Jupiter-sized planet found orbiting white dwarf star in the Milky Way

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Australia; New Zealand; TAS
W. M. Keck Observatory/Adam Makarenko
W. M. Keck Observatory/Adam Makarenko

A Jupiter-sized planet has been found orbiting a white dwarf star in the Milky Way by astronomers from Australia and New Zealand. The team found the gas giant was able to survive the death of its host star, which occurs when the star runs out of hydrogen to burn, and now orbits much closer than previously expected of planets orbiting white dwarfs. The team say that this discovery supports a prediction that over half of white dwarf stars may have similar orbiting planets.

Media release

From: Springer Nature

Astronomy: New gas giant planet found orbiting white dwarf star *IMAGES & VIDEOS*

Evidence of a gas-giant, Jupiter-mass planet orbiting a white dwarf star in a wide orbit in the Milky Way is described in a paper published this week in Nature. Although models have implied that planets of this size and in a similar orbit have been able to survive the death of their host stars from the giant phase into white dwarfs, no such planet has previously been observed.

Joshua Blackman and colleagues obtained deep exposures of the field surrounding a Jupiter-mass planet (MOA2010BLG477Lb) discovered previously through microlensing, a technique that is sensitive to cold planets and does not depend on the light from the host star for measurement. Microlensing can also detect remnants of stars such as white dwarfs. The authors determined that this planet formed at the same time as its host star and managed to survive after the star stopped burning hydrogen in its core. Gas-giant planets orbiting white dwarfs are typically thought to move to orbits 5 or 6 astronomical units (AU) away, but this planet is around 2.8 AU from its star.

These findings provide evidence that planets can survive the giant phase of their host star’s evolution, and supports the prediction that over half of white dwarfs are predicted to have similar planetary companions. 

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White Dwarf System Debris Ring
White Dwarf System Debris Ring
White Dwarf System Animation Text
Keck Observatory B Roll
Journal/
conference:
Nature
Research:Paper
Organisation/s: Massey University, University of Tasmania
Funder: This work was supported by the University of Tasmania through the UTAS Foundation, ARC grant DP200101909, and the endowed Warren Chair in Astronomy. We acknowledge the support of ANR COLD WORLDS (ANR-18-CE31-0002) at the Institut d’Astrophysique de Paris and the Laboratoire d’Astrophysique de Bordeaux. D.P.B., A.B., N.K., C.R. and S.K.T. were supported by NASA through grant NASA-80NSSC18K0274 and by NASA award no. 80GSFC17M0002. E.B. acknowledges support from NASA grant 80NSSC19K0291. Work by N.K. is supported by JSPS KAKENHI grant no. JP18J00897. C.D. acknowledges financial support from the State Agency for Research of the Spanish MCIU through the ‘Center of Excellence Severo Ochoa’ award to the Instituto de Astrofísica de Andalucía (SEV-2017-0709), and the Group project ref. PID2019-110689RB-I00/AEI/10.13039/501100011033. D.V. gratefully acknowledges the support of the STFC via an Ernest Rutherford Fellowship (grant ST/ P003850/1).
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