94 Ceti b

94 Ceti b
	Simulated view of the 94 Ceti binary system
Discovery
Discovered by	Mayor et al.
Discovery date	August 7, 2000
Detection method	Doppler Spectroscopy
Orbital characteristics
Semi-major axis	1.427 AU (213,500,000 km)
Eccentricity	0.30±0.04
Orbital period (sidereal)	535.7±3.1 d
Inclination	65 or 115 ±3
Time of periastron	2,450,944±12
Argument of periastron	41±8
Semi-amplitude	36.2±1.9
Star	94 Ceti
Physical characteristics
Mass	1.855±0.045 MJ

94 Ceti b or 94 Ceti Ab to distinguish it from the distant red dwarf companion, is an extrasolar planet orbiting its star once every 1.2 years. It was discovered on August 7, 2000 by a team led by Michel Mayor.^[2]

It is most stable if its inclination is about 65 or 115, yielding a mass of about 1.85 that of Jupiter.^[1]

^ ^a ^b ^c ^d Cite error: The named reference Plávalová2013 was invoked but never defined (see the help page).
^ Cite error: The named reference Mayor2004 was invoked but never defined (see the help page).

[Plávalová2013-1] Cite error: The named reference Plávalová2013 was invoked but never defined (see the help page).

[Mayor2004-2] Cite error: The named reference Mayor2004 was invoked but never defined (see the help page).

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