White subgiant · Pavo
β Pavonis
Also known as: β Pav, HIP 102395
mag 3.4140 light-years
About
β Pavonis is a white subgiant of magnitude 3.4 in Pavo, about 140 light-years away.
How to find it
- β Pavonis is in the constellation Pavo.
- Best evenings: around mid-September it is highest at about 9 pm (10 pm in summer time); a month earlier, two hours later.
- Where on Earth: it is seen well, at least 10° up, from south of 14° N.
When it rises and sets tonight, how high it climbs and how much the Moon gets in the way are worked out in your browser for your place.
What you will see
- EyesVisible from the suburbs on a clear night, but lost in bright city skies.
- Binoculars (10×50)A sharp point; binoculars bring out its colour and the fainter stars around it.
- Telescope (6–8 inch)Still a point of light at any magnification — stars are too far away to show a disc. Low in the sky, bright stars twinkle and flash colours.
Stars look the same in any instrument: brighter and sharper, but never bigger.
Facts
| Designation | β Pavonis (β Pav) |
|---|---|
| Hipparcos number | HIP 102395 |
| Type | White subgiant |
| Spectral type | A5IV |
| Colour | Yellowish whiteB−V colour index 0.16 |
| Magnitude | 3.4The smaller the number, the brighter. |
| Distance | 140 light-yearsThe light you see left it around 1890. |
| Proper motion | 0.044″ per year across the sky |
| Constellation | Pavo |
| Right ascension (J2000) | 20h 44m 57.5s |
| Declination (J2000) | −66° 12′ 12″ |
Sources and credits
Star data: HYG Database by David Nash, CC BY-SA 4.0. All data sources →