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Wednesday, 18 January 2017

The Universe in 101 words: Could we see back in time?




One type of time travel that happens daily is seeing into the past: Light’s speed is limited, so the Universe is full of images from distant eras. A couple of everyday examples are:


  • We see the Moon as it was 1.5 seconds ago. 
  • We see the Sun as it was eight minutes ago.
  • We stars as they were up to 13 billionyears ago.


So here’s a thought: If we could locate a huge reflective surface 32.5 million light years away*, and focus an incredibly powerful telescope on it, we could see the dinosaurs.

Although watching Jurassic park would be simpler...

*32.5 million yars for the image of Earth to reach it, and 32.5 million years for the light to be reflected back  equals 65 million years.

 

Monday, 16 January 2017

The Universe in 101 words: What's lightening like on Jupiter?

Above: Jupiter - still owning it.
The biggest lightening storms are found on Jupiter, the biggest planet in our solar system. 

Well, I guess that makes sense. 

Jupiter's bolts are ten times more powerful than terrestrial bolts. With no surface they simply strike within the clouds, like sheet lightening on Earth - so you'd seldom see the whole bolt, just a diffuse flash. They spring from Jupiter's water cloud layer, below its clouds of ammonia. 

Below the clouds the hydrogen atmosphere gets hotter and thicker, becoming an ocean of ‘supercritical fluid. Over that 'ocean' the clouds form an immense roof, punctuated by the lightening...


Wednesday, 11 January 2017

The Universe in 101 words: Could anything live in Venus' clouds?

Are you looking for a  gift with a difference? How about art by a mad scientist?
 

Although it's named after the brand of skincare products*, Venus'  clouds would remove your face, not moisturise it – they’re made of sulphuric acid, and punctuated by lightning

But that might not stop exotic microbes calling them home: In principle life might use sulphuric acid instead of water, and on Earth some microbes live in cloud droplets. Venus' endless yellow-white cloudscape has mysterious chemical imbalances, and strange UV absorbing pattern in it

Could these be signs of microbes floating in the relatively Earth-like layer between the blue sky, acid rain, and scalding surface? We can't say, but unless we explore those clouds...

*Yes, that's a joke. They're actually both named after Venus Williams, who was named after the brand of razors (citation needed).

Saturday, 7 January 2017

What is the Milky Way? And how is pizza involved?

Are you looking for a  gift with a difference? How about art by a mad scientist?
 


Given how many people live in and around cities these days, you may not have seen this:

Image courtesy of Stephane Guisard

I mean the Milky Way not the cactus.

The reason why a lot of people won't have seen it (including me - at least for a while) is that it doesn't really look anything like that bright. That picture is taken with a camera that was left to gather light for minutes or hours, turning a faint band of fuzz running across the sky into a glistening river of starlight.

To see anything like that picture you'll have to go well away from civilisations lights - then, in night sky, you'll see a band of stars. If you went into space, well away from Earth and the Sun**, you'd see that band actually running all the way around the sky. 

But, even if you did, the Milky Way still wouldn't be giving you the whole story.
 
It looks like a band of stars, but it’s actually a disk of them – it's a galaxy, a two hundred thousand light year wide disk of stars. The reason why it looks like a band running across the night sky is that we’re inside the disk – Earth is located about two thirds of the way from the middle, which it circles every 250 million years. 

Above: A map of the Milky way, showing the position of Earth.

Not convinced? To get a visual and tasty idea of how this works, cook yourself an extra large pizza. 

If you have no pizza in this is an excellent opportunity to order a take away pizza – tell your waistline a mad scientist made you do it – but ask them not to slice it. 

Once you have your large pizza take it into the kitchen*. Now slice out some of the pizza – enough that you can get a camera, iphone, or your head, inside the pizza. I’d go for a couple of traditionally shaped wedges taken centre to rim, but if you’re hell bent on scientific accuracy (and a monster) you could slice an appropriately sized circular chunk out, centred on a spot two thirds from the middle. Take the remaining pizza, and put your image-making thing inside the gap in the pizza. 

A cat is not an imaging device, although this is hilarious.

If you are using your own eyes and went for the scientifically accurate circular chunk removed two thirds from the centre... you are probably now wearing the pizza on your head. But as funny as that is it doesn’t affect the outcome.

Anyway, get your eyes or lens precisely on the level of the pizza, and take a picture (or just look through the scalding sauce now dripping onto your face): You can see that the disk shaped pizza is a band stretching across the 'scamera picture. 

Now imagine that your pizza is two hundred thousand light years wide and faintly glowing, and you’ll understand how the gigantic, disk shaped Milky Way galaxy can look like a band of light. 

You also have a fair bit of mess, but at last you have (slightly mutilated but hopefully still edible ) pizza. 

* This is not actually necessary, but ...I'd recommend it. 
**When I say get away from cities... that's a bit excessive, but you could.

Sunday, 1 January 2017

Answers for Authors: What's the view like from other parts of our galaxy?

