HIP 94409
HIP 94409 is a M-type (Red) star located in the constellation Lyra.
HIP 94409 is an extraordinarily remote star, situated approximately 326,156 light-years from Earth.
HIP 94409 is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.
HIP 94409 has an apparent magnitude of +9.43, 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 +1.607.
Fiziksel Özellikler
| Spektral Sınıf | Class M — M-type (Red) |
| Renk İndeksi (B−V) | 1,607 |
Gözlem
| Görünür Parlaklık | +9.43 |
| Mutlak Parlaklık | -10,57 |
| Mesafe | 326,156 ly |
| Takımyıldız | Lyra |
Konum
| Sağ Açıklık | 19h 12,90m |
| Dik Açı | 42° 32,94′ |
Sıkça Sorulan Sorular
What type of star is HIP 94409?
HIP 94409 is a Class M — M-type (Red) star.
How far is HIP 94409 from Earth?
HIP 94409 is approximately 326,156.0 light-years from Earth.
Can you see HIP 94409 with the naked eye?
With an apparent magnitude of 9.43, HIP 94409 is not visible to the naked eye.
What constellation is HIP 94409 in?
HIP 94409 is located in the constellation Lyra.