HIP 11887
HIP 11887 is a K-type (Orange) star.
At a distance of roughly 1,029 light-years, HIP 11887 is a distant star lying deep within the Milky Way galaxy.
HIP 11887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 11887 has an apparent magnitude of +7.74, 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 red hue, which corresponds to a B-V color index of +1.602.
भौतिक गुण
| वर्णक्रम वर्ग | K Class K — K-type (Orange) |
| रंग सूचकांक (B−V) | 1.602 |
प्रेक्षण
| आभासी परिमाण | +7.74 |
| निरपेक्ष परिमाण | 0.24 |
| दूरी | 1,029 ly |
स्थिति
| दक्षिणांश | 2h 33.29m |
| दिगंश | -26° 17.46′ |
Frequently Asked Questions
What type of star is HIP 11887?
HIP 11887 is a Class K — K-type (Orange) star.
How far is HIP 11887 from Earth?
HIP 11887 is approximately 1,028.9 light-years from Earth.
Can you see HIP 11887 with the naked eye?
With an apparent magnitude of 7.74, HIP 11887 is not visible to the naked eye.