Are you looking for a  gift with a difference? How about art by a mad scientist?
 


To answer this we first need a quick bit of galactic geography:
Go out on a really dark, clear, night, far from any artificial lights, give your eyes time to adapt to the darkness, and look up. You will probably see many more stars than you’re used to and, stretching across the sky from horizon to horizon, a long band of faintly lowing fuzziness: That's the Milky Way, the galaxy that our Sun, our solar system, and this planet are part of.
 
This thing - although this is a long exposure that intensifies the light in the image. It doesn't look much like a swirl of stars from Earth, as we're inside the disk

It’s a collection of hundreds of billions of stars, at least that many planets, comets, nebula, and much weirder things with names like ‘magnetars’, ‘pulsars’, ‘white dwarfs’ that sound like they came straight out of an early draft of superhero comic. It's actually shaped like the swirl of cream in a coffee mug - and we can divide it into three bits:

  • The central bulge / galactic core: The centre of the swirl, the core is made of a mix of stars of all ages. It's also one of the oldest neighbourhoods, and has both a lot of old stars and clusters of very young stars, and gas clouds primed for new star growth. Everything is very close packed (less than half a light year between stars on average, often much closer). The bulge is about 5,000 light years in radius, and has at least two gigantic black holes in the centre, one of which is the supermassive Sagittarius A* black hole, our galaxy's central black hole which weighs as much as 4,300,000 Suns. 
  • The disc/arms: The arms of the swirl. About 60,000 light years in radius, and around 1,000 light years deep where the Sun is, it's mainly made of young to middle age stars. Beyond the edge of the disk is a mysterious ring of stars and gas surrounding it, with a radius of 75,000 to 80,000 light years, called the Monocerous ring
  • The galactic halo: This is where my coffee metaphor runs out completely, unless you’ve brewed your coffee in weightlessness and then spilled it – these are, well, wispy bits outside the main galaxy. They are made of widely spaced gas and stars, floating above or below the plane of the disk in a rough ball, stretching to a radius of 130,000 lightyears. Although the stars and gas are incredibly sparse there, set within the halo are locales called globular clusters: Round clusters of hundreds of thousands of ancient stars, which are often separated from each by less than the width of our solar system.
Let’s assume I’ve got a ship fast enough, and well supplied enough, to go around the galaxy and stop in each section. What would my human eye see? 

The galactic disk: 
A map of the galactic disk, showing the spiral arms. Courtesy of Universe Today.

The nice thing about figuring out the view from the galactic disk is I live in it: Earth is located in the 'Orion spur' - a sub arm of the disk about 25,000 light years from the galactic centre. So there's lots of information to go on...

After my eyes have some time to adjust to the darkness the Milky way is a rough, very broad, band of faintly glowing fuzz stretching across the sky. In the direction of the constellation Sagittarius I can see a bulge in the band, with dark gaps in it - that's the direction of the galactic core. The gaps are dark nebula, blocking light from that direction out. 
I can't actually see the galactic core - there's too much gas, dust,and intervening stars in the way. What I see is the result of the disk getting slightly thicker in that direction.
If I look about with care I see the occasional dim fuzzy blob of a star forming nebula (like the one on Orion’s belt), and glittering collections of blue stars - open clusters

Above: The Pleiades, a cluster of young stars still wearing the remains of the nebula that created them.

The stunning colours I've seen in pictures from space telescopes are nowhere to be seen because, well, my eye isn't a space telescope. But it's good enough to make out some things: Above and below the plane of the galaxy I can see the Magellanic Clouds - smaller galaxies that orbit the Milky Way - as broader fuzzy patches well away from the galactic centre.


The galactic centre: 
Above: Incredibly densely clustered stars near the galactic core, Courtesy of the European Southern Observatory.
The stars of the core are densely packed, often living within fractions of a light year of each other, and many of the biggest and brightest are either huge, ancient, red stars or clusters of equally bright, young blue ones. The bright, close clustered, stars around me stop anything outside the galactic centre being  visible - the core seems to be the whole universe.

The sky is much, much brighter than on Earth: A lot of these stars are as bright as Venus from Earth – some are as bright as a full moon all by themselves. How bright is that in total? It’s very had to tell exactly, because clouds of gas and dust keep us from getting a really good count and the brightest stars wash out the fainter ones… but a back of the envelope calculation suggests the sky would glow with at least 1/300 the the brightness of the Sun from Earth**.

If that doesn’t sound so bright – the full Moon is juist 1/400,000 the as bright as the Sun, so the sky in the galactic core would be over a thousand times brighter than the full moon. Switching the lights off on my spaceship would still leave me with the equivalent light of bright sunset.

But!

If I head deeper into the core, eventually I come to the heart of darkness: Sagittarius A*, the 4.3 million solar mass black hole our galaxy is centred on. The vast black hole is 'only' as wide across as the orbit of the planet Mercury, but for half a lightyear around it is a swirling doughnut of superhot gas that X-ray telescopes can pick up even from Earth -
the graveyard of stars and planets that passed too close to the hole.

