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75 Ceti c
extrasolar planet
75 Cet c
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Statements
instance of
exoplanet
2 references
stated in
Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars
stated in source according to
Exoplanet Archive
stated in
Extrasolar Planets Encyclopaedia
mass
0.91±0.09
Jupiter mass
1 reference
stated in
Extrasolar Planets Encyclopaedia
time of discovery or invention
August 2023
1 reference
stated in
Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars
stated in source according to
Exoplanet Archive
discovery method
Doppler spectroscopy
2 references
stated in
Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars
stated in source according to
Exoplanet Archive
stated in
Extrasolar Planets Encyclopaedia
constellation
Cetus
1 reference
based on heuristic
inferred from equatorial coordinates
parent astronomical body
75 Ceti
2 references
stated in
Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars
stated in source according to
Exoplanet Archive
object stated in reference as
75 Cet
stated in
Extrasolar Planets Encyclopaedia
object stated in reference as
75 Cet
argument of periapsis
123±156.8
degree
1 reference
stated in
Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars
stated in source according to
Exoplanet Archive
123±156
degree
1 reference
stated in
Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars
stated in source according to
Extrasolar Planets Encyclopaedia
M sin i
0.912±0.143
Jupiter mass
1 reference
stated in
Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars
stated in source according to
Exoplanet Archive
0.91±0.09
Jupiter mass
1 reference
stated in
Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars
stated in source according to
Extrasolar Planets Encyclopaedia
orbital eccentricity
0.023±0.191
1 reference
stated in
Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars
stated in source according to
Exoplanet Archive
orbital period
2,051.62±45.98
day
1 reference
stated in
Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars
stated in source according to
Exoplanet Archive
semi-major axis of an orbit
3.929±0.058
astronomical unit
1 reference
stated in
Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars
stated in source according to
Exoplanet Archive
3.929±0.058
astronomical unit
1 reference
stated in
Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars
stated in source according to
Extrasolar Planets Encyclopaedia
epoch
J2000.0
2 references
stated in
Exoplanet Archive
stated in
Extrasolar Planets Encyclopaedia
right ascension
38.0391598
degree
1 reference
stated in
Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars
stated in source according to
Exoplanet Archive
declination
−1.0350269
degree
1 reference
stated in
Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars
stated in source according to
Exoplanet Archive
time of periapsis
2,454,285±181
Julian day
epoch
J2000.0
1 reference
stated in
Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars
stated in source according to
Extrasolar Planets Encyclopaedia
Identifiers
Extrasolar Planets Encyclopaedia exoplanet ID
75_cet_c--8784
0 references
75_cet_ac--8784
0 references
NASA Exoplanet Archive ID
75 Cet c
0 references
Sitelinks
Wikipedia
(1 entry)
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enwiki
75 Ceti c
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