HD 154857 b explained

HD 154857 b
Discoverer:McCarthy et al.
AAT
Australia
Discovery Site:AAPS
Discovered:2004
Apsis:astron
Aphelion:1.8AU
Perihelion:0.64AU
Semimajor:1.2±
Eccentricity:0.47±0.02
Period:409±1 d
1.12 y
Time Periastron:2450346±5
Arg Peri:59±4
Semi-Amplitude:50.4±1
Mass:>1.8±0.4
(>570±100)

HD 154857 b is an extrasolar planet approximately 224 light years away in the constellation of Ara. This is a gas giant mass that orbits the star in an eccentric orbit. This planet was detected by using Anglo-Australian Telescope (AAT) UCLE spectrometer.

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