The galactic halo: 
Above: The Andromeda galaxy, in a long exposure photograph that brings out otherwise invisible details. Our galaxy might look similar, from outside. Courtesy of Brian Snyder.
The galactic halo is pretty lonely place. I’m well outside the galactic bulge and the disk, which are stretched out below me. 


I might have expected to see something like a celestial fried egg in an infinite black frying pan - but then I’m not remembering the view from Earth: There the galaxy is a dim fuzzy band across the night sky, even though I was looking lengthwise through it, with all the accumulated light of the  galaxy on my line of sight. Up here, looking down on the relatively thin galactic disk from a great distance, the only part that is very bright to the human eye is the galactic central bulge: A twinkling, fuzzy edged, blob of a billion stars – from here it’s easily brighter than the full Moon

Around it is an ethereal, almost invisible swirl of mist. That’s the galactic disk. You don’t need to take my word that it would be virtually see through: The Andromeda galaxy, that is regularly in the night sky from most locations, and it’s bigger than a full Moon. 

Ever seen it hanging in the sky

Above: The Andromeda galaxy, in a long exposure shot that makes it's outer regions brighter, and easier to see. Courtesy of Ted Van.
Probably not – even through a telescope, the only really visible bit is it’s galactic core. The spiral arms are vast, but too thin for our eyes to really make out.  

That said, it’s a dark sky out here: Rather than being separated by five or six light years, as in the spiral arms, the stars out here are separated by hundreds or thousands of light years. For that reason, if you turn so the bright core is behind you, it’s possible to dimly make out the structure of the spiral arms. Other galaxies are also more visible than from Earth, even through the disk of the Milky Way.

Globular cluster: 
A globular cluster - a vast ball of ancient, close packed stars.
 The last stop on our galactic whistle stop tour: These are huge collections of ancient, red stars floating in the galactic halo. Mostly they're located in a shell around the galactic core - and the stars are, if anything, even more tightly packed – big, bright old stars, dating from when the rest of the galaxy was just a huge cloud of gas. I can't
see much outside of the cluster, except maybe the galactic core. 
Although this place is as bright as the core, the quality of the light is different: Orange-white, as every star is an ancient red giant or dwarf.
The close stellar quarters means that any planets will have been stripped away from their solar systems - not that there will have been many: Globular clusters are incredibly poor in heavier, planet forming, elements. This is a place where no new stars have been formed for billions of years - in many ways it's a tiny, zombie galaxy in it's own right.

And, finally, I can turn and head back to Earth. Hopefully I didn't leave the oven on... 

**The back-of-an-envelope calculation went: The very central cubic parsec (1 parsec = 3.26 lightyears) of our galaxy is estimated to contain 10,000,000 stars. To get a rough lower limit for how bright that would be, lets assume all those stars are as bright as the Sun (in reality many of them are far, far brighter), and arrange them in a sphere with a radius of 0.825 light years - the average distance from the centre assuming the stars are evenly spaced. Earth is 8 light minutes – 0.000015 of a light year, from the Sun. That means our hypothetical stars are each 55000 times further away from the centre of the sphere than the Sun is from Earth. Luminous intensity decreases with the square of distance, so each of those stars is delivering 1/ 3,025,000,000th of the Sun’s intensity at Earth. Multiplied by 10,000,000 that givs a total brightness, across the whole sky, of 1/302th the brightness of the Sun from Earth.

Saturday, 31 December 2016

6 stunning images from the International Space Station



Are you looking for a  gift with a difference? How about art by a mad scientist?
 
The International Space Station: A  football field sized orbiting laboratory - also home away from home, a port for spaceships from many nations, and even a tourist destination....


The ISS crew have a busy schedule, but not a nonstop one - it does allow a certain amount of time casually lounging by the window and looking at the Earth - as demonstrated by Tracey Caldwell Dyson here.



Although it does a lot of pure science experiments, the ISS is also a test bed for new technologies, and new in space construction methods. In this shot one of the crew floats in the middle of the BEAM habitat, an experimental kind of room for space stations that is flown up folded, and inflated to full size in space.


 
To lay the foundations for future missions, and to give the crew's diet a bit of variety, the ISS crew grow vegetables in hydroponic bays. Kjel Lindgren shows off a crop of Red Romaine lettuce for the camera.

 
If you're going to play the guitar in a space station you'd better be able to play a selection everyone likes, or you may see it go floating past your bedroom window  one day



In the background a Dragon supply ship is  being brought into dock using the space station's crane like robotic arm. In the foreground... what can I say apart from: If you've got a dream....



This picture is emblematic of the perils the crew face: This innocuous mark is a crack in one of the stations quadruple  glazed windows. It was probably caused by something smaller than a fleck of paint, but travelling many times faster than a bullet.


A space shuttle moves in to dock with the station, as both a silhouetted against the Sun in this amazing photograph by
Thierry Legault.