HD 142 b

Host HD 142 · 5 published parameter sets in the archive snapshot. The archive default is highlighted. Each row is computed from that paper’s own values only.

Why this planet is in the demo: default 396.96768034 M_earth (Msini, Feng et al. 2022) vs composite 2256.5816897 M_earth (Mass, limit flag 0, Gaia Collaboration et al. 2023); ratio 5.68.

Parameter sets for HD 142 b
PaperR [R⊕]M [M⊕]a [AU]densityinsolationequilibrium temperaturehabitable-zone status
Feng et al. 2022default
pset-hd-142-b-feng-et-al-2022
—396.96768034
Msini
1.039— no planet radius— no stellar radius— no stellar radius— no stellar radius
Butler et al. 2006
pset-hd-142-b-butler-et-al-2006-2006apj-646-505b
—416.34
Msini
1.045— no planet radius— no stellar radius— no stellar radius— no stellar radius
Gaia Collaboration et al. 2023
pset-hd-142-b-gaia-collaboration-et-al-2023
—2256.5816897
Mass
—— no planet radius— no stellar radius— no stellar radius— no stellar radius
Tinney et al. 2002
pset-hd-142-b-tinney-et-al-2002
—327.35
Msini
1— no planet radius— no stellar radius— no stellar radius— no stellar radius
Wittenmyer et al. 2012
pset-hd-142-b-wittenmyer-et-al-2012
—397.27
Msini
1.02— no planet radius2.84 [2.61–3.10]331 [324–338]2.84 [2.61–3.10]
too hot

What the composite table would give

The archive’s Planetary Systems Composite Parameters table keeps one row per planet and fills each value from whichever reference its rules pick, so a single row can mix papers.

Composite values and their references
ValueCompositeReference
radiusEarth12.7Calculated Value
massEarth2256.5816897
Mass
Gaia Collaboration et al. 2023
semiMajorAxisAu1.039Feng et al. 2022
stellarRadiusSun1.47Wittenmyer et al. 2012
stellarTeffK6245Wittenmyer et al. 2012
  • density: 6.09 [5.22–6.94] — mixes Calculated Value + Gaia Collaboration et al. 2023
  • insolation: 2.75 [2.46–3.08] — mixes Feng et al. 2022 + Wittenmyer et al. 2012
  • equilibrium temperature: 328 [319–337] — mixes Feng et al. 2022 + Wittenmyer et al. 2012
  • habitable-zone status: 2.75 [2.46–3.08]
    too hot
    — mixes Feng et al. 2022 + Wittenmyer et al. 2012

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