The future of our Solar System

The sequence of the figures below illustrates the future of our own Solar System.
(© Boris Gänsicke, University of Warwick)



The figure on the right shows the Solar System as it is now, with Mercury, Venus, Earth and Mars orbiting in relatively close orbits around the Sun. The large gas planets Jupiter and Saturn are in wide orbits. Uranus, Neptune, and Pluto are even further out, and not visible on the scale of this diagram. An asteroid belt extends from a distance of about 450 solar radii from the Sun out to about 720 solar radii. The Sun produces the energy it radiates away, 400 million billion billion Watts, by the nuclear fusion of hydrogen deep in its core.

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As the Sun evolves through its stellar life cycle, it will eventually burn all the hydrogen content of its core, and start to swell up to become a red giant. During this phase, it will sweep up the inner planets Mercury, Venus, and proably the Earth as well. But while growing to a red giant, the Sun will also lose about half of its mass, and as a consequence Mars, the asteroids, and the outer planets will move further out. This will happen in about 5 to 8 billion years from now.

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Once the outer envelope of the red giant is dispersed, the core of what used to be the Sun shrinks into an Earth-sized object, still containing about half the mass that the Sun once had: a white dwarf has formed. This compact star is initially very hot, more than a hundred thousand degrees but, devoid of nuclear energy, it is condemned to cool down as time passes, with its planets and asteroids relentlessly orbiting around it.

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Eventually, one of the asteroids may be dislodged form its nearly circular orbit by the gravitational pull of Jupiter, and be sent on a course that will bring it very close to the white dwarf. The strong gravitational field will tidally disrupt the asteroid as it gets too close to the white dwarf, and the rocky and metal-rich material of the asteroid will then be evaporated by the radiation from the hot white dwarf and form a ring of gas rotating closely around the white dwarf (note the different scale compared to the three figures above). It is this that we have detected around the white dwarf SDSS1228+1040, which has been cooling for about 100 million years since the red giant phase: a disk of elements such as calcium, magnesium, and iron,  orbiting the compact star at a distance of only 1.2 solar radii with a velocity of more than 1000 kilometers per second. In that respect, our observations of SDSS1228+1040 resemble a glimpse into the remote future of our own solar system.

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