HOPS 383: Difference between revisions
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⚫ | |caption=Infrared images from instruments at Kitt Peak National Observatory (left) and NASA's Spitzer Space Telescope document the outburst of HOPS 383, a young protostar in the Orion star-formation complex. The background is a wide view of the region taken from a Spitzer four-color infrared mosaic. |
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| names = [[Herschel Orion Protostar Survey|HOPS]] 383 |
| names = [[Herschel Orion Protostar Survey|HOPS]] 383 |
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'''HOPS 383''' is a Class 0 [[protostar]]. It is the first class-0 protostar discovered to have had an outburst,<ref name=ScienceDaily-2015-03-24>{{cite news |url= https://www.sciencedaily.com/releases/2015/03/150324183632.htm |title= NASA satellites catch 'growth spurt' from newborn protostar |date= 24 March 2015 |publisher= [[Science Daily]] }}</ref> and as of 2020, the youngest protostar known to have had an outburst.<ref name=ScienceDaily-2015-03-24/> The protostar was discovered by the [[Herschel Orion Protostar Survey]] (HOPS) team.<ref name=USDOD-2015-03-06>{{cite web |url= http://science.dodlive.mil/2015/03/06/nrl-astrophysicist-explores-star-formation-in-orions-belt/ |title= NRL Astrophysicist Explores Star Formation in Orion’s Belt |date= 6 March 2015 |publisher= [[U.S. Department of Defense]] }}</ref> |
'''HOPS 383''' is a Class 0 [[protostar]]. It is the first class-0 protostar discovered to have had an outburst,<ref name=ScienceDaily-2015-03-24>{{cite news |url= https://www.sciencedaily.com/releases/2015/03/150324183632.htm |title= NASA satellites catch 'growth spurt' from newborn protostar |date= 24 March 2015 |publisher= [[Science Daily]] }}</ref> and as of 2020, the youngest protostar known to have had an outburst.<ref name=ScienceDaily-2015-03-24/> The protostar was discovered by the [[Herschel Orion Protostar Survey]] (HOPS) team.<ref name=USDOD-2015-03-06>{{cite web |url= http://science.dodlive.mil/2015/03/06/nrl-astrophysicist-explores-star-formation-in-orions-belt/ |title= NRL Astrophysicist Explores Star Formation in Orion’s Belt |date= 6 March 2015 |publisher= [[U.S. Department of Defense]] }}</ref> |
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==Observations== |
==Observations== |
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==Further reading== |
==Further reading== |
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* {{cite journal |doi=10.1088/2041-8205/800/1/L5 |title=Hops 383: An Outbursting Class 0 Protostar in Orion |year=2015 |last1=Safron |first1=Emily J. |last2=Fischer |first2=William J. |last3=Megeath |first3=S. Thomas |last4=Furlan |first4=Elise |last5=Stutz |first5=Amelia M. |last6=Stanke |first6=Thomas |last7=Billot |first7=Nicolas |last8=Rebull |first8=Luisa M. |last9=Tobin |first9=John J. |last10=Ali |first10=Babar |last11=Allen |first11=Lori E. |last12=Booker |first12=Joseph |last13=Watson |first13=Dan M. |last14=Wilson |first14=T. L. |journal=The Astrophysical Journal |volume=800 |issue=1 |pages=L5 |arxiv=1501.00492 |bibcode=2015ApJ...800L...5S |s2cid=45127705 }} |
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{{Stars of Orion}} |
{{Stars of Orion}} |
Revision as of 20:42, 3 June 2022
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Orion |
Right ascension | 5h 35m 29.81s |
Declination | −4° 59′ 51.1″ |
Characteristics | |
Evolutionary stage | Class 0 protostar |
Astrometry | |
Distance | 1,400 ly (420 pc) |
Other designations | |
HOPS 383 | |
Database references | |
SIMBAD | data |
HOPS 383 is a Class 0 protostar. It is the first class-0 protostar discovered to have had an outburst,[1] and as of 2020, the youngest protostar known to have had an outburst.[1] The protostar was discovered by the Herschel Orion Protostar Survey (HOPS) team.[2]
Observations
Outburst
HOPS 383 had an outburst between 2004 and 2006 (a "dramatic mid-infrared brightening"); the increase in magnitude was detectable at the 24 μm (35 times increase) and 4.5 μm, and was also detectable at the submillimetre.[3] After 6 years, observations showed no signs of fading.[3]
X-Ray
The Chandra X-Ray Observatory detected an X-ray flare from HOPS 383 in December of 2017.[4] This was the first detection of X-rays from a Class 0 protostar that will evolve into a sun-like star.[4] The flare lasted 3 hours and 20 minutes.[5] It significantly impacted the previously-thought timeline for when such events occur in the evolution of a protostar. Furthermore, it has improved astronomers' understanding of the Sun's earlier evolutionary stages.
References
- ^ a b "NASA satellites catch 'growth spurt' from newborn protostar". Science Daily. 24 March 2015.
- ^ "NRL Astrophysicist Explores Star Formation in Orion's Belt". U.S. Department of Defense. 6 March 2015.
- ^ a b Safron, Emily J.; Megeath, S. Thomas; Booker, Joseph; Fischer, William J.; Furlan, Elise; Rebull, Luisa M.; Stutz, Amelia M.; Stanke, Thomas; Billot, Nicolas; Tobin, John J.; Ali, Babar (2015-02-10). "HOPS 383: AN OUTBURSTING CLASS 0 PROTOSTAR IN ORION". Astrophysical Journal Letters. 800 (1). doi:10.1088/2041-8205/800/1/L5. ISSN 2041-8205.
- ^ a b "Chandra :: Photo Album :: HOPS 383 :: June 18, 2020". chandra.harvard.edu. Retrieved 2021-12-29.
- ^ "Chandra Press Room :: X-rays From a Newborn Star Hint at Our Sun's Earliest Days :: 18 June 2020". chandra.harvard.edu. Retrieved 2021-12-30.
Further reading
- Safron, Emily J.; Fischer, William J.; Megeath, S. Thomas; Furlan, Elise; Stutz, Amelia M.; Stanke, Thomas; Billot, Nicolas; Rebull, Luisa M.; Tobin, John J.; Ali, Babar; Allen, Lori E.; Booker, Joseph; Watson, Dan M.; Wilson, T. L. (2015). "Hops 383: An Outbursting Class 0 Protostar in Orion". The Astrophysical Journal. 800 (1): L5. arXiv:1501.00492. Bibcode:2015ApJ...800L...5S. doi:10.1088/2041-8205/800/1/L5. S2CID 45127705.