaxy is one where its spiral arms aren’t easily distinguished. They’re kind of patchy and hard to discern, though they’re definitely there. But it’s not just their surface appearances that captures the interest of astronomers.
Astronomers are mostly interested in NGC 4237’s central bulge. There’s likely a supermassive black hole in there somewhere. There’s evidence that the mass of the black hole is related to the central bulge’s mass, but the relationship isn’t well-understood yet. Astronomers study the central bulge to try and understand how galaxies evolve, and how the central black hole grows over time.
A supermassive black hole (SMBH) can be orders of magnitude more massive than our Sun. Sagittarius A*, the supermassive black hole at the center of the Milky Way, is about 4.31±0.38 million solar masses. Other SMBHs can be billions of solar masses.
There are theories explaining how SMBHs might grow to become so large over time. There’s broad agreement that once a black hole is in place in the center of a galaxy, it can grow through accretion. But exactly where they come from in the first place, and how they shape galactic evolution, are still open questions.