18 amazing facts about space and astronomy
What do lemons and raspberries have to do with space, just how dense is a neutron star and how powerful is a gamma-ray burst?
Space is vast, and filled with weird and wonderful things. Some of the bizarre inhabitants and phenomena of our Universe are more astounding than even the most extreme sci-fi or space movie.
This selection of some of the most mind-boggling facts about our cosmos takes a bite-sized look at our intriguing planet, Moon, Solar System, Galaxy and Universe.
Here are some of the most mindblowing facts about space and astronomy.
18 facts about space
The Moon is lemon-shaped
Despite its appearance in the night sky, our natural satellite is nowhere near round. In fact, the Moon is shaped like a lemon, with flattened poles and bulges on both the near and far side around its equator.
This strange shape is thought to have been created during interactions with Earth soon after its formation.
Clouds at the centre of the Milky Way smell of rum, taste of raspberries and are packed with booze
In 2009, astronomers exploring a giant cloud of gas and dust at the centre of the Milky Way made a surprise discovery – the cloud was packed full of a chemical known as ethyl formate, which has a couple of intriguing properties: it is responsible for giving raspberries their flavour, and has the smell of rum.
Another nearby region is also notable as it’s full of ethyl alcohol, or ethanol, the type we use to make alcoholic beverages.
It contains enough alcohol to supply every person on the planet with 300,000 pints of beer per day for the next billion years!
If bottled at the source, the proof for this beer would be very low, with an alcohol content of less than one per cent, but as the cloud also contains plenty of other nasty chemicals, among them carbon monoxide and hydrogen cyanide, it would still leave you with quite a headache the next morning.
On Mercury a day lasts twice as long as a year
Technically, one Mercurian day lasts 59 Earth days, while a year lasts 88.
However, due to Mercury’s very eccentric orbit and alignment with the Sun, the length of time from sunrise to sunrise, known as a ‘solar day’, is equal to 176 Earth days — twice as long as a Mercurian year.
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If your spacesuit started leaking, you could survive for a couple of minutes
Although films such as Total Recall show instant explosions and rapidly puffed-up spacesuits, the effects of being exposed to space are slightly less dramatic.
Although it would definitely be unpleasant, you could survive for a couple of minutes.
After around 10 seconds, you would lose consciousness. The lower pressure of the vacuum would cause your blood to boil, along with other body fluids (the moisture on your tongue, for example) – but this boiling alone would not be fatal due to the pressure maintained by our blood vessels themselves.
Gas bubbles would form in your bodily fluids, causing your body to swell up and bloat. The low humidity of space would cause you to cool down rapidly, and your eyes may freeze over.
Within one to two minutes, the lack of oxygen would be deadly.
The stress of the situation may make these symptoms worse – you would become oxygen-deprived more quickly.
A rapid decompression would cause damage to your lungs, eardrums and sinuses, along with bruising and bleeding from soft tissues.
One teaspoonful of neutron star would weigh the same as the entire human population
A neutron star’s density is mind-boggling. These stars are composed almost entirely of neutrons packed together in a tiny radius.
Just a teaspoonful of this material would weigh over a trillion kilograms — more than the weight of the entire human population (which reaches a few hundred billion kilograms).
To make something as dense as a neutron star, the whole of humanity would need to be crammed into a space the size of a sugar cube.
Gamma-ray bursts can release more energy in 10 seconds than our Sun will in its entire life
Nothing in the Universe rivals the power unleashed during a gamma-ray burst, a brief but incredibly intense flash of high-energy radiation.
There are many types of GRB: some are thought to form when a massive star implodes; others when two neutron stars merge together.
There are stars we will never be able to see
Ever since the Big Bang, most objects in space have been moving away from one another. In fact, the expansion of the Universe is actually accelerating.
As regions of space are whizzing away from one another at an ever-increasing rate, the first population of stars to form in the Universe are now too far away for us to ever hope of spying them – even using the best present or future telescope.
Hope is not lost; we can attempt to spot them indirectly via the energetic bursts of radiation they emit at the end of their lives.
Black holes have theoretical opposites known as white holes
Black holes are known for their voracious appetites; their influence is so strong that even light can’t escape their gravity. But they have a theoretical converse – white holes.
They are effectively the opposite of their dark relatives, spitting out light and matter instead of trapping it.
So far, they are purely hypothetical objects; astronomers are contemplating how they could form in reality.
If Jupiter’s magnetic field were visible, it would appear bigger than the Moon
The region of space in which a mass’s magnetic field dominates is known as its magnetosphere. These regions surround planets, pulsars and even our Galaxy.
