(126154) 2001 YH140: Difference between revisions
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| name={{mp|(126154) 2001 YH|140}} |
| name={{mp|(126154) 2001 YH|140}} |
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| discovery=yes |
| discovery=yes |
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| discoverer=[[Michael E. Brown]],<br/> [[Chadwick A. Trujillo]]<ref name=iau>{{ |
| discoverer=[[Michael E. Brown]],<br/> [[Chadwick A. Trujillo]]<ref name=iau>{{Cite web|url=http://cfa-www.harvard.edu/iau/lists/TNOs.html|title=List Of Transneptunian Objects|accessdate=August 2, 2010|publisher=IAU Minor Planet Center}}</ref> |
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| discovered=December 18, 2001 |
| discovered=December 18, 2001 |
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| mp_name={{mp|(126154) 2001 YH|140}} |
| mp_name={{mp|(126154) 2001 YH|140}} |
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| alt_names=''none'' |
| alt_names=''none'' |
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| mp_category=[[trans-Neptunian object|TNO]] ([[ |
| mp_category=[[trans-Neptunian object|TNO]] ([[Resonant trans-Neptunian object|Resonant]])<ref name="MPEC 2009-R09">{{Cite web |
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|title=MPEC 2009-R09 : |
|title=MPEC 2009-R09 :Distant Minor Planets (2009 SEPT. 16.0 TT) |
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|date=2009-09-04 |
|date=2009-09-04 |
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|publisher=IAU Minor Planet Center |
|publisher=IAU Minor Planet Center |
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| arg_peri=354.4° |
| arg_peri=354.4° |
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| mean_anomaly=13.5° |
| mean_anomaly=13.5° |
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| orbit_ref=<ref name=iau/><ref name="jpldata">{{ |
| orbit_ref=<ref name=iau/><ref name="jpldata">{{Cite web |
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|date=2009-02-02 last obs |
|date=2009-02-02 last obs |
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|title=JPL Small-Body Database Browser: (126154) 2001 YH140 |
|title=JPL Small-Body Database Browser: (126154) 2001 YH140 |
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| abs_magnitude=5.8<ref name=Muller2010/> |
| abs_magnitude=5.8<ref name=Muller2010/> |
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| albedo=0.06–0.10<ref name=Muller2010/> |
| albedo=0.06–0.10<ref name=Muller2010/> |
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| spectral_type = |
| spectral_type = |
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| single_temperature=~42 [[kelvin|K]]}} |
| single_temperature=~42 [[kelvin|K]]}} |
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'''{{mp|(126154) 2001 YH|140}}''', also written as '''(126154) 2001 YH140''', is a resonant trans-neptunian object discovered on December 18, 2001 by C. A. Trujillo, M. E. Brown. |
'''{{mp|(126154) 2001 YH|140}}''', also written as '''(126154) 2001 YH140''', is a resonant trans-neptunian object discovered on December 18, 2001 by C. A. Trujillo, M. E. Brown. |
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==Orbit and rotation== |
==Orbit and rotation== |
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(126154) 2001 YH140 is locked in the 5:3 mean motion resonance with [[Neptune]].<ref name=Muller2010/> When it makes three revolutions around the Sun, Neptune makes exactly five. The rotation period of 2001 YH140 is estimated to be {{nowrap|13.25 ± 0.2 hours}}.<ref name=Sheppard2007>{{ |
(126154) 2001 YH140 is locked in the 5:3 mean motion resonance with [[Neptune]].<ref name=Muller2010/> When it makes three revolutions around the Sun, Neptune makes exactly five. The rotation period of 2001 YH140 is estimated to be {{nowrap|13.25 ± 0.2 hours}}.<ref name=Sheppard2007>{{Cite journal|last=Sheppard|first=Scott S.|title=Light Curves of Dwarf Plutonian Planets and other Large Kuiper Belt Objects: Their Rotations, Phase Functions, and Absolute Magnitudes|year=2007|journal=The Astronomical Journal|volume=134 |doi=10.1086/519072|pages=787–798|url=http://adsabs.harvard.edu/abs/2007AJ....134..787S}}</ref> |
