Here I give you the incredible facts behind some of the most interesting stars, and show you how pick them out for yourself in the sky tonight…
If you cast your eyes into the night sky tonight, all the stars are really just individual point sources of light of different subtle brightness and colours, and all inside our galaxy The Milky Way. Of course all together the stars in the sky make for a pretty fantastic skyscape, but there’s much more to those little points of light than meets the eye. Like in much of astronomy your imagination is valuable, you could never see up close the mind bending size of the red and blue supergiants, or get anywhere close to imagining just what the sunshine is like coming from a star 10,000 times more luminous than our Sun. The stars come in all different sizes, colours, brightness, temperatures, including some that look like one star but is in fact a system of two, or even four stars orbiting each other.
Based on view from UK, approximately 56 degrees north.
That twinkling bright star that always catches your eye, flashing all different colours, red, green, blue. This star is Sirius and well known, also known as “The Dog Star” it is the brightest star in the sky. It lies to the lower left of that famous winter constellation Orion, in its constellation Canis Major. Sirius stands out in the winter and early spring sky twinkling and flashing different colours because its light is distorted as it passes through more thickness of the atmosphere, being a high luminous star so low down in the sky.
This distant sun is putting out the sunshine equivalent to 25 times that of ours, is twice as massive, and is 1.7 times the radius of the Sun. So when you look at the Dog Star in the night sky it looks like the one star, well of course it does. But this relatively nearby sun actually has company with it out in space. The Dog Star has a smaller stellar companion called, wait for it…”The Pup”. The Dog Star known as Sirius A, and its smaller companion Sirius B (The Pup), are a binary star system orbiting every 51 years, with a distance from each other of roughly our Sun to Uranus. I said Sirius is relatively nearby, well yes in cosmic scales it is at a measly 8.6 light years distant, just down the road. The Sirius system qualifies as a neighbour to our own solar sytem, so the light you see from it has taken 8.6 years to cross space and reach you. The Sirius star system is fairly young at only 300 million years at its oldest, so it accomplished nuclear fusion as it formed out of its gas cloud at about the start of the Permian period on Earth. So of course this makes Sirius much younger than the Sun.
Sirius B is a faint companion to the main star, and is a high mass white dwarf, almost equal to the Sun’s mass. This is pretty amazing actually considering that Sirius B has nearly the mass of the Sun all packed into a shining blue ball only the size of planet Earth…and you might know that the Sun is so big it could hold 1.3 million Earths in its volume. Sirius B was originally an even higher mass star than the highly visible Sirius A, but used up all its stellar fuel, bloated up into a red giant star, shed off its outer layers, and left behind the highly dense object astronomers observe today.
Sirius is at magnitude -1.45
Coordinates for Sirius RA 6h, 45m, 42s / DEC -16, 43′, 51″
Where and when…
Tonight Sirius is visible rising from the the south east as darkness falls in its constellation Canis Major, also seen in this map in relation to Orion. Sirius climbs low to the south by the early hours, and moves to the south west by daybreak.
If you look to the constellation of Orion tonight you’ll see a ticking time bomb 520 light years away. Marking the left shoulder of Orion the hunter is the red super giant star Betelgeuse. It stands out, as it’s definitely red looking, and bright.
It’s a colossal star at up to 1,000 times the diameter of the Sun, and shining in visible light a ridiculous 10,000 times brighter. It is violent and unpredictable, it swells and contracts, and sheds vast amounts of material into space in huge plumes.
This monster sun is coming near to the end of its lifetime, has evolved into a red supergiant, and is due to go supernova. Well, due doesn’t really mean next week, although it’s entirely possible, in astronomical terms due could be any time over the next 10,000 years, but Betelgeuse is going to blow that’s for sure.
A supernova is an unimaginably powerful event when the star collapses under its own weight after using up all its fuel. It tears itself apart exploding outwards seeding the cosmos with its elements to form new stars, planets, and maybe life…well it’s exactly how we got here. Supernovae are so bright they can outshine their host galaxy. If (when) Betelgeuse goes kaboom, you won’t have to wait till night time to view it, you’ll be able to see the supernova aftermath in broad daylight.
