HIP 69618
HIP 69618 is a B-type (Blue-White) star located in the constellation Centaurus.
Located approximately 481.8 light-years from Earth, HIP 69618 resides within the broader disk of our Milky Way galaxy.
HIP 69618 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
With an apparent magnitude of +5.03, HIP 69618 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its blue hue, which corresponds to a B-V color index of -0.074.
الخصائص الفيزيائية
| النوع الطيفي | B Class B — B-type (Blue-White) |
| مؤشر اللون (B−V) | -0,074 |
الرصد
| القدر الظاهري | +5.03 |
| القدر المطلق | -0,82 |
| المسافة | 482 ly |
| الكوكبة | Centaurus |
الموضع
| المطلع المستقيم | 14h 14,95m |
| الميل | -57° 5,17′ |
Frequently Asked Questions
What type of star is HIP 69618?
HIP 69618 is a Class B — B-type (Blue-White) star.
How far is HIP 69618 from Earth?
HIP 69618 is approximately 481.8 light-years from Earth.
Can you see HIP 69618 with the naked eye?
With an apparent magnitude of 5.03, HIP 69618 is visible to the naked eye.
What constellation is HIP 69618 in?
HIP 69618 is located in the constellation Centaurus.