Tycho G

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Template:Short description

Tycho G
File:SN1572.Companion.jpg
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 Template:RA[1]
Declination Template:DEC[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. Template:Rnd ly
(approx. Template:Rnd pc)
Details
Mass1.0[3] Template:Solar mass
Radius1.32–2.63[3] Template:Solar radius
Luminosity1.9–7.6[3] Template:Solar luminosity
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
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
2MASS J00252358+6408019, [RCM2004]+Tycho G
Database references
SIMBADdata

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Tycho G has been proposed as the surviving binary companion star of the SN 1572 supernova event. The star is located about Script error: No such module "val". light-years away in the constellation Cassiopeia. It is a subgiant, similar to the Sun in temperature, but more evolved and luminous.

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]

See also

References

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External links

Template:Stars of Cassiopeia