For a full article dedicated to Betelgeuse, go here “The Red Supergiant Star Betelgeuse”
Betelgeuse is at magnitude 0.45
Coordinates for Betelgeuse RA 5h, 55m, 50s / DEC 7, 24′, 30″
Where and when…
This evening you’ll see the constellation of Orion, with Betelgeuse marking its upper left shoulder rising in the east from mid evening. It then climbs higher in the south during the small hours, before sinking to the south west by daybreak.
The star Arturus is a red giant, 25 times the diameter of the Sun, and travelling at some pace through the Galaxy. If you look low to the north at nightfall you’ll see the unmistakable shape of the Plough, or The Big Dipper, whatever you prefer. If you imagine a line that follows the curve of the handle, you’ll come to a bright orange star 30 degrees from the Plough handle end star.
This is Arcturus, the brightest star in its constellation Bootes, and one of the brightest in the sky. Arcturus was originally a star not unlike the Sun but is further along in its lifetime, as it has now evolved into a red giant. Arcturus has swelled up to a bloated size as it comes to the end of its stellar fuel, and will eventually cast off its outer layers to become a planetary nebula, just as our Sun will do in a few billion years time. Arcturus is emitting about 110 times as much visible light as the Sun, but in infra-red it is even more powerful at around 200 times stronger. This stellar specimen 36.7 light years away is a few thousand degrees cooler than the Sun, and likely much older.
This star is moving at a rapid speed through the galaxy, and in a weird direction. It is travelling at a speed of 122 kilometres per second not in the general direction of all the rest of the stars, gas, and dust, but doing its own thing going perpendicular through the plane of the Milky Way. It has company too, Arcturus is one of about 50 other stars moving in the same way, in a stellar stream called the Arcturus Stream. Streams of stars like this are caused by gravitational tidal forces, stretching and pulling collections of stars from their original formation into long tendrils.
Arcturus is at magnitude -0.04
Where and when…
To find Arcturus follow an imaginary curving line from the handle of the Plough, to a distance of 30 degrees from the handle end star (Alkaid). You’ll come to a bright orange star, this is Arcturus in Bootes
Tonight you’ll see this star moderately low in the north west at nightfall, where it sets in early evening. It then rises from the north east during the small hours and climbs into the daybreak.
Coordinates for Arcturus RA 14h, 16m, 14s /DEC 19, 07′, 24″
If you’ve got an unobstructed north eastern horizon, after dark look low for a bright star and you might see Capella in Auriga. Capella is actually the sixth brightest star in the entire sky. Auriga is between constellations Orion and Perseus along the plane of the Milky Way. Look at Capella and yes it looks like your pretty normal, brighter than average star twinkling away. But all is not what it seems, Capella isn’t one, Capella is four, it is a star system of two binary pairs.
Capella’s clutch of four Suns come in two different flavours, a main pair of large G type stars measuring 12 solar radii…and a pair of faint, cooler red dwarfs. The main pair, and the red dwarfs make two binary pairs orbiting around each other. The main pair are in the same class of stars as our own Sun (G type), and orbit close to one another (100 million kilometres), whereas the red dwarfs lie some distance away. Quite far away in fact, the red dwarfs lie at around 10,000 astronomical units from the main stars, that’s 10,000 times the distance of the Earth from the Sun. Yes, space is big!
The main large pair each weigh in at roughly 2.7 times the mass of the Sun, and kick out 79 times more sunshine. They orbit each other once every 104 days, with about 100 million kilometres between them.
The second pair, being red dwarfs will have a mass of less than half that of the Sun’s. These smaller, cooler stars are the longest lived stars in the universe, so long lived in fact that the cosmos hasn’t even been in existance long enough for any to come to the end of their lives. So no red dwarf star has ever yet been observed to die, as they are slow burning, they really do take their sweet time. Red dwarfs can also emit as little as 1/10,000th the light of the Sun, so any planets in orbit around them need to huddle in close to warm any potential life there.
So there it is, the ‘star’ Capella in Auriga, 42.2 light years from Earth, and a little bit more to it than you might have first thought.
Capella is at magnitude 0.05
Where and when…
Tonight look low north east and you might see Capella climbing from the horizon after night fall. It then climbs high in the east and stays on view all night, moving lower to the west by daybreak.
