HIP 75887
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HIP 75887 is a K-type (Orange) star.
At a distance of roughly 1,310 light-years, HIP 75887 is a distant star lying deep within the Milky Way galaxy.
HIP 75887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 75887 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 +1.416.
Sifat Fisik
| Kelas Spektral | K Class K — K-type (Orange) |
| Indeks Warna (B−V) | 1,416 |
Pengamatan
| Magnitudo Semu | +8.02 |
| Magnitudo Mutlak | 0,00 |
| Jarak | 1,310 ly |
Posisi
| Asensio Rekta | 15h 30,00m |
| Deklinasi | -52° 50,85′ |
Frequently Asked Questions
What type of star is HIP 75887?
HIP 75887 is a Class K — K-type (Orange) star.
How far is HIP 75887 from Earth?
HIP 75887 is approximately 1,309.9 light-years from Earth.
Can you see HIP 75887 with the naked eye?
With an apparent magnitude of 8.02, HIP 75887 is not visible to the naked eye.