{"id":32002,"date":"2022-05-24T10:18:32","date_gmt":"2022-05-24T10:18:32","guid":{"rendered":"https:\/\/c01.purpledshub.com\/bbcskyatnight\/?post_type=purple_issue&p=32002"},"modified":"2022-05-24T10:18:32","modified_gmt":"2022-05-24T10:18:32","slug":"seeing-the-solar-systems-future","status":"publish","type":"post","link":"https:\/\/c01.purpledshub.com\/bbcskyatnight\/2022\/05\/24\/seeing-the-solar-systems-future\/","title":{"rendered":"Seeing the Solar System\u2019s future"},"content":{"rendered":"\n
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<\/p>\n<\/div><\/div>\n\n

Seeing the Solar System\u2019s future<\/h2>\n\n

Recent observations offer clues about whether the planets will survive our Sun\u2019s far-off fate of swelling out into the Solar System as a red giant. Colin Stuart <\/strong>investigates<\/p>\n\n

All good things must come to an end, even stars. Eventually, all stars \u2013 including the Sun \u2013 will die and the Universe will fade to black forever For now, our star is able to persist by constantly churning hydrogen into helium. This process, called nuclear fusion, creates enough outwards pressure to resist the relentless force of gravity trying to collapse the Sun into oblivion.<\/span><\/p>\n\n

Currently, the Sun is getting through 600 million tonnes of hydrogen every single second and there will come a time when there is no hydrogen left to burn. Despite its voracious appetite for this abundant element, astronomers estimate that the Sun has about 5 billion years\u2019 worth of fuel left.<\/p>\n\n

Once the hydrogen is exhausted, gravity will win and the Sun\u2019s core will begin to collapse. With solar material now considerably more compressed, the temperature in the core will climb to a staggering 100 million degrees. That compares to the 15 million degrees you\u2019ll currently find in there. Meanwhile, the pressure will reach over a trillion times the atmospheric pressure here on Earth<\/p>\n\n

Such crazy temperatures and pressures mean that helium becomes the ingredient rather than the product, and it gets pressed into carbon and oxygen. The Sun will get through the equivalent of 10 Earth masses of helium every second. This \u2018helium burning\u2019 happens at a much faster rate than the previous slow-and-steady hydrogen-burning phase. The delicate balance within the Sun is now upset the other way. The outwards pressure is so great that it trumps gravity and the Sun begins to bloat into a red giant. It will eventually swell to swallow Mercury and Venus, and it may engulf Earth as well.<\/span><\/p>\n\n

\"\"
Scientists have located a Jupiter-like planet orbiting a white dwarf near the Milky Way\u2019s centre. Its orbit takes it twice as close to its star as Jupiter is from our Sun <\/figcaption><\/figure><\/div>\n\n

The Sun\u2019s final death throes will then see it eject its outer layers into space like a snake shedding its skin. Astronomers call the beautiful, glowing and nested shells of gas this creates a planetary nebula.<\/p>\n\n

Nestled at its centre will be a white dwarf \u2013a ball of carbon and oxygen the size of Earth. Indeed, this is As a Sun-like star runs out of fuel, it expands and loses its outer layers before becoming an Earth-sized ball<\/span> all that will remain of the Sun\u2019s once mighty core. For decades, astronomers have wondered about the true effect of a Sun-like star\u2019s death on its system of planets and moons, in particular whether any planets can survive the onslaught. Now, at last, we have some idea thanks to a breakthrough discovery.<\/span><\/p>\n\n

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\u2018Gravitational microlensing\u2019 can be used to view otherwise unobservable objects. Here, light from a blue star (top) is bent as it passes through the gravitational field of a star (centre) <\/figcaption><\/figure><\/div>\n\n
Clues to our Solar System\u2019s fate<\/strong><\/h5>\n\n

A team led by Joshua Blackman, from the University of Tasmania, Australia, recently found a Jupiter-like planet swirling around a white dwarf close to the centre of our Milky Way Galaxy. \u201cThe system we\u2019ve discovered is a glimpse into the possible future of the Solar System,\u201d says Blackman. While the dying Sun will likely take out the terrestrial planets, the outer planets could well survive. \u201cThis is the first time one of these planets in a similar orbit to Jupiter has been found,\u201d he says.<\/span><\/p>\n\n

Blackman made this important discovery using a technique called \u2018gravitational microlensing\u2019. \u201cThe gravity of the white dwarf and its companion planet acts like a magnifying glass,\u201d Blackman says. \u201cIt bends the light from a more distant star and makes it appear brighter to observers here on Earth.\u201d<\/p>\n\n

However, for this to happen, there has to be a near perfect alignment between the foreground \u2018lens\u2019 and the background star. According to Blackman, the chances of the right alignment are \u201cone in a million\u201d. So, to boost their chances of seeing it, they looked towards the centre of the Milky Way where stars are huddled more closely together. Observe enough background stars and a rare alignment becomes almost guaranteed.<\/span><\/p>\n\n

