V883 Orionis
Appearance
Observation data Epoch J2000 Equinox J2000 | |
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Constellation | Orion |
Right ascension | 05h 38m 18.102s[1] |
Declination | −07° 02′ 26.02″[1] |
Characteristics | |
Variable type | FU Ori |
Details | |
Myr | |
V883 Ori, HBC 489 | |
Database references | |
SIMBAD | data |
V883 Orionis is a
V883 Orionis, like most protostars, is surrounded by a circumstellar disc of dust. The dust has a water snow-line, a certain distance where the stellar irradiance from the star is low enough that water can freeze to snow. The water snow-line was directly imaged by ALMA, when a stellar outburst increased the amount of insolation and pushed the line out farther.[2] In 2023, it was announced that signs of water vapor had been detected in V883 Orionis' disc.[5]
Gallery
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Artist's impression of the planet-forming disc around V883 Orionis
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Informative video about the planet-forming disc around V883 Orionis
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Artist's impression of the water snow line around V883 Orionis, detected with ALMA
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IC 429 and IC 430 next to the bright foreground star49 Ori. V883 Ori is the faint star just beyond the tip of IC 429.
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V883 Ori (bright star) and part of IC 429 with the Hubble Space Telescope
References
- ^ S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ S2CID 205249709.
- .
- .
- ESO. 8 March 2023. Retrieved 21 March 2023.