Star · G8III
HIP 98385
HIP 98385 is a giant star of spectral type G8III in the constellation Aquila, 575.2 light-years from the Sun.
| Constellation | Aquila |
|---|---|
| Distance | 575.2 light-years (176.4 pc) |
| Apparent magnitude | magnitude 6.17 |
| Absolute magnitude | magnitude −0.06 |
| Spectral type | G8III |
| Surface temperature | 4,450 K |
| Luminosity | 171 L☉ |
| Radius | 22 R☉ |
| Mass | 3.95 M☉ (estimated) |
| Right ascension (J2000) | 19h 59m 22.6s |
| Declination (J2000) | +1° 22′ 40″ |
| Space velocity (relative to the Sun) | 57.5 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.17). Visible from the whole Northern Hemisphere and south to latitude 89° S. It stands highest at midnight in July, the best time to observe it.
Through a telescope from Earth
Light's journey
The light you see tonight set out around the year 1451. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 10 million years.
The Sun seen from there
From a planet around HIP 98385, the Sun would look like a star of magnitude 11.06, in the direction where our sky has the constellation Monoceros. It would be invisible to the naked eye.
Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.