HIP 93900
HIP 93900 is a K-type (Orange) star located in the constellation Aquila.
At a distance of roughly 1,169 light-years, HIP 93900 is a distant star lying deep within the Milky Way galaxy.
HIP 93900 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 93900 has an apparent magnitude of +8.02, placing it beyond naked-eye visibility. A good pair of binoculars or a small telescope is required to observe this star. Observers will note its red hue, which corresponds to a B-V color index of +1.521.
Physikalische Eigenschaften
| Spektralklasse | Class K — K-type (Orange) |
| Farbindex (B−V) | 1,521 |
Beobachtung
| Scheinbare Helligkeit | +8.02 |
| Absolute Helligkeit | 0,25 |
| Entfernung | 1,169 ly |
| Sternbild | Aquila |
Position
| Rektaszension | 19h 7,24m |
| Deklination | -4° 53,89′ |
Häufig gestellte Fragen
What type of star is HIP 93900?
HIP 93900 is a Class K — K-type (Orange) star.
How far is HIP 93900 from Earth?
HIP 93900 is approximately 1,169.0 light-years from Earth.
Can you see HIP 93900 with the naked eye?
With an apparent magnitude of 8.02, HIP 93900 is not visible to the naked eye.
What constellation is HIP 93900 in?
HIP 93900 is located in the constellation Aquila.