HIP 3250
HIP 3250 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 2,330 light-years, HIP 3250 is a distant star lying deep within the Milky Way galaxy.
HIP 3250 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 3250 has an apparent magnitude of +8.75, 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 +1.771.
Физические свойства
| Спектральный класс | K Class K — K-type (Orange) |
| Показатель цвета (B−V) | 1,771 |
Наблюдение
| Видимая звёздная величина | +8.75 |
| Абсолютная звёздная величина | -0,52 |
| Расстояние | 2,330 ly |
| Созвездие | Cassiopeia |
Положение
| Прямое восхождение | 0h 41,40m |
| Склонение | 59° 24,68′ |
Frequently Asked Questions
What type of star is HIP 3250?
HIP 3250 is a Class K — K-type (Orange) star.
How far is HIP 3250 from Earth?
HIP 3250 is approximately 2,329.7 light-years from Earth.
Can you see HIP 3250 with the naked eye?
With an apparent magnitude of 8.75, HIP 3250 is not visible to the naked eye.
What constellation is HIP 3250 in?
HIP 3250 is located in the constellation Cassiopeia.