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==Physical characteristics== |
==Physical characteristics== |
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In 2010 thermal flux from 2001 YH140 in the [[far-infrared]] was measured by the [[Herschel Space Telescope]]. As a result its equivalent size was estimated to lie within a range from 300 to 390 km.<ref name=Muller2010>{{ |
In 2010 thermal flux from 2001 YH140 in the [[far-infrared]] was measured by the [[Herschel Space Telescope]]. As a result its equivalent size was estimated to lie within a range from 300 to 390 km.<ref name=Muller2010>{{Cite journal|last=Muller|first=T.G.|coauthors=Lellouch, E.; Stansberry, J. ''et al.''|title=“TNOs are Cool”: A survey of the trans-Neptunian region I. Results from the Herschel science demonstration phase (SDP)|journal=Astronomy and Astrophysics|volume=518|year=2010|page=L146|doi=10.1051/0004-6361/201014683|url=http://adsabs.harvard.edu/abs/2010A%26A...518L.146M}}</ref> |
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==References== |
==References== |
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{{ |
{{Reflist}} |
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{{MinorPlanets Navigator|(126153) 2001 YN139|PageName={{mp|(126154) 2001 YH|140}}|(126155) 2001 YJ140}} |
{{MinorPlanets Navigator|(126153) 2001 YN139|PageName={{mp|(126154) 2001 YH|140}}|(126155) 2001 YJ140}} |
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{{Trans-Neptunian objects}} |
{{Trans-Neptunian objects}} |
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{{DEFAULTSORT:2001 |
{{DEFAULTSORT:2001 Yh140}} |
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{{CentaurTNO-stub}} |
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Revision as of 11:05, 26 September 2010
Discovery | |
---|---|
Discovered by | Michael E. Brown, Chadwick A. Trujillo[1] |
Discovery date | December 18, 2001 |
Designations | |
Designation | (126154) 2001 YH140 |
none | |
TNO (Resonant)[2] | |
Orbital characteristics[1][3] | |
Epoch December 31, 2006 (JD 2454100.5) | |
Aphelion | 48.39 AU |
Perihelion | 36.368 AU |
42.204 AU) | |
Eccentricity | 0.138 |
100297.827 d (274.60 a) | |
13.5° | |
Inclination | 11.1° |
108.9° | |
354.4° | |
Physical characteristics | |
Dimensions | 345 ± 45 km[4] |
Mass | ~4.0×1019 kg |
Mean density | 2.0 g/cm³ (assumed) |
~0.09 m/s² | |
~0.18 km/s | |
13.25 ± 0.2 h[5] | |
Albedo | 0.06–0.10[4] |
Temperature | ~42 K |
5.8[4] | |
(126154) 2001 YH140, also written as (126154) 2001 YH140, is a resonant trans-neptunian object discovered on December 18, 2001 by C. A. Trujillo, M. E. Brown.
Orbit and rotation
(126154) 2001 YH140 is locked in the 5:3 mean motion resonance with Neptune.[4] When it makes three revolutions around the Sun, Neptune makes exactly five. The rotation period of 2001 YH140 is estimated to be 13.25 ± 0.2 hours.[5]
Physical characteristics
In 2010 thermal flux from 2001 YH140 in the far-infrared was measured by the Herschel Space Telescope. As a result its equivalent size was estimated to lie within a range from 300 to 390 km.[4]
References
- ^ a b "List Of Transneptunian Objects". IAU Minor Planet Center. Retrieved August 2, 2010.
- ^ "MPEC 2009-R09 :Distant Minor Planets (2009 SEPT. 16.0 TT)". IAU Minor Planet Center. 2009-09-04. Retrieved 2009-10-04.
- ^ "JPL Small-Body Database Browser: (126154) 2001 YH140". 2009-02-02 last obs. Retrieved 2010-08-03.
{{cite web}}
: Check date values in:|date=
(help) - ^ a b c d e Muller, T.G. (2010). ""TNOs are Cool": A survey of the trans-Neptunian region I. Results from the Herschel science demonstration phase (SDP)". Astronomy and Astrophysics. 518: L146. doi:10.1051/0004-6361/201014683.
{{cite journal}}
: Unknown parameter|coauthors=
ignored (|author=
suggested) (help) - ^ a b Sheppard, Scott S. (2007). "Light Curves of Dwarf Plutonian Planets and other Large Kuiper Belt Objects: Their Rotations, Phase Functions, and Absolute Magnitudes". The Astronomical Journal. 134: 787–798. doi:10.1086/519072.