202 Chryseïs: Difference between revisions

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{{Use dmy dates|date=October 2019}}
{{Use dmy dates|date=October 2019}}
{{Infobox planet
{{Infobox planet
| minorplanet=yes
| minorplanet = yes
|image= Орбита астероида 202.png
| image = 202 Chryseïs.png
|caption=Orbital diagram
| caption = [[Lightcurve]]-base 3D-model of 202 Chryseïs.
| background=#D6D6D6
| background = #D6D6D6
| name=202 Chryseïs
| name = 202 Chryseïs
| discoverer=[[Christian Heinrich Friedrich Peters|C. H. F. Peters]]
| discoverer = [[Christian Heinrich Friedrich Peters|C. H. F. Peters]]
| discovered=11 September 1879
| discovered = 11 September 1879
| mpc_name=(202) Chryseïs
| mpc_name = (202) Chryseïs
| alt_names=A879 RA, A901 TA<br/>1935 BL
| alt_names = A879 RA, A901 TA<br/>1935 BL
| pronounced={{IPAc-en|k|r|aɪ|ˈ|s|iː|ᵻ|s}}<ref>Noah Webster (1884) ''A Practical Dictionary of the English Language''</ref>
| pronounced = {{IPAc-en|k|r|aɪ|ˈ|s|iː|ᵻ|s}}<ref>Noah Webster (1884) ''A Practical Dictionary of the English Language''</ref>
| named_after=[[Chryseis]]
| named_after = [[Chryseis]]
| mp_category=[[Asteroid belt|Main belt]]
| mp_category = [[Asteroid belt|Main belt]]
| epoch=31 July 2016 ([[Julian day|JD]] 2457600.5)
| epoch = 31 July 2016 ([[Julian day|JD]] 2457600.5)
| semimajor={{Convert|3.0713|AU|Gm|abbr=on}}
| semimajor = {{Convert|3.0713|AU|Gm|abbr=on}}
| perihelion={{Convert|2.7567|AU|Gm|abbr=on}}
| perihelion = {{Convert|2.7567|AU|Gm|abbr=on}}
| aphelion={{Convert|3.3859|AU|Gm|abbr=on|lk=on}}
| aphelion = {{Convert|3.3859|AU|Gm|abbr=on|lk=on}}
| eccentricity=0.10244
| eccentricity = 0.10244
| period=5.38 [[Julian year (astronomy)|yr]] (1966.0 [[Julian year (astronomy)|d]])
| period = 5.38 [[Julian year (astronomy)|yr]] (1966.0 [[Julian year (astronomy)|d]])
| inclination=8.8535°
| inclination = 8.8535°
| asc_node=136.848°
| asc_node = 136.848°
| arg_peri=1.3159°
| arg_peri = 1.3159°
| mean_anomaly=11.1527[[Degree (angle)|°]]
| mean_anomaly = 11.1527[[Degree (angle)|°]]
| avg_speed=16.99 km/s
| avg_speed = 16.99 km/s
| dimensions={{val|86.15|2.4|ul=km}}
| dimensions = {{val|86.15|2.4|ul=km}}
| mass=
| mass =  
| density=
| density =  
| rotation={{Convert|23.670|h|d|abbr=on|lk=on}}<ref name="jpldata"/><br />23.670 ± 0.001 h<ref name="aaa555_A104"/>
| rotation = {{Convert|23.670|h|d|abbr=on|lk=on}}<ref name="jpldata"/><br />23.670 ± 0.001 h<ref name="aaa555_A104"/>
| spectral_type=[[S-type asteroid|S]]
| spectral_type = [[S-type asteroid|S]]
| abs_magnitude=7.42
| abs_magnitude = 7.42
| albedo={{val|0.2562|0.015}}
| albedo = {{val|0.2562|0.015}}
| single_temperature=
| single_temperature =  
| mean_motion={{Deg2DMS|0.18311|sup=ms}} / day
| mean_motion = {{Deg2DMS|0.18311|sup=ms}} / day
| orbit_ref=<ref name="jpldata">{{Cite web |url=https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=202;cad=1 |title=202 Chryseis |work=[[JPL Small-Body Database]] |publisher=[[NASA]]/[[Jet Propulsion Laboratory]] |access-date=12 May 2016}}</ref>
| orbit_ref = <ref name="jpldata">{{Cite web |url=https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=202;cad=1 |title=202 Chryseis |work=[[JPL Small-Body Database]] |publisher=[[NASA]]/[[Jet Propulsion Laboratory]] |access-date=12 May 2016}}</ref>
| observation_arc=136.57 yr (49881 d)
| observation_arc = 136.57 yr (49881 d)
| uncertainty=0
| uncertainty = 0
}}
}}


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==References==
==References==
{{reflist|refs=
<references>


<ref name="aaa555_A104">{{citation | display-authors=1
<ref name="aaa555_A104">{{citation | display-authors=1
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  | date=October 2011 | bibcode=2011MPBu...38..208S | postscript=. }}</ref>
  | date=October 2011 | bibcode=2011MPBu...38..208S | postscript=. }}</ref>


}} <!-- end of reflist -->
</references> <!-- end of reflist -->


== External links ==
== External links ==

Latest revision as of 15:50, 25 December 2025

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202 Chryseïs is a large, lightly coloured Main belt asteroid that is probably composed of silicate rocks. It was discovered by C. H. F. Peters on September 11, 1879, in Clinton, New York, and was named after the mythical Trojan woman Chryseis.

The rotation period for this asteroid is close to a day long, so the construction of a complete light curve requires photometric observations from multiple locations at widely spaced latitudes. This task was completed in January and February, 2011, yielding a synodic rotation period of 23.670 ± 0.001 h, with a brightness variation of 0.20 ± 0.02 in magnitude[1]

References

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External links

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