HD 48265 b

Host HD 48265 · 4 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 484.69075 M_earth (Msini, Barbato et al. 2018) vs composite 2351.9302118 M_earth (Mass, limit flag 0, Wu et al. 2026); ratio 4.85.

Parameter sets for HD 48265 b
PaperR [R⊕]M [M⊕]a [AU]densityinsolationequilibrium temperaturehabitable-zone status
Barbato et al. 2018default
pset-hd-48265-b-barbato-et-al-2018
—484.69075
Msini
1.814— no planet radius1.07 [0.92–1.23]259 [250–268]1.07 [0.92–1.23]
inside
Jenkins et al. 2017
pset-hd-48265-b-jenkins-et-al-2017
—467.2101
Msini
1.81— no planet radius1.18 [1.05–1.32]265 [258–273]1.18 [1.05–1.32]
too hot
Minniti et al. 2009
pset-hd-48265-b-minniti-et-al-2009
—380
Msini
1.6— no planet radius— no stellar radius— no stellar radius— no stellar radius
Wu et al. 2026
pset-hd-48265-b-wu-et-al-2026-2026aj-171-189w
—2351.9302118
Mass
1.87— no planet radius— no stellar radius— no stellar radius— no stellar radius

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
radiusEarth12.6Calculated Value
massEarth2351.9302118
Mass
Wu et al. 2026
semiMajorAxisAu1.814Barbato et al. 2018
stellarRadiusSun1.901Barbato et al. 2018
stellarTeffK5733Barbato et al. 2018
  • density: 6.67 [3.47–9.75] — mixes Calculated Value + Wu et al. 2026
  • insolation: 1.07 [0.92–1.23]
  • equilibrium temperature: 259 [250–268]
  • habitable-zone status: 1.07 [0.92–1.23]
    inside

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