Star · B5IV
HIP 93437
HIP 93437 is a subgiant star of spectral type B5IV in the constellation Lyra, 1,555 light-years from the Sun.
| Constellation | Lyra |
|---|---|
| Distance | 1,555 light-years (476.9 pc) |
| Apparent magnitude | magnitude 6.39 |
| Absolute magnitude | magnitude −2.00 |
| Spectral type | B5IV |
| Surface temperature | 11,870 K |
| Luminosity | 1,010 L☉ |
| Radius | 7.52 R☉ |
| Mass | 6.55 M☉ (estimated) |
| Right ascension (J2000) | 19h 01m 48.4s |
| Declination (J2000) | +33° 37′ 17″ |
| Space velocity (relative to the Sun) | 21.3 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.39). Visible from the whole Northern Hemisphere and south to latitude 56° S. North of latitude 56° N 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 471. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 28 million years.
The Sun seen from there
From a planet around HIP 93437, the Sun would look like a star of magnitude 13.22, in the direction where our sky has the constellation Puppis. 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.