HIP 104757
HIP 104757 is a K-type (Orange) star.
At a distance of roughly 1,004 light-years, HIP 104757 is a distant star lying deep within the Milky Way galaxy.
HIP 104757 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 104757 has an apparent magnitude of +8.49, 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 orange hue, which corresponds to a B-V color index of +1.092.
Sifat Fisik
| Kelas Spektral | K Class K — K-type (Orange) |
| Indeks Warna (B−V) | 1,092 |
Pengamatan
| Magnitudo Semu | +8.49 |
| Magnitudo Mutlak | 1,05 |
| Jarak | 1,004 ly |
Posisi
| Asensio Rekta | 21h 13,36m |
| Deklinasi | 20° 14,50′ |
Frequently Asked Questions
What type of star is HIP 104757?
HIP 104757 is a Class K — K-type (Orange) star.
How far is HIP 104757 from Earth?
HIP 104757 is approximately 1,003.6 light-years from Earth.
Can you see HIP 104757 with the naked eye?
With an apparent magnitude of 8.49, HIP 104757 is not visible to the naked eye.