HIP 102900
HIP 102900 is a K-type (Orange) star.
At a distance of roughly 2,146 light-years, HIP 102900 is a distant star lying deep within the Milky Way galaxy.
HIP 102900 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 102900 has an apparent magnitude of +8.01, 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 +1.304.
Физические свойства
| Спектральный класс | K Class K — K-type (Orange) |
| Показатель цвета (B−V) | 1,304 |
Наблюдение
| Видимая звёздная величина | +8.01 |
| Абсолютная звёздная величина | -1,08 |
| Расстояние | 2,146 ly |
Положение
| Прямое восхождение | 20h 50,79m |
| Склонение | -39° 23,79′ |
Frequently Asked Questions
What type of star is HIP 102900?
HIP 102900 is a Class K — K-type (Orange) star.
How far is HIP 102900 from Earth?
HIP 102900 is approximately 2,145.8 light-years from Earth.
Can you see HIP 102900 with the naked eye?
With an apparent magnitude of 8.01, HIP 102900 is not visible to the naked eye.