HIP 42900
HIP 42900 is a K-type (Orange) star.
HIP 42900 is an extraordinarily remote star, situated approximately 326,156 light-years from Earth.
HIP 42900 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 42900 has an apparent magnitude of +7.71, 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 +1.720.
Fiziksel Özellikler
| Spektral Sınıf | K Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,720 |
Gözlem
| Görünür Parlaklık | +7.71 |
| Mutlak Parlaklık | -12,29 |
| Mesafe | 326,156 ly |
Konum
| Sağ Açıklık | 8h 44,53m |
| Dik Açı | -47° 59,16′ |
Frequently Asked Questions
What type of star is HIP 42900?
HIP 42900 is a Class K — K-type (Orange) star.
How far is HIP 42900 from Earth?
HIP 42900 is approximately 326,156.0 light-years from Earth.
Can you see HIP 42900 with the naked eye?
With an apparent magnitude of 7.71, HIP 42900 is not visible to the naked eye.