Star · M0III
HIP 98485
HIP 98485 is a giant star of spectral type M0III in the constellation Sagittarius, 1,099 light-years from the Sun.
| Constellation | Sagittarius |
|---|---|
| Distance | 1,099 light-years (337.0 pc) |
| Apparent magnitude | magnitude 6.11 |
| Absolute magnitude | magnitude −1.53 |
| Spectral type | M0III |
| Surface temperature | 3,600 K |
| Luminosity | 1,700 L☉ |
| Radius | 106 R☉ |
| Mass | 7.6 M☉ (estimated) |
| Right ascension (J2000) | 20h 00m 26.5s |
| Declination (J2000) | −43° 02′ 36″ |
| Space velocity (relative to the Sun) | 52.7 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.11). Visible from the whole Southern Hemisphere and north to latitude 47° N. South of latitude 47° S it never sets. 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 927. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 19 million years.
The Sun seen from there
From a planet around HIP 98485, the Sun would look like a star of magnitude 12.47, in the direction where our sky has the constellation Lynx. 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.