A fragment of a planet that has survived the death of its star has been discovered by University of Warwick astronomers in a disc of debris formed from destroyed planets, which the star ultimately consumes.
The iron and nickel rich planetesimal survived a system-wide cataclysm that followed the death of its host star, SDSS J122859.93 + 104032.9. Believed to have once been part of a larger planet, its survival is all the more expensive than it orbits closer to its previous thought possible, going around it once every two hours.
The discovery, reported in the journal Science is the first time that scientists have used spectroscopy to discover a solid body in orbit around a white dwarf, using subtle variations in the emitted light to identify additional gas that the planetesimal is generating. Telescopio Canarias in La Palma, the scientists studied a disc orbiting a white dwarf 410 light years away, formed by the disruption of rocky bodies composed of elements such as iron, magnesium, silicon and oxygen – the four key building blocks of the Earth and most rocky bodies. Within that disc they discovered a ring of gas streaming from a solid body, like a comet's tail. This gas could either be generated by the body itself or by evaporating dust as it collides with small debris within the disc.
The astronomers estimate that this body has to be at least a kilometer in size, but could be as large as a few hundred kilometers in diameter, comparable to the largest asteroids known in our Solar System.
White dwarfs are the remains of stars like our sun that have burned all their fuel and shed their outer layers, leaving behind a core which slowly cools over time. This particular star has shrunk so dramatically the planetesimal orbits within its sun's original radius. Evidence suggests that it was once part of a larger body further out in its solar system and is likely to have been a planet apart than the star started its cooling process.
Lead author Dr. Christopher Manser, a Research Fellow in the Department of Physics, said: "The star would have been about two solar masses, but now the white dwarf is only 70% of the mass of our Sun. size of the Earth — and this makes the star, and in general all white dwarfs, extremely dense.
"The white dwarf's gravity is so strong — about 100,000 times that of the Earth's — that a typical asteroid will be ripped apart by gravitational forces if it passes too close to the white dwarf. "Professor Boris Gaensicke, co-author of the Department of Physics, adds:" The planetesimal we have discovered is deep into the gravitational well of the white dwarf, much closer to it than we would expect to find anything still alive. That is possible because it must be very dense and / or very likely to have internal strength that holds it together, so we propose that it is composed of iron and nickel.
"If it was pure iron it could survive where it lives now, but it could be a body that is rich in iron but with internal strength to keep it together, which is consistent with the planet's being a fairly massive fragment of a planet core. If correct, the original body was at least hundreds of kilometers in diameter because it is only that point planets begin to differentiate — like oil on water — and have heavier elements sink to form a metallic core. ”
Solar systems, and a glimpse into the future of our own.
Dr. Christopher Manser said: "As stars age they grow into red giants, which 'clean out' much of the inner part of their planetary system. In our Solar System, the Sun will expand to where the Earth currently orbits, and will wipe out Earth, Mercury, and Venus Mars and beyond will survive and move further out.
"The general consensus is that 5-6 billion years from now, our Solar System will be white dwarf in place of the Sun, orbited. at Mars, Jupiter, Saturn, the outer planets, as well as asteroids and comets. Gravitational interactions are likely to occur in such remnants of planetary systems, meaning the bigger planets can easily nudge the smaller bodies onto an orbit that takes them close to the white dwarf, where they get shredded by its enormous gravity.
"Learning about the masses of asteroids, or planetary fragments that can reach a white dwarf can tell us something about the planets that we know must further out in this system, but we currently have no way to detect.
"Our discovery is only the second solid planetesimal found in a tight orbit around a white dwarf, with the previous one found because debris passing in front of the star blocked some of its light – that is the "transit method" widely used to discover exoplanets around Sun-like stars The spectroscopic method we developed in this year has been finely tuned, which means that each system observed several hours mostly leads to nothing. search can detect close-in planetsimals without the need for a specific alignment. We already know of several other systems with debris discs very similar to SDSS J122859.93 + 104032.9, which we will study next. We are confident that we will discover additional planetaryimals orbiting white dwarfs, which will then allow us to learn more about their general properties. "
First evidence of rocky planet formation in Tatooine system
C.J. Manser or al., "A planetesimal orbiting within the debris disc around a white dwarf star," Science (2019). science.sciencemag.org/cgi/doi… 1126 / science.aat5330
"A glance in the end of a planetary system," Science (2019). science.sciencemag.org/cgi/doi… 1126 / science.aax0051
Heavy metal planet fragment survives destruction from dead star (2019, April 4)
retrieved April 4, 2019
This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no
part may be reproduced without the written permission. The content is provided for information purposes only.