Star · A2
HIP 92296
HIP 92296 is a main-sequence star of spectral type A2 in the constellation Scutum, 501.4 light-years from the Sun.
| Constellation | Scutum |
|---|---|
| Distance | 501.4 light-years (153.7 pc) |
| Apparent magnitude | magnitude 6.49 |
| Absolute magnitude | magnitude 0.56 |
| Spectral type | A2 |
| Surface temperature | 7,850 K |
| Luminosity | 53.4 L☉ |
| Radius | 3.95 R☉ |
| Mass | 2.83 M☉ (estimated) |
| Right ascension (J2000) | 18h 48m 39.5s |
| Declination (J2000) | −6° 00′ 16″ |
| Space velocity (relative to the Sun) | 36.2 km/s |
In the sky
Visible to the naked eye under a dark sky (apparent magnitude 6.49). Visible from the whole Southern Hemisphere and north to latitude 84° N. 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 1525. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 8.9 million years.
The Sun seen from there
From a planet around HIP 92296, the Sun would look like a star of magnitude 10.76, 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.