Exoplanet · gas giant
HIP 55507 b
HIP 55507 b is a gas giant orbiting the star HIP 55507. Its year lasts 5,140 Earth days. It was discovered in 2022 by the Radial Velocity method.
| Host star | HIP 55507 |
|---|---|
| Distance | 83.1 light-years (25.5 pc) |
| Orbital period | 14.1 years |
| Orbital radius | 5.06 AU |
| Eccentricity | 0.362 |
| Radius | 12.6 R⊕ · 1.12 R♃ |
| Mass | 2,590 M⊕ · 8.14 M♃ |
| Density | 7.1 g/cm³ |
| Surface gravity | 16.3 × Earth |
| Equilibrium temperature | 76 K (-197 °C) |
| Stellar flux received | 0.0056 × Earth |
| Discovery method | Radial Velocity |
| Discovery year | 2022 |
| Discovered by | Multiple Observatories |
Habitable zone
Beyond the habitable zone: it receives only %0.56 of the light the Earth does, a frozen world.
Its star in the sky
In the planet's sky its star is a disc 0.076° across: 0.14 times the Sun as we see it from Earth.
In the sky
A telescope is needed to see it: its apparent magnitude is 9.80. Visible from the whole Northern Hemisphere and south to latitude 43° S. North of latitude 43° N it never sets. It stands highest at midnight in March, the best time to observe it.
Light's journey
The light you see tonight set out around the year 1943. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.5 million years.
Data: NASA Exoplanet Archive, PSCompPars. Its look in the simulation is a rendering based on the measured radius, mass and temperature.