BD +20°307
Sign in to saveBD+20°307 is a close binary star system approximately 300 light-years away in the constellation Aries. The system is surrounded by a dusty ring, and probably orbited by a 0.48 white dwarf on a wide (980 AU) orbit.
Astronomical data · SIMBAD
- Object type
- SB*
- Spectral type
- G0
- Distance
- 383 light-years
- Redshift
- z = -0.00004146115751924029
- Coordinates
- RA 28.7098° · Dec 21.3062°
via SIMBAD · CDS Strasbourg
Wikidata facts
- Constellation
- Aries
- Distance from Earth
- 119.9890
- Image
- Colliding planets.jpg
Show 10 more facts
- right ascension component of proper motion
- 39.32
- declination component of proper motion
- -31
- spectral class
- G0
- catalog code
- Gaia DR2 97294345128598656
- right ascension
- 28.70976691333630
- declination
- 21.30623978048820
- apparent magnitude
- 7.603
- parallax
- 8.460
- radial velocity
- -12.43
- epoch
- J2000.0
Sources (1)
via Wikidata · CC0
~5 min read
Encyclopedic overview
6 sectionsContents
- Spectroscopic binary
- Dust cloud
- Sun-like stars with hot dust
- See also
- References
- External links
BD+20°307 is a close binary star system approximately 300 light-years away in the constellation Aries. The system is surrounded by a dusty ring, and probably orbited by a 0.48 white dwarf on a wide (980 AU) orbit.
The dust that orbits around several hundred main-sequence stars is cold and comes from a Kuiper-belt analogous region. In the Solar System the ongoing collisions between asteroids generate a tenuous cloud of dust known as the zodiacal light. When the Solar System was young such collisions were more common and the rate of dust production was probably many times higher. Zodiacal dust around stars much younger than the Sun has been rarely found. Only a few main-sequence stars have revealed warm (>120 K) zodiacal dust.
Excerpted from Wikipedia’s “BD +20°307” article, available under the CC BY-SA 4.0 licence.