
51 Pegasi b
Planet· orbits the Sun
51 Pegasi b ('Dimidium') — the first exoplanet ever found around a Sun-like star (1995). A 'hot Jupiter' of at least ~0.46 Jupiter masses whipping around its star every 4.2 days, far closer than Mercury — a type of world no one expected. Found by radial velocity, so its mass is a minimum and its size is a model estimate; no density is quoted. Never imaged.
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Key facts
Minimum mass
8.72 × 10²⁶ kg
0.459 M♃ (146 M⊕)
Year
4.23 Earth days
Distance from 51 Pegasi
7,883,808 km
Science
Physical
- Minimum mass (m·sin i)
- 8.72 × 10²⁶ kg · 0.459 M♃ (146 M⊕)
- Radius
- Not measured
Orbital
- Semi-major axis
- 7,883,808 km
- Eccentricity
- 0.0063
- Inclination
- 0.00 °
- Orbital period
- 4.2 days
- Perihelion
- 7,834,140 km
- Aphelion
- 7,933,476 km
- Mean orbital velocity
- 136 km/s
Composition
- Bulk composition
- A 'hot Jupiter' — a gas giant of at least about half Jupiter's mass orbiting its star every 4.2 days, far closer than Mercury. Its very existence overturned expectations that giant planets must form far from their stars, and launched exoplanet science. Never imaged.
- Cloud appearance
- Appearance based on NASA/JPL-Caltech's artist's concept. No spacecraft has imaged this world, so its real appearance is unknown — The banded clouds shown are a representation of its class, shown only in Vision mode; Realism shows a plain spectral colour.
Radiation & temperature
- Insolation
- 506 S⊕ · 506× the sunlight Earth receives
- Equilibrium temperature
- 1,284 K (1011 °C)
Discovery & history
- Method
- Radial-velocity detection (stellar wobble)
- Name
- Its IAU proper name is 'Dimidium' (Latin for 'half', for its ~half-Jupiter minimum mass) — the first exoplanet ever given a proper name (2015).
Announced in October 1995 by Mayor & Queloz — the discovery that launched exoplanet science and shared the 2019 Nobel Prize in Physics. In 2015 it became the first exoplanet to receive an IAU proper name, 'Dimidium'.
Images

Images from open archives · credit shown per image