HD 196050

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HD 196050
Observation data
Epoch J2000.0
Constellation
(pronunciation)
Pavo
Right ascension 20h 37m 51.7102s
Declination −60º 38' 04.1346″
Apparent magnitude (V) 7.6
Absolute magnitude (V) 4.2
Distance 153.05 ly
(46.93 pc)
Spectral type G3V
Other designations
HIP 101806, SAO 254837

HD 196050 is a star located in the constellation Pavo at a distance of 153 light years or 47 parsecs or 1.45 exameters away from the Solar System. This star has the apparent magnitude of 7.6 and the absolute magnitude is 4.2. It is a yellow main-sequence star of spectral type G3. The mass & radius are larger than the Sun by 10-20%. The age of the star is younger and intermediate in metallicity. The star is also called by the Hipparcos number 101806.

[edit] HD 196050 b

HD 196050 b
Discovery
Discovered by Jones et al.
Discovery site Australia
Discovery date 2002
Detection method Doppler Spectroscopy
Designations
Alternative names HIP 101806 b
SAO 254837 b
Semi-major axis 2.54 AU
Eccentricity 0.228±0.038
Orbital period 1378±21 d
Average orbital speed 20.1 km/s
Angular distance 54.12 mas
Longitude of periastron 187±12°
Time of periastron 2450843±56JD
Semi-amplitude 49.7±2 m/s
Physical characteristics
Mass >2.90 MJ

HD 196050 b is a 1378-day extrasolar planet with a minimum mass of 2.90 Jupiter mass or 5.51 wekagrams. The average orbital distance is 2.54 astronomical units or 380 gigameters or 12.3 microparsecs. The eccentricity of the orbit is 22.8%. The periastron (closest) distance is 1.96 AU and the apastron (farthest) distance is 3.12 AU. The average orbital velocity is 20.1 km/s and the semi-amplitude is 49.7 m/s. The longitude of periastron is 187° and the time of periastron is 2,450,843 JD.

The planet is typically discovered by using Doppler spectrometer by looking for shifts in the spectrum of the star. In Australia, Jones et al. found this planet in 2002 by using the telescope in Anglo-Australian Observatory.

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