This is a unique way to look for alien worlds because the two leading methods rely on seeing changes in the light of the host star. Either the star gets dimmer when a planet ghosts in front of it, or we see changes in the starlight caused by the star wobbling due to the gravitational pull of an otherwise unseen planet. Removing the need to see the star\u2019s light opens the door to finding more weird and wonderful worlds like those swirling around dead stars.<\/span><\/p>\n\n

Object of mystery<\/strong><\/h5>\n\n

In fact, the team wasn\u2019t actually looking for planets around dead stars at all. Instead, they were searching for worlds circling ordinary stars in the prime of their lives. This particular microlensing event was seen way back in 2010 and Blackman recently reanalysed the data. The amount of lensing suggests the star has a mass between 15 and 93 per cent that of our own Sun. Then Blackman used the Keck Observatory in Hawai\u2019i to take a closer look, but he was in for a shock: there was nothing to see. The lensing had told them that an object with the mass of a small star was there, but it was seemingly invisible.<\/p>\n\n

\u201cWe were puzzled and spent quite a few years trying to explain the discrepancy between our expectation and what we observed,\u201d says Blackman.\u201cEventually we worked out that the reason we do not see the star is because it\u2019s too dim to see.\u201d They were able to rule out other dead stars like black holes and neutron stars. \u201cIt has to be a white dwarf,\u201d<\/span> Blackman says.<\/p>\n\n

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The Nancy Grace Roman Telescope will be able to image giant planets around white dwarfs near the Milky Way\u2019s centre<\/figcaption><\/figure>\n\n

The white dwarf magnified the light from a background star, but that light was warped by the presence of a planet in tow. The amount of warping told Blackman how massive the planet is. This particular planet is 40 per cent more massive than Jupiter and it orbits the white dwarf approximately twice as close as Jupiter circles around the Sun.<\/span><\/p>\n\n

According to Blackman, such proximity meant it was touch and go whether the planet would survive the death of its star. \u201cIt only needed to be slightly closer to its host star to be disrupted during the star\u2019s giant phase,\u201d he says. \u201cBut the planet survived because it was at a large enough orbit.\u201d<\/p>\n\n

\u201cIt\u2019s a very exciting discovery,\u201d says Thea Kozakis, from the Technical University of Denmark. \u201cSince there are so few known planetary systems around white dwarfs, every planet gives so much insight,\u201d she says.<\/p>\n\n

We may not have to wait too long for the floodgates to open and more discoveries like this to come pouring in. The Nancy Grace Roman Telescope, due for launch in 2027, will be able to directly image giant planets around white dwarfs close to the centre of our Milky Way. For the first time we\u2019ll have a more complete census of these cosmic survivors and we will start to learn so much more about the future of our own Solar System. In particular, we will learn whether planets like these are the lucky few, or whether it\u2019s common for Jupiter-like planets to survive their stars being extinguished.<\/span><\/p>\n\n

\n
\n
\"\"
With their icy shells melted by an expanding red giant Sun, Jupiter\u2019s moon Europa<\/figcaption><\/figure>\n<\/div>\n\n\n\n
\n
\"\"
and Saturn\u2019s Enceladus could be a temporary refuge for life-forms fleeing from<\/figcaption><\/figure>\n<\/div>\n<\/div>\n\n

Kozakis says that these enduring gas giants are a compelling idea because the death of their stars could turn their moons into potentially habitable worlds. Astronomers often talk about a \u2018habitable zone\u2019, a region around a star where the temperature is just right to permit the existence of liquid water. An expanding, dying star will shift this region considerably further out.<\/span><\/p>\n\n

Revealing water worlds<\/strong><\/h5>\n\n

In our own Solar System, for example, Jupiter and Saturn currently have icy moons, such as Europa and Enceladus. In fact, according to Kozakis, approximately 99.9 per cent of the Solar System\u2019s water lies beyond the realm of the terrestrial planets.\u201cDuring the red giant phase it is possible that the increased luminosity of the host star can melt the icy shells of these frozen water worlds, revealing the liquid water oceans that lie beneath,\u201d she says.<\/span><\/p>\n\n

It could offer our descendants a stay of execution.\u201c[Whatever forms of life that are] still around in five billion years would likely have a better chance of survival if it moved to one of Jupiter\u2019s moons,\u201d says Blackman.<\/span> It would, however, only be a temporary reprieve.\u201cWhite dwarfs start off extremely hot and then cool off over time due to the lack of an internal heat source,\u201d says Kozakis. \u201cThis means that the traditional habitable zone will slowly move inward towards the white dwarf over time.\u201d Eventually, you would need to be one hundred times closer to the white dwarf than Earth currently is to the Sun in order to keep warm. An unusually hot white dwarf could relax this constraint, but then it would also give off huge amounts of radiation that life would struggle to deal with.<\/span><\/p>\n\n

Ultimately, unless you are planning to move away from the Solar System, the death of our star is inescapable. Everything comes to an end, so it\u2019s best to enjoy things while they last.<\/p>\n\n

