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Top 10 Facts About "The Milky Way Galaxy"

Top 10 Facts About "The Milky Way Galaxy"
  1. The Milky Way Is Vast
  2. The Milky Way is an estimated 100,000 light-years in diameter and contains up to 400 billion stars, including our own sun. In spite of such a huge number of stars, the distance between Earth and even our nearest star system Alpha Centauri is vast, and as Douglas Adams pointed out in The Hitchhiker’s Guide to the Galaxy, “Space is Big—Really Big. You don’t know how mind-bogglingly huge space is..” And, of course, he was absolutely correct. Needless to say, comprehending such astronomically large numbers and sizes isn’t easy. Can you imagine 186,282 miles, for instance? Of course you can’t, and yet light travels that far in a single second. Alpha Centauri is 25.6 trillion miles (4.3 light-years) away – good luck imagining that – and to put things into some kind of perspective, if you were to count at a rate of one per second, it would take about 11 and a half days to reach just one million.
  3. Just One Of Many Galaxies
  4. The point being that we’re really not good at large sizes! It isn’t that long ago that we used to think of the stars as light leaks in a black curtain, just a little further than we could reach, and heaven was on the other side. Size is so elusive that it wasn’t until 1923 that Edwin Hubble was finally able to prove that our galaxy was not the whole universe, and that in fact there were hundreds of billions of galaxies beyond our own. Nevertheless, even with the best technology we can currently muster it would take centuries to reach our nearest star. The Space Shuttle, for instance, would take around 165,000 years to reach Alpha Centauri, while the Voyager-1 spacecraft which has now left our solar system will not pass other stars for 40,000 years.
  5. Classified As A Barred Spiral Galaxy
  6. Our galaxy is a spiral armed galaxy, and as is typical for about sixty-seven percent of those, ours is barred. It is suspected that such bars are the consequence of a galaxy drawing gas from the spirals into the heart of the galaxy, but as the density of the bars increase over the millennia their own gravity destroys them resulting in spirals without bars. It seems to be part of a middle-aged spiral galaxy’s normal life cycle to have bars for a while.
  7. Black Hole Located At Its Centre
  8. Of course all this matter heading for the heart of the galaxy has to go somewhere. The oldest star in our galaxy is about 13.82 billion years years old, forming just shortly after the Big Bang, which means a lot of time has passed, and a lot of matter has gone tumbling into the centre of the galaxy. There awaits a supermassive black hole called Sagittarius A, 26,000 light years away from Earth and the source of intense radio waves.
  9. Cannibalizes Other Galaxies
  10. Some spiral galaxies form by brushing past other galaxies. Their gravities shred their globular shapes and leave long trails of stars that wrap around the remaining large bodies of stars. Often that is the end of it, with their relative speeds so high that they will never interact again. Sometimes there is enough attraction between them that they condense to form a single galaxy. While the above instance is not rare, most spirals are explained by one or both of these theories. You can look at them at your own convenience. The Density Wave Theory which explains Saturn’s rings explains some spirals, while the SSPSF model explains many others, but the language and mathematics in the latter may be difficult to digest.
  11. On A Collision Course With Andromeda
  12. Interestingly, two galaxies could pass right through each other and have no collisions despite their billions of stars. In actual fact, that scenario is rather more likely than an actual collision because of the vast distances between objects, which is a bit of a relief since we and the Andromeda Galaxy are headed for a meeting in the far future.
  13. Galactic Year Last 250 Million Years
  14. A galactic year lasts between 225 and 250 million years in our part of the galaxy, since rotation speeds alter depending on location. The best estimate for ourselves appears to be in the 240 million year range, since we’re about two-thirds of the way out on the Orion Arm of our galaxy.
  15. A Star Maker
  16. With between 100 and 400 billion stars in the Milky Way Galaxy, and enough interstellar dust to make 100 billion more, we’re not likely to run out of stars any time soon. There is a distinct advantage to having so many stars. Current theories of stellar formation seem to indicate that most stars will have planets.
  17. Milky Way Could Contains Millions Of Planets
  18. Planets and each sun will have a “Goldilocks” zone. In other words, it’s possible that most stars will have a planet (or two) that will fall in the habitable zone for life where it’s not too cold and not too hot — it’s just right. It could have liquid water, if it’s solid; even if it’s a gas giant it could have water in the atmosphere, so that something organic could float and live, despite the lack of “surface”.
  19. Frank Drake And Alien Civilizations
  20. Drake was a radio astronomer who was intrigued by the notion of extraterrestrial life communicating deliberately (or accidentally) by radio. He set up a conference and created an equation to stimulate discussion among the attendees. It was never intended to represent reality, but to help people consider just what we need to know in order to seek other life in the galaxy. Some elements we know and can compute; others are “best guesses”. Either way, all the equation shows is that there might be hundreds or even thousands of civilizations in our galaxy. But because civilizations rise and fall over time, they don’t all exist at one time. And most will be nomadic or agrarian but not technologically capable. If there are technological civilizations, they should number about 43 (arguable, but as good a guess as any) at this point in galactic evolution. With fairly even but random distribution they are probably about 40+ light years apart. Unless we’re particularly lucky, we probably don’t have a nearby neighbor.