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- V883 Orionis is a protostar in the constellation of Orion. It is associated with IC 430 (Haro 13A), a peculiar Hα object surveyed by Guillermo Haro in 1952. It is assumed to be a member of the Orion Nebula cluster at 414±7 pc. 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. (en)
- 獵戶座V883（V883 Orionis）是一顆在天球上位於獵戶座的原恆星。 (zh)
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- 3793 (xsd:nonNegativeInteger)
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- V883 Orionis is a protostar in the constellation of Orion. It is associated with IC 430 (Haro 13A), a peculiar Hα object surveyed by Guillermo Haro in 1952. It is assumed to be a member of the Orion Nebula cluster at 414±7 pc. 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. (en)
- 獵戶座V883（V883 Orionis）是一顆在天球上位於獵戶座的原恆星。 (zh)
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- V883 Orionis (en)
- 獵戶座V883 (zh)
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