HD 179079 b
HD 179079 b is a Neptune-like planet orbiting the G5 IV star HD 179079 in the constellation Aquila. It lies about 227 light-years from Earth and was discovered in 2008 using the radial velocity method.
Is HD 179079 b in the Habitable Zone?
HD 179079 b orbits inside the inner edge of the habitable zone of HD 179079. So close to its star, surface conditions are far too hot for liquid water.
Habitable zone of HD 179079: 1.172–2.770 AU (conservative: 1.484–2.626 AU), per Kopparapu et al. (2014). Earth orbits the Sun at 1 AU.
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Orbit and Year Length
A year on HD 179079 b — one full orbit around HD 179079 — lasts 14.5 Earth days, shorter than Mercury's 88-day year. It orbits at an average distance of 0.121 AU — closer to its star than Mercury is to the Sun. Its orbit is nearly circular (eccentricity 0.049).
How Was HD 179079 b Discovered?
HD 179079 b was discovered in 2008 using the radial velocity method, with observations from W. M. Keck Observatory.
The radial velocity method measures the subtle wobble of a star caused by the gravitational pull of an orbiting planet, visible as periodic shifts in the star's light spectrum. The size of the wobble reveals the planet's minimum mass.
How Far Away Is HD 179079 b?
HD 179079 b is 227.4 light-years (69.7 parsecs) from Earth. Light arriving here tonight left the planet around the year 1799. A probe traveling at the speed of Voyager 1 — about 17 km/s, the fastest outbound spacecraft ever launched — would need roughly 4,002,240 years to make the journey.
Earth Similarity Index
The Earth Similarity Index (ESI) scores how physically similar a planet is to Earth, from 0 to 1, based on radius, density, escape velocity and surface temperature. HD 179079 b scores 0.15, ranking #4,222 of 5,568 planets with a known ESI. For reference, Mars scores about 0.70.
The Host Star: HD 179079
HD 179079
- Spectral type
- G5 IV
- Surface temperature
- 5,646 K (Sun: 5,772 K)
- Mass
- 1.14 M☉
- Radius
- 1.63 R☉
- Luminosity
- 2.3988 L☉
- Age
- 7.0 billion years (Sun: 4.6)
Planetary System
HD 179079 b is the only planet known to orbit HD 179079 so far.
HD 179079 b — Complete Data
| Mass (best estimate) | 25.74 Earth masses |
|---|---|
| Orbital period | 14.48 days |
| Orbital distance | 0.121 AU |
| Eccentricity | 0.049 |
| Earth Similarity Index | 0.15 |
| Distance from Earth | 227.4 light-years (69.7 parsecs) |
| Constellation | Aquila |
| Discovery method | Radial Velocity |
| Discovery facility | W. M. Keck Observatory |
| Discovery year | 2008 |
Data: NASA Exoplanet Archive, last updated 2018-09-25. Earth Similarity Index: PHL @ UPR Arecibo.
Frequently Asked Questions About HD 179079 b
Is HD 179079 b habitable?
No — HD 179079 b orbits too close to its star and is too hot for liquid water to exist on its surface.
How far away is HD 179079 b?
HD 179079 b is about 227 light-years from Earth in the constellation Aquila. A spacecraft traveling as fast as Voyager 1 (about 17 km/s) would need roughly 4,002,240 years to get there.
How long is a year on HD 179079 b?
One orbit around HD 179079 takes 14.5 Earth days — short enough that 25 of its years would fit into one Earth year.
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