Tycho G

Tycho G has been proposed as the surviving binary companion star of the SN 1572 supernova event. The star is located about 6400±1500 light-years away in the constellation Cassiopeia. It is a subgiant, similar to our Sun in temperature, but more evolved and luminous.

Tycho G

Tycho G as seen by Hubble
Credit: NASA, ESA, CXO and P. Ruiz-Lapuente (University of Barcelona)
Observation data
Epoch J2000      Equinox J2000
Constellation Cassiopeia
Right ascension  00h 25m 23.59s[1]
Declination 64° 08′ 02.0″[1]
Apparent magnitude (V) 18.71[2]
Characteristics
Spectral type G0/1 IV[3]
Astrometry
Radial velocity (Rv)−79.22[2] km/s
Proper motion (μ) RA: −2.50[2] mas/yr
Dec.: −4.22[2] mas/yr
Parallax (π)0.5118 ± 0.1208 mas
Distanceapprox. 6,000 ly
(approx. 2,000 pc)
Details
Mass1.0[3] M☉
Radius1.32 - 2.63[3] R☉
Luminosity1.9 - 7.6[3] L☉
Surface gravity (log g)4.0[2] cgs
Temperature6,025[2] K
Metallicity−0.13[2]
Rotational velocity (v sin i)< 6[2] km/s
Age5.7[2] Gyr
Other designations
2MASS J00252358+6408019, [RCM2004]+Tycho G
Database references
SIMBADdata

Origin of the name

The supernova SN 1572 is often called "Tycho's supernova", named after Tycho Brahe who observed the "new star" in 1572. The postfix "G" originates from the candidate companion stars considered in a 2004 study, labelled Tycho A to Tycho V.[4]

Evidence for companion hypothesis

Tycho G is travelling away from us at nearly 80 km/s, much faster than the mean velocity of other stars in its stellar neighbourhood. It matches the properties of some models for the pre-supernova star system, although other studies exclude it.[5]

gollark: Though there are still unencrypted pager messages around here, so who knows...
gollark: One would assume that important military or whatever stuff would be encrypted.
gollark: The somewhat exposed HV wiring around running water seems kind of cursed.
gollark: > Talk of HV and other electronic hazards previously in <#426054145645215756> will be relegated to #danger-high-voltage, which itself will require passing a test to view.
gollark: <#424396218031013888>

See also

References
  1. Cutri, R. M.; Skrutskie, M. F.; Van Dyk, S.; Beichman, C. A.; Carpenter, J. M.; Chester, T.; Cambresy, L.; Evans, T.; Fowler, J.; Gizis, J.; Howard, E.; Huchra, J.; Jarrett, T.; Kopan, E. L.; Kirkpatrick, J. D.; Light, R. M.; Marsh, K. A.; McCallon, H.; Schneider, S.; Stiening, R.; Sykes, M.; Weinberg, M.; Wheaton, W. A.; Wheelock, S.; Zacarias, N. (2003). "VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)". VizieR On-line Data Catalog: II/246. Originally Published in: 2003yCat.2246....0C. 2246. Bibcode:2003yCat.2246....0C.
  2. Kerzendorf, Wolfgang E.; Yong, David; Schmidt, Brian P.; Simon, Joshua D.; Jeffery, C. Simon; Anderson, Jay; Podsiadlowski, Philipp; Gal-Yam, Avishay; Silverman, Jeffrey M.; Filippenko, Alexei V.; Nomoto, Ken'Ichi; Murphy, Simon J.; Bessell, Michael S.; Venn, Kim A.; Foley, Ryan J. (2013). "A High-resolution Spectroscopic Search for the Remaining Donor for Tycho's Supernova". The Astrophysical Journal. 774 (2): 99. arXiv:1210.2713. Bibcode:2013ApJ...774...99K. doi:10.1088/0004-637X/774/2/99.
  3. González Hernández, Jonay I.; Ruiz-Lapuente, Pilar; Filippenko, Alexei V.; Foley, Ryan J.; Gal-Yam, Avishay; Simon, Joshua D. (2009). "The Chemical Abundances of Tycho G in Supernova Remnant 1572". The Astrophysical Journal. 691: 1. arXiv:0809.0601. Bibcode:2009ApJ...691....1G. doi:10.1088/0004-637X/691/1/1.
  4. Ruiz-Lapuente, Pilar; Comeron, Fernando; Méndez, Javier; Canal, Ramon; Smartt, Stephen J.; Filippenko, Alexei V.; Kurucz, Robert L.; Chornock, Ryan; Foley, Ryan J.; Stanishev, Vallery; Ibata, Rodrigo (2004). "The binary progenitor of Tycho Brahe's 1572 supernova". Nature. 431 (7012): 1069. arXiv:astro-ph/0410673. Bibcode:2004Natur.431.1069R. doi:10.1038/nature03006. PMID 15510140.
  5. Pan, Kuo-Chuan; Ricker, Paul M.; Taam, Ronald E. (2014). "Search for Surviving Companions in Type Ia Supernova Remnants". The Astrophysical Journal. 792: 71. arXiv:1407.6829. Bibcode:2014ApJ...792...71P. doi:10.1088/0004-637X/792/1/71.
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