HIP 18415

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HIP 18415 is a B-type (Blue-White) star located in the constellation Perseus.

At a distance of roughly 1,026 light-years, HIP 18415 is a distant star lying deep within the Milky Way galaxy.

HIP 18415 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.

HIP 18415 has an apparent magnitude of +8.96, 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 blue-white hue, which corresponds to a B-V color index of +0.128.

Fiziksel Özellikler

Spektral Sınıf B Class B — B-type (Blue-White)
Renk İndeksi (B−V) 0,128

Gözlem

Görünür Parlaklık +8.96
Mutlak Parlaklık 1,47
Mesafe 1,026 ly
Takımyıldız Perseus

Konum

Sağ Açıklık 3h 56,21m
Dik Açı 46° 57,14′

Frequently Asked Questions

What type of star is HIP 18415?
HIP 18415 is a Class B — B-type (Blue-White) star.
How far is HIP 18415 from Earth?
HIP 18415 is approximately 1,025.6 light-years from Earth.
Can you see HIP 18415 with the naked eye?
With an apparent magnitude of 8.96, HIP 18415 is not visible to the naked eye.
What constellation is HIP 18415 in?
HIP 18415 is located in the constellation Perseus.