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Astronomers May Have Found a Second-Generation Planet

Confirmed

Science Desk

In Short: Astronomers using Hubble data from 1999 have found evidence of a second-generation planet around a white dwarf.

Hubble 15102 SECONDGEN WIDE THUMB, NASA
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Astronomers may have discovered a second-generation planet orbiting the white dwarf HS 0209+0832, located 270 light-years away in the constellation Cetus. This finding suggests that planets can form from the debris of a dying star, a process previously theorized but never confirmed.

According to University of Warwick astronomer Jamie Williams and colleagues, the white dwarf's far-ultraviolet spectrum, obtained in 1999 with the Space Telescope Imaging Spectrograph (STIS) on the Hubble Space Telescope, revealed the presence of carbon, aluminum, silicon, calcium, titanium, nickel, and zinc in the atmosphere, along with 100 unidentified lines.

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The discovery of these unusual chemical signatures, particularly the high levels of niobium, suggests that a second-generation planet may have formed from the material expelled by the white dwarf. Niobium was found at concentrations more than 1,000 times higher than those seen in the Sun.

Williams explained, 'Forming the protoplanetary disc in this situation is not easy and helps explain why these planets are so rare.' The researchers suggest that the material being absorbed by the white dwarf came from a planet formed from the star’s own expelled matter.

The planet, if confirmed, would be the first actually spotted, scientists report in a study published in Nature Astronomy. The existence of second-generation planets was predicted theoretically more than 15 years ago.

NASA’s TESS (Transiting Exoplanet Survey Satellite) observed the white dwarf for four months, detecting periodic brightness variations that indicate a planet orbits at a distance of about 3.7 million miles, much closer than Mercury orbits the Sun.

The planet, believed to be as large as Jupiter or Saturn, appears to have formed from the remains of a star that’s 270 light-years from Earth. 'In a sense, this system has given birth to a new world using the foundations of the old one,' said Dr. Nicholas Stone from the University of Warwick.

Unlike ordinary planets, which form from the disc of material surrounding a young star, the suspected planet appears to have formed much later. This means that, by extension, understanding LRDs, SMBH, and galaxies, are all related.

The researchers detected a faint, repeating change in brightness occurring approximately every 4.4 days, indicating the presence of a planet. This discovery offers a new glimpse into how planets might form after a star reaches the end of its life.

Eventually, the white dwarf will cool and then maintain a consistent temperature, with the planet in its stable habitable zone for millions of years.

The discovery of the second-generation planet, led by researchers at the University of Warwick and supported by the European Research Council, offers a new glimpse into how planets might form after a star reaches the end of its life.

This finding opens a door to the idea that even in their death throes, solar-type stars can produce planets which might potentially offer limited habitability.

What this adds

Astronomers using Hubble data from 1999 have found evidence of a second-generation planet around a white dwarf, confirming a theoretical prediction made over 15 years ago.

The discovery of high levels of niobium and other heavy elements in the white dwarf's atmosphere provides a chemical signature that distinguishes this planet from ordinary 'first-generation' planets.

This finding adds to the growing body of evidence that planetary systems can potentially rebuild themselves after stellar death, suggesting that the formation of planets is not limited to the early stages of a star's life.

Background

Astronomers using Hubble data from 1999 have found evidence of a second-generation planet around a white dwarf.

Astronomers have confirmed the existence of a Jupiter-sized planet, named Elias 2-24 b, which is less than a million years old, making it the youngest known planet ever discovered.

What's confirmed

What's still developing

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