Phi2 Pavonis

Source: Wikipedia, the free encyclopedia.

Phi2 Pavonis
Observation data
ICRS
)
Constellation Pavo
Right ascension 20h 40m 02.63822s[1]
Declination −60° 32′ 56.0200″[1]
Apparent magnitude (V) +5.10[2]
Characteristics
Spectral type G0 V Fe-0.8 CH-0.5[3]
U−B color index −0.02[2]
B−V color index +0.53[2]
Distance
80.4 ± 0.5 ly
(24.7 ± 0.2 pc)
Details
Gyr
HIP 101983, HR 7875, SAO 254846[6]
Database references
SIMBADdata
ARICNSdata

Phi2 Pavonis2 Pav, φ2 Pavonis) is a solitary

interstellar dust. It is a member of the thin disk population.[4]

This is a yellow-white hued

Sun's radius. The star is radiating 3.39 times the solar luminosity from its photosphere at an effective temperature of 6,091 K.[4]

This system was in 1991 a test case for the

In 1998, using the European Southern Telescope in Chile, a

planet was announced to be orbiting the star.[9] This team retracted this claim in 2002, but found a different periodicity of 7 days possibly due to stellar rotation.[10]

See also

References