SDSS J1240+6710 or SDSS J124043.01+671034.68, nicknamed Dox by its discoverers,[1] is a white dwarf in the constellation Draco. It was discovered by Kepler de Souza Oliveira, Detlev Koester and Gustavo Ourique.[2][1][3] It is unusual for having an atmosphere of almost pure oxygen. The atmosphere also has a detectable amount of magnesium, neon (under 4%) and silicon, but no hydrogen, helium or carbon. A possible explanation for the unusual composition would be if its mass were close to the limit for collapsing to a neutron star.[4] However, its mass is only 0.56 solar masses, below the mass expected for a star that could convert carbon to oxygen, neon and magnesium.[5]
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Draco |
| Right ascension | 12h 40m 43.60s |
| Declination | +67° 10′ 34.68″ |
| Details | |
| Mass | 0.56 M☉ |
| Other designations | |
Dox, SDSS J124043.01+671034.68, SDSS J1240+6710 | |
| Database references | |
| SIMBAD | data |
The star was originally catalogued in the catalogue of new white dwarf stars from the Data Release 12 of the Sloan Digital Sky Survey.[6][7] Gustavo Ourique, an undergraduate in Physics at Universidade Federal do Rio Grande do Sul, identified the star's unique spectrum, working under the advice of Dr. Kepler Oliveira (S.O. Kepler). The star's spectrum was modeled by Dr. Detlev Koester, characterizing its composition, temperature and mass.
In 2020, the star was discovered to be moving at an unusually high velocity. There is no fully-confirmed explanation for this. There are various theories put forth as to possible reasons for this. Some researchers indicate this may be due to a supernova that has not been observed yet, and which would cause this star to move at high velocities.
However, there is no definitive data that can absolutely prove that this is what happened. Astronomers note that some supernovas are difficult to detect, especially if they do not contain the element nickel, which is a key indicator for such events. [8]
References
edit- ^ a b Herkewitz, William (31 March 2016). "Newly Discovered Star Has an Almost Pure Oxygen Atmosphere". Popular Mechanics.
- ^ Kepler, S. O.; Koester, D.; Ourique, G. (31 March 2016). "A white dwarf with an oxygen atmosphere". Science. 352 (6281): 67–69. Bibcode:2016Sci...352...67K. doi:10.1126/science.aad6705. PMID 27034367.
- ^ Gänsicke, Boris (1 April 2016). "An odd one out". Science. 352 (6281): 37. Bibcode:2016Sci...352...37G. doi:10.1126/science.aaf3768. PMID 27034360. S2CID 42293901.
- ^ Hummel, Philipp (30 March 2016). "Weißer Zwerg im Sauerstoff" (in German). Retrieved 1 April 2016.
- ^ "Witte dwergster vertoont een ongewone zuurstofatmosfeer" (in Dutch). 31 March 2016. Retrieved 1 April 2016.
- ^ Kepler, S. O.; Pelisoli, I.; Koester, D.; Ourique, G.; Romero, A. D.; Reindl, N.; Kleinman, S. J.; Eisenstein, D. J.; Valois, A. D. M.; Amaral, L. A. (30 November 2015). "New white dwarf and subdwarf stars in the Sloan Digital Sky Survey Data Release 12". Monthly Notices of the Royal Astronomical Society. 455 (4): 3413–3423. arXiv:1510.08409. Bibcode:2016MNRAS.455.3413K. doi:10.1093/mnras/stv2526. hdl:10183/140429. Retrieved 1 April 2016.
- ^ Grush, Loren (31 March 2016). "Astronomers spot a never-before-seen type of white dwarf star". The Verge. Retrieved 1 April 2016.
- ^ Nuclear blast sends star hurtling across galaxy By Paul Rincon, Science editor, BBC News website, 15 July 2020.