Coordinates for Capella RA 5h, 17m, 36s / DEC 46, 0′, 37″
If you look high to the south west at night fall you’ll see the fifth brightest star in the sky Vega in constellation Lyra . It lies adjacent to the distinctive shape of the swan of constellation Cygnus. Vega is one of the three bright stars that make up the summer triangle, together with Deneb in Cygnus, and Altair in Aquila. The summer triangle is an imaginary shape drawn between these stars against the celestial sphere, and is high up in the sky for northern latitudes during summer.
Compared to the Sun Vega is much, much younger at only one tenth the age of our own star. That makes Vega under 500 million years old, forming out of its gas cloud into a brand new star, just as complex life was starting to really get its act together on Earth. But Vega is not only younger than the Sun but has also 2.1 times more mass, meaning Vega will also die at a younger age. This is the fate of the larger higher mass stars, they have a brief and often violent life, going through their fuel at a quicker rate. In fact Vega is evolving so fast that it could already be nearing middle age, these heavier stars live fast and die young. Vega at 25.3 light years away is also bigger than our Sun, at over 2.7 times its radius.
All that is very interesting but Vega is doing something else, that you might not expect when you see it sitting there apparently unchanging and motionless in the sky. This star is spinning so fast it’s just under the point of breaking apart, it’s at 93% of that point. Just like how our very own Jupiter bulges out at the equator and squashes at the poles from its fast rotation, so it is the same for Vega. The equator of Vega is racing around at a speed of 274 kilometres per second, and the whole star rotates once on its axis every 12.5 hours. As you look up at the star in the night sky, you’re actually looking down onto its pole, so Vega’s axis of rotation is is pretty much pointing directly at you. This means that from your perspective on Earth if you could actually see it, you’d see Vega’s equatorial bulge. It’s large at a massive 23% increased diameter across its equator, than its poles.
Vega is at magnitude 0.00
Where and when…
Tonight Vega is in the constellation of Lyra high in the south west after dark. It sinks low to the north before daybreak.
Coordinates for Vega RA 18h, 37m, 21s / DEC 38, 47′, 43″
Mizar (and Alcor)
Look up to Ursa Major tonight low in the north after dark, and you’ll find the famous and easily recognisable asterism of the Plough, also known as the Big Dipper. The Plough is not the whole Ursa Major constellation (The Great Bear), but forms only a part of it. Also the seven stars of the Plough are not physically related to each other, but appear to be because of their similar brightness forming the well known shape.
Ok so as you’re looking up at the Plough, see the second star in from the end of the handle? That’s Mizar, at just over 78 light years away. But keep looking and you should see another less bright star pop into view next to it, that’s Alcor at just over 81 light years away…3 light years behind Mizar. So the star Mizar in the Plough handle is actually a double with Alcor. This easy naked eye double was thought to have once been used as a test for good eye sight. If you can see both stars then you’ve got pretty good vision, although spectacular eye sight is not required as most people can pick out both Mizar and Alcor quite easily.
But there’s more to these two stars, more stars in fact. If you look at Mizar through a telescope you’ll see that it itself is actually a binary double system. Bright Mizar has a nearby fainter companion star orbiting around it, Mizar A being the main star, and Mizar B its companion. Stay with me here, as it goes even deeper. Both Mizar A and also its fainter orbiting companion Mizar B even have their own companion stars orbiting around them as well. But these extra stars are so close that they appear as just the one star known as a spectroscopic double. But what about the other star in the main pair, Alcor? Well it was also found that Alcor has a companion, a star also orbiting so close that they just appear as the one, another spectroscopic double. So Mizar, the second star in the Plough handle is in fact really a double, double, double, six suns all gravitationally bound together in a sextuple system. The Mizar star sytem is one of only two six star systems in the whole sky, the other is Castor in the constellation Gemini.
Mizar is at magnitude 2.2
Where and when…
Tonight as darkness falls you’ll see the Plough low in the north after dark. It then climbs very high in the north east up to daybreak.
Coordinates for Mizar RA 13h, 24m, 25s / DEC 54, 51′, 42″
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