HIP 84485
HIP 84485 is a K-type (Orange) star located in the constellation Scorpius.
At a distance of roughly 1,763 light-years, HIP 84485 is a distant star lying deep within the Milky Way galaxy.
HIP 84485 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 84485 has an apparent magnitude of +8.48, 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 +1.619.
Fiziksel Özellikler
| Spektral Sınıf | Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,619 |
Gözlem
| Görünür Parlaklık | +8.48 |
| Mutlak Parlaklık | -0,18 |
| Mesafe | 1,763 ly |
| Takımyıldız | Scorpius |
Konum
| Sağ Açıklık | 17h 16,31m |
| Dik Açı | -39° 36,64′ |
Sıkça Sorulan Sorular
What type of star is HIP 84485?
HIP 84485 is a Class K — K-type (Orange) star.
How far is HIP 84485 from Earth?
HIP 84485 is approximately 1,763.0 light-years from Earth.
Can you see HIP 84485 with the naked eye?
With an apparent magnitude of 8.48, HIP 84485 is not visible to the naked eye.
What constellation is HIP 84485 in?
HIP 84485 is located in the constellation Scorpius.