HIP 14890

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HIP 14890 is a K-type (Orange) star located in the constellation Perseus.

At a distance of roughly 1,294 light-years, HIP 14890 is a distant star lying deep within the Milky Way galaxy.

HIP 14890 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.

HIP 14890 has an apparent magnitude of +8.26, 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 +1.303.

Sifat Fisik

Kelas Spektral K Class K — K-type (Orange)
Indeks Warna (B−V) 1,303

Pengamatan

Magnitudo Semu +8.26
Magnitudo Mutlak 0,27
Jarak 1,294 ly
Rasi Bintang Perseus

Posisi

Asensio Rekta 3h 12,18m
Deklinasi 53° 14,29′

Frequently Asked Questions

What type of star is HIP 14890?
HIP 14890 is a Class K — K-type (Orange) star.
How far is HIP 14890 from Earth?
HIP 14890 is approximately 1,294.3 light-years from Earth.
Can you see HIP 14890 with the naked eye?
With an apparent magnitude of 8.26, HIP 14890 is not visible to the naked eye.
What constellation is HIP 14890 in?
HIP 14890 is located in the constellation Perseus.