WD 1145+017
Coordinates: 11h 48m 33.63s, +01° 28′ 59.4″
Characteristics | |
---|---|
Spectral type | DB[1] |
Observation data Epoch J2000.0 [1] Equinox J2000.0 [1] | |
Constellation | Virgo[2] |
Right ascension | 11h 48m 33.63s [1] |
Declination | +01° 28′ 59.4″ [1] |
Apparent magnitude (V) | 17.0 [3] |
Astrometry | |
Distance | 570[4] ly (174.0 [3] pc) |
Details | |
Mass | 0.6[5] M☉ |
Radius | 0.02[5] R☉ |
Temperature | 15900 ± 500[3] K |
Metallicity [Fe/H] | ~0.1 dex |
Age | 0.175 ± 75[5][lower-alpha 1] Gyr |
Other designations | |
WD 1145+017[1] (EPIC 201563164[3]) is a white dwarf star located approximately 570 light-years (170 pc) from Earth in the constellation of Virgo. It is the first white dwarf to be observed with a transiting planetological object orbiting around it.
Stellar characteristics
The white dwarf has a mass of 0.6 M☉, radius of 0.02 R☉ (1.4 R⊕) and a temperature of 15,900 K, typical for white dwarf stars. It has been a white dwarf for 175 million years.[6] The star included strong absorption lines due to magnesium, aluminium, silicon, calcium iron and nickel. These elements commonly found in rocky planets are polluting the surface of the star, and would normally be expected to mix through the star and disappear from view after a million years.[6]
Based on recent studies and its mass, the star was likely an early F-type main sequence star (spectral type F0) before it became a red giant.[7]
The apparent magnitude of the star, or how bright it appears from Earth's perspective, is about 17. Therefore, it is too dim to be seen with the naked eye.
Planetary system
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 0.0006678 M⊕ | ~0.005 | 0.1875 ± 0.04 | — | ~89° | ~0.01 R⊕ |
Dusty disk | 0.5? AU | — | — |
The supposed planetesimal, WD 1145+017 b,[3] with a 4.5 hour orbit, is being ripped apart by the star and a remnant of the former planetary system that the star hosted before becoming a white dwarf. It is the first observation of a planetological object being shredded by a white dwarf. Several other large pieces have been seen in orbit as well. All the various larger pieces have orbits of 4.5 to 4.9 hours. Rocky material is raining down onto the star, and showing up in the star's spectrum. The system was detected by the Kepler space telescope in its extended K2 mission. Though the system was not a target of interest, it was within the field of view of observing sessions, and analysis of the observed data revealed the system.[8][9][10][11]
An excess of infrared radiation indicates that there is a dusty disk with a temperature of 1,150 K (880 °C).[6]
Notes
- ↑ White dwarf cooling age, not the actual age.
References
- 1 2 3 4 5 6 7 "WD 1145+017". SIMBAD. Retrieved 25 October 2015.
- ↑ Christopher Crockett (21 October 2015). "White dwarf upsets planetary system, consumes evidence".
- 1 2 3 4 5 6 7 "Planet WD 1145+017 b". The Extrasolar Planet Encyclopedia. Retrieved 30 October 2015.
- ↑ Christine Pulliam (21 October 2015). "Cosmic "Death Star" is Destroying a Planet". Harvard-Smithsonian Center for Astrophysics. 2015–21.
- 1 2 3 Andrew Vanderburg; John Asher Johnson; Saul Rappaport; Allyson Bieryla; Jonathan Irwin; John Arban Lewis; David Kipping; Warren R. Brown; Patrick Dufour; David R. Ciardi; Ruth Angus; Laura Schaefer; David W. Latham; David Charbonneau; Charles Beichman; Jason Eastman; Nate McCrady; Robert A. Wittenmyer; Jason T. Wright (11 June 2015). "A disintegrating minor planet transiting a white dwarf" (PDF). Nature (published 22 October 2015). 526: 546–549. arXiv:1510.06387. Bibcode:2015arXiv151006387V. doi:10.1038/nature15527.
- 1 2 3 Bryce Croll; Paul A. Dalba; Andrew Vanderburg; Jason Eastman; Saul Rappaport; John DeVore; Allyson Bieryla; Philip S. Muirhead; Eunkyu Han; David W. Latham; Thomas G. Beatty; Robert A. Wittenmyer; Jason T. Wright; John Asher Johnson; Nate McCrady (8 October 2015). "Multiwavelength Transit Observations of the Candidate Disintegrating Planetesimals Orbiting WD 1145+017". arXiv:1510.06434v1.
- ↑ Veras, Dimitri (2016). "Post-main-sequence planetary system evolution". arXiv:1601.05419 [astro-ph.EP].
- ↑ Ian O'Neill (21 October 2015). "Caught in the Act: White Dwarf is Killing a Planet". Discovery Channel.
- ↑ Michael D. Lemonick (21 October 2015). "Zombie Star Caught Feasting On Asteroids". National Geographic.
- ↑ "NASA's Kepler K2 Mission Discovers Planet-Destroying White Dwarf Star". Sci-News.com. 22 October 2015.
- ↑ Camille M. Carlisle (26 October 2015). "White Dwarf Eats Mini Planet?". Sky and Telescope.
External links
- Harvard Center for Astrophysics, EPIC 201563164
- AstronomyNow, WD 1145+017
- AmericaSpace, WD 1145+017