ดาวโรหิณี

87Alp Tau

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An orange K-type star, Aldebaran glows with the warm tint captured in its high B–V colour index of 1.538. It is Alpha Tauri, the brightest star of the constellation Taurus, appearing to sit against the Hyades cluster as the bull's eye. At apparent magnitude 0.87 and a distance of 66.6 light-years, the star's absolute magnitude of −0.68 shows an intrinsic brightness moderately above the Sun's. Its northern declination of +16° makes Aldebaran visible from both hemispheres, and its distinctly orange light stands out among the largely blue and white first-magnitude stars of the northern winter sky.

คุณสมบัติทางกายภาพ

ประเภทสเปกตรัม K Class K — K-type (Orange)
ดัชนีสี (B−V) 1.538

การสังเกต

โชติมาตรปรากฏ +0.87
โชติมาตรสัมบูรณ์ -0.68
ระยะทาง 66.6 ly
กลุ่มดาว Taurus

ตำแหน่ง

ไรต์แอสเซนชัน 4h 35.92m
เดคลิเนชัน 16° 30.56′

Related Chemistry

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Frequently Asked Questions

What type of star is ดาวโรหิณี?
ดาวโรหิณี is a Class K — K-type (Orange) star.
How far is ดาวโรหิณี from Earth?
ดาวโรหิณี is approximately 66.6 light-years from Earth.
Can you see ดาวโรหิณี with the naked eye?
With an apparent magnitude of 0.87, ดาวโรหิณี is visible to the naked eye.
What constellation is ดาวโรหิณี in?
ดาวโรหิณี is located in the constellation Taurus.