Kepler-452 b

Host Kepler-452 · 6 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: named in spec planet selection rule 2.

Parameter sets for Kepler-452 b
PaperR [R⊕]M [M⊕]a [AU]densityinsolationequilibrium temperaturehabitable-zone status
Jenkins et al. 2015default
pset-kepler-452-b-jenkins-et-al-2015
1.63—1.046— no planet mass1.12 [0.93–1.44]262 [250–279]1.12 [0.93–1.44]
too hot
Berger et al. 2018
pset-kepler-452-b-berger-et-al-2018
1.511——— no planet mass— no semi-major axis— no semi-major axis— no semi-major axis
Morton et al. 2016
pset-kepler-452-b-morton-et-al-2016
1.5——— no planet mass— no semi-major axis— no semi-major axis— no semi-major axis
Q1-Q17 DR24 KOI Table
pset-kepler-452-b-q1-q17-dr24-koi-table
1.13—0.9892— no planet mass0.59 [0.47–0.98]223 [211–253]0.59 [0.47–0.98]
inside
Q1-Q17 DR25 KOI Table
pset-kepler-452-b-q1-q17-dr25-koi-table
1.09—0.994— no planet mass0.58 [0.45–0.80]222 [209–241]0.58 [0.45–0.80]
inside
Q1-Q17 DR25 Supplemental KOI Table
pset-kepler-452-b-q1-q17-dr25-supplemental-koi-table
———— no planet mass— no semi-major axis— no semi-major axis— no semi-major axis

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
radiusEarth1.63Jenkins et al. 2015
massEarth3.29
M-R relationship
Calculated Value
semiMajorAxisAu1.046Jenkins et al. 2015
stellarRadiusSun1.11Jenkins et al. 2015
stellarTeffK5757Jenkins et al. 2015
  • density: 4.21 [2.83–6.18] — mixes Calculated Value + Jenkins et al. 2015
  • insolation: 1.12 [0.93–1.44]
  • equilibrium temperature: 262 [250–279]
  • habitable-zone status: 1.12 [0.93–1.44]
    too hot

All planets