HIP 15617

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HIP 15617 is a B-type (Blue-White) star located in the constellation Perseus.

At a distance of roughly 1,087 light-years, HIP 15617 is a distant star lying deep within the Milky Way galaxy.

HIP 15617 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.

HIP 15617 has an apparent magnitude of +9.17, 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 +0.000.

Physikalische Eigenschaften

Spektralklasse B Class B — B-type (Blue-White)
Farbindex (B−V) 0,000

Beobachtung

Scheinbare Helligkeit +9.17
Absolute Helligkeit 1,56
Entfernung 1,087 ly
Sternbild Perseus

Position

Rektaszension 3h 21,10m
Deklination 43° 21,63′

Frequently Asked Questions

What type of star is HIP 15617?
HIP 15617 is a Class B — B-type (Blue-White) star.
How far is HIP 15617 from Earth?
HIP 15617 is approximately 1,087.2 light-years from Earth.
Can you see HIP 15617 with the naked eye?
With an apparent magnitude of 9.17, HIP 15617 is not visible to the naked eye.
What constellation is HIP 15617 in?
HIP 15617 is located in the constellation Perseus.