<\/div>
\n

How to make a white dwarf<\/span><\/strong><\/h4>\n\n\n\n

As a Sun-like star runs out of fuel, it expands and loses its outer layers before becoming an Earth-sized ball<\/strong><\/p>\n\n\n\n

\"\"<\/figure>\n\n\n\n

1. Burning hydrogen<\/strong><\/p>\n\n\n\n

A Sun-like star is powered by nuclear fusion, which turns hydrogen into helium with the release of energy. This can go on for around 10 billion years. During this time it is said to be a \u2018main sequence\u2019 star.<\/p>\n\n\n\n

2. Shell burning<\/strong><\/p>\n\n\n\n

A star is said to move off the main sequence when it transitions from burning hydrogen to fusing helium. This often happens in layers surrounding the dead core and so astronomers refer to it as \u2018shell burning\u2019.<\/p>\n\n\n\n

3. Red giant<\/strong><\/p>\n\n\n\n

The star gets through its helium one hundred times faster than it did its hydrogen. This creates huge amounts of outwards pressure and it surges out into its planetary system. Its surface would reach out to about where Earth is now.<\/span><\/p>\n\n\n\n

4. Planetary Nebula<\/strong><\/p>\n\n\n\n

Helium burning is unstable. It sends shockwaves through the star and convulsions shake it apart. A few of these events, each 100,000 years apart, create nested shells called a \u2018planetary nebula\u2019.<\/p>\n\n\n\n

5. White dwarf<\/strong><\/p>\n\n\n\n

A core of carbon and oxygen \u2013 the products of helium fusion \u2013 is left at the centre. Astronomers refer to this as a white dwarf and it contains about half the mass of the original star packed into an Earth-sized ball.<\/p>\n<\/div><\/section>\n\n

Red giant to planetary nebula<\/strong><\/h4>\n\n

Despite the name, planetary nebulae are blown out by dying red giant stars<\/strong><\/p>\n\n

\"\"
No two planetary nebulae are the same. Clockwise from top left: the Butterfly Nebula (NGC 6302), Eskimo Nebula (NGC 2392), Necklace Nebula, Cat\u2019s Eye Nebula (NGC 6543), Red Rectangle Nebula and Helix Nebula. What will the Sun\u2019s planetary nebula end up looking like?<\/figcaption><\/figure>\n\n

Astronomers are pretty confident of the Sun\u2019s fate because the Universe is littered with similar cosmic tombstones. The Cat\u2019s Eye Nebula, in Draco, is perhaps the most famous example of these so-called \u2018planetary nebulae\u2019. They are about a lightyear across (a quarter of the distance from the Sun to the next nearest star).<\/p>\n\n

It\u2019s worth saying that the name planetary nebulae is a terrible one. When early astronomers, armed with primitive telescopes, first stumbled upon them they thought they looked like planets. Today we know better, but the unhelpful name has stuck around.<\/p>\n\n

Planetary nebulae themselves, however, do not stick around for long. They are initially bright because they are lit up by intense ultraviolet light from the dying star. Yet this is only enough to sustain a planetary nebula for a few tens of thousands of years. Eventually it will fade and the intricate grave-marker will disappear from view.<\/p>\n\n

No two planetary nebulae are quite the same either. Sometimes they are roughly spherical, but at other times have a distinct split appearance. The reasons for these unique shapes aren\u2019t entirely clear, but it\u2019s thought to have a lot to do with how the magnetic field of the star gets shaped and moulded as it perishes.<\/p>\n\n

It could be that one day, billions of years from now, an alien race will look across the stars and see a glowing ball of gas that is all that remains of our Sun.<\/p>\n\n

\n\n
\"\"<\/figure><\/div>\n\n

Colin Stuart (@skyponderer) is an astronomy author and speaker. Get a free e-book at colinstuart.net\/ebook<\/p>\n\n

STOCKTREK IMAGES\/TOMASZ DABROWSKI\/ISTOCK\/GETTY IMAGES; ILLUSTRATION, NASA\/ESA\/HUBBLE, NASA\/ESA\/ANDREW FRUCHTER (STSCI) AND THE ERO TEAM (STSCI\/ST-ECF), NASA\/ESA AND THE HUBBLE HERITAGE TEAM (STSCI\/AURA), NASA\/ESA\/C.R. O\u2019DELL (VANDERBILT UNIVERSITY) AND M. MEIXNER, P. MCCULLOUGHAND G. BACON, H. VAN WINCKEL (KU LEUVEN)\/M. COHEN (UC BERKELEY) H. BOND (STSCI) T. GULL (GSFC)\/ ESA\/NASA, NASA, NASA\/ESA\/HEIC AND THE HUBBLE HERITAGE TEAM (STSCI\/AURA), NASA\/JPL-CALTECH\/SETI INSTITUTE, NASA\/JPL\/SPACE SCIENCE INSTITUTE, GETTY, MARK GARLICK<\/p>\n","protected":false},"excerpt":{"rendered":"

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