The planets in our Solar System have magnetospheres that interact with and are shaped by the charged particles in the wind streaming from our Sun.
The largest magnetosphere in our Solar System surrounds Jupiter. Jupiter rotates very fast and has a very strong magnetic field, and its magnetosphere is filled with plasma from its volcanically active moon, Io.
These features, coupled with the fact that the solar wind is slower and less dense at Jupiter than at Earth, lead to a very sizeable Jovian magnetosphere.
It is easily big enough to contain a body the size of our Sun and, if visible, would be larger than the Moon in our night sky; quite an achievement considering that it is over 1,500 times farther away.
Neptune has only completed one orbit around the Sun since its discovery
Neptune takes a whopping 165 years to complete one full orbit around the Sun. Since it was discovered in 1846, Neptune only recently finished its first full post-discovery orbit in 2011.
Demoted planet Pluto has yet to match this – it is not even close to completing one full, 248-year orbit since its discovery in 1930.
Planets can wander through space without a parent star
Not all planets form and stay around stars: astronomers estimate that there could be more than 200 billion of them floating free and drifting through our Galaxy.
These ‘rogue’ planets were thought to have been kicked out of their home systems.
While this is true for some, other planets may have formed completely independently of an accretion disk (as was the case for our Solar System) instead forming from the collapse of tiny, cold clouds known as globulettes.
The Sun loses a billion kilos per second
Particles in the Sun’s upper atmosphere are so hot and energetic that they speed out into space as part of the solar wind.
Our star sheds around 1.3 trillion trillion trillion particles every second. This equates to roughly one billion kilograms of matter per second, or one Earth every 185 million years.
Most Sun-like stars in our galaxy are in multiple star systems
Our Sun may be a single star, but it is in the minority.
Over half of the Sun-like stars in the Milky Way are part of multiple star systems, binaries or triplets, with stars orbiting around a common centre of mass.
Most lower-mass stars like red dwarfs, however, live alone without a companion.
Vast amounts of water have been found in space
Earth’s oceans may not be that unique. Three of Jupiter’s moons (Europa, Ganymede, and Callisto) and two of Saturn’s (Enceladus (pictured above) and Titan) are thought to have underwater seas.
Europa’s ocean may contain over twice the volume of water found on Earth. However, the most water ever discovered surrounds a black hole some 12 billion lightyears away.
This region contains vast amounts of water vapour, the equivalent of 140 trillion times the volume of water in Earth’s oceans.
There is gravity on the ISS
Footage of astronauts on the ISS may give the impression of a gravity-free environment, but onboard gravity is actually only 10-11% weaker than it is on Earth’s surface.
Astronauts float freely due to the ISS’s continual state of free-fall, the same effect experienced by skydivers.
The difference with the ISS is that it also has horizontal motion. As the ISS moves ‘sideways’ and falls towards Earth, the horizon curves away beneath it at the same rate, keeping the ISS in orbit and simulating a feeling of weightlessness for anyone on board.
Our days are getting longer
Earth’s spin speed is slowing: every year, it takes our planet a little longer to complete one full revolution on its axis.
The change is miniscule, however. Every century, Earth slows by 1/500th of a second; 1,000 years from now, one day will be two hundredths of a second longer than today.
The Moon is getting farther away every year
The Moon exerts a pull on Earth, causing our planet to be slightly egg-shaped.
It affects water even more, creating tides and causing the oceans to pile up towards one side of the planet, forming a ‘tidal bulge’.
This bulge is dragged around with the Moon as it orbits. As Earth rotates faster than the Moon – 24 hours versus 27.3 days – the bulge moves slightly ahead of the Moon’s position in orbit.
The Moon pulls back on it, effectively trying to slow it down and causing Earth’s rotation rate to gradually slow down over time as a result.
As the two bodies interact through gravity, this tugging causes Earth to lose energy while the Moon gains energy.
Because of this energy boost the Moon is slowly spiralling outwards, moving away from us by 3.8cm per year.
Heat from the Big Bang is still around today
The early Universe consisted of a hot soup of ionised gas: a sort of opaque plasma.
About 380,000 years after the Big Bang, this gas cooled sufficiently enough that atoms were able to form.
Radiation left over from the Big Bang is still around us today, and is known as the cosmic microwave background (CMB).
It can't be seen with the naked eye, but various missions over the years have been able to study it in microwave light, including ESA's Planck satellite and the WMAP mission.
Nicky Jenner is a science writer who works with the European Space Agency and the Hubble Space Telescope.