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WD 0032−317

From Wikipedia, the free encyclopedia
White dwarf system with a hot brown dwarf
WD 0032−317
Observation data
Epoch       Equinox
ConstellationSagittarius
Right ascension00h 34m 49.8573s
Declination−31° 29′ 52.686″
Characteristics
Evolutionary stageWhite dwarf
Astrometry
Parallax (π)2.320±0.053 mas
Distance431.1±9.8 pc
Orbit
PrimaryWD 0032−317
Details
WD 0032−317
Mass0.4187±0.0047 (He-core)
0.386±0.014 (Hybrid-core) M
Radius0.0266±0.0012 R
Temperature36965±100 K
WD 0032−317 b
Mass0.0812±0.0029 (He-core)
0.0750±0.0037 (Hybrid-core) M
Radius0.0789+0.0085
−0.0083
(He-core)
0.0747+0.0085
−0.0079
(Hybrid-core) R
Temperature5126±28 (He-core)
5111±41 (Hybrid-core) (equilibrium temperature) K
Other designations
WD 0032−317, MCT 0032-3146, EC 00323-3146, GALEX J003449.8-312952, 2MASS J00344984-3129524, TIC 251857373, USNO-B1.0 0585-00006922, Gaia DR3 2317319612801004416, Gaia DR2 2317319612801004416
Database references
SIMBADdata

WD 0032−317 is a low masswhite dwarf star orbited bybrown dwarfWD 0032−317 b.

WD 0032−317

[edit]

The white dwarf WD 0032−317 is located about 1,400light years fromEarth.[1] WD 0032−317 formed about three billion years ago when a low mass star (possibly of 1.3solar masses) expanded into itsred giant phase. The star then blew out its outer layers leaving behind the helium-richcore (which is WD 0032−317).

WD 0032−317 b

[edit]

The orbiting brown dwarf, WD 0032−317 b, was massive enough to survive the red giant'snova event.[2] It is an extremely hot and very large (75-88Jupiter masses) brown dwarf that orbits WD 0032−317. One orbit from WD 0032−317 b takes only 2.5 hours. This object is tidally locked to its star with a day side temperature of 8,000 K (7,730 °C; 13,940 °F) and a night temperature of about 2,000 K (1,730 °C; 3,140 °F) making its temperature equivalent to aplanet orbiting close to a late stageB-type star. The intenseultraviolet (UV) exposure can break down themolecules in WD 0032−317's atmosphere and vaporize materials from the surface of the brown dwarf.[3][4][5]

References

[edit]
  1. ^Atkinson, Nancy (2023-08-17)."This Brown Dwarf is 2,000 Degrees Hotter Than the Sun".Universe Today. Retrieved2023-08-28.
  2. ^Yirka, Bob; Phys.org."Discovery of a Brown Dwarf Hotter Than the Sun".phys.org. Retrieved2023-08-28.
  3. ^Hallakoun, Na’ama; Maoz, Dan; Istrate, Alina G.; Badenes, Carles; Breedt, Elmé; Gänsicke, Boris T.; Jha, Saurabh W.; Leibundgut, Bruno; Mannucci, Filippo; Marsh, Thomas R.; Nelemans, Gijs; Patat, Ferdinando; Rebassa-Mansergas, Alberto (2023-08-14)."An Irradiated-Jupiter Analogue Hotter Than the Sun".Nature Astronomy:1–12.arXiv:2306.08672.doi:10.1038/s41550-023-02048-z.ISSN 2397-3366.
  4. ^Gamillo, Elizabeth (15 August 2023)."Astronomers Find a Brown Dwarf That's Hotter Than the Sun | Astronomy.com".Astronomy Magazine. Retrieved28 August 2023.
  5. ^"A Brown Dwarf Star Serves as an Ultrahot-Jupiter Analogue".pubs.aip.org. Retrieved28 August 2023.


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