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{{Short description|Main belt asteroid}} |
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{{Use dmy dates|date=October 2019}} |
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{{Infobox planet |
{{Infobox planet |
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| minorplanet=yes |
| minorplanet=yes |
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| background=# |
| background=#D6D6D6 |
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| name=264 Libussa |
| name=264 Libussa |
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| image= |
| image=264Libussa (Lightcurve Inversion).png |
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| image_scale = |
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| caption=A three-dimensional model of 264 Libussa based on its light curve |
| caption=A three-dimensional model of 264 Libussa based on its light curve |
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| discoverer=[[Christian Heinrich Friedrich Peters|C. H. F. Peters]] |
| discoverer=[[Christian Heinrich Friedrich Peters|C. H. F. Peters]] |
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| discovered=22 December 1886 |
| discovered=22 December 1886 |
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| mpc_name=(264) Libussa |
| mpc_name=(264) Libussa |
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| pronounced= {{IPA-de|ˈliːbʊsaː|lang}} |
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| alt_names= |
| alt_names=A886 YA |
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| named_after=[[Libuše]] |
| named_after=[[Libuše]] |
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| mp_category=[[Asteroid belt|Main belt]] |
| mp_category=[[Asteroid belt|Main belt]] |
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| mass= |
| mass= |
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| density= |
| density= |
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| surface_grav= |
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| escape_velocity= |
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| rotation={{Convert|9.2276|h|d|abbr=on|lk=on}}<ref name="JPL"/><ref name="Pilcher2009"/> |
| rotation={{Convert|9.2276|h|d|abbr=on|lk=on}}<ref name="JPL"/><ref name="Pilcher2009"/> |
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| spectral_type=[[S-type asteroid|S]] |
| spectral_type=[[S-type asteroid|S]] |
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| observation_arc=123.02 yr (44934 d) |
| observation_arc=123.02 yr (44934 d) |
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| uncertainty=0 |
| uncertainty=0 |
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| moid={{Convert|1.42116|AU|Gm|abbr=on}} |
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| jupiter_moid={{Convert|2.25369|AU|Gm|abbr=on}} |
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| tisserand=3.289 |
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}} |
}} |
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'''264 Libussa''' is a [[Asteroid belt|Main belt]] [[asteroid]] that was discovered by [[Christian Heinrich Friedrich Peters|C. H. F. Peters]] on December 22, 1886 in [[Clinton, Oneida County, New York|Clinton, New York]] and was named after [[Libussa]], the legendary founder of [[Prague]]. It is classified as an [[S-type asteroid]]. |
'''Libussa''' ([[minor planet designation]]: '''264 Libussa''') is a [[Asteroid belt|Main belt]] [[asteroid]] that was discovered by [[Christian Heinrich Friedrich Peters|C. H. F. Peters]] on December 22, 1886, in [[Clinton, Oneida County, New York|Clinton, New York]] and was named after [[Libuše|Libussa]], the legendary founder of [[Prague]].<ref>{{cite book | chapter=(264) Libussa | title=Dictionary of Minor Planet Names – (264) Libussa | publisher=[[Springer Berlin Heidelberg]] | date=2007 | last=Schmadel | first=Lutz D. | page=38 | isbn=978-3-540-00238-3 | doi=10.1007/978-3-540-29925-7_265}}</ref> It is classified as an [[S-type asteroid]]. |
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[[Photometry (astronomy)|Photometric]] observations of this asteroid at the Organ Mesa Observatory in [[Las Cruces, New Mexico]] in 2008 gave an asymmetrical, bimodal [[light curve]] with a period of 9.2276 ± 0.0002 hours and a brightness variation of 0.33 ± 0.03 in [[Magnitude (astronomy)|magnitude]].<ref name="Pilcher2009"/> Observation from the [[W. M. Keck Observatory]] show an [[angular size]] of 57 mas, which is close to the resolution limit of the instrument. The estimated maximum size of the asteroid is about 66 ± 7 km. It has an asymmetrical shape with a size ratio of more than 1.22 between the major and minor axes.<ref name="Marchis2006"/> |
[[Photometry (astronomy)|Photometric]] observations of this asteroid at the Organ Mesa Observatory in [[Las Cruces, New Mexico]], in 2008 gave an asymmetrical, bimodal [[light curve]] with a period of 9.2276 ± 0.0002 hours and a brightness variation of 0.33 ± 0.03 in [[Magnitude (astronomy)|magnitude]].<ref name="Pilcher2009"/> Observation from the [[W. M. Keck Observatory]] show an [[angular size]] of 57 mas, which is close to the resolution limit of the instrument. The estimated maximum size of the asteroid is about 66 ± 7 km. It has an asymmetrical shape with a size ratio of more than 1.22 between the major and minor axes.<ref name="Marchis2006"/> |
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Between 2005 and 2021, 264 Libussa has been observed to [[Occultation|occult]] five stars. |
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==References== |
==References== |
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{{Reflist|refs= |
{{Reflist|refs= |
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<ref name="JPL">{{Citation | first1=Donald K. | last1=Yeomans | url=https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=264 | title=264 Libussa | publisher=[[NASA Jet Propulsion Laboratory]] | accessdate=11 May 2016 | postscript=. | work=JPL Small-Body Database Browser}}</ref> |
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<ref name="JPL">{{Citation |
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| first1 = Donald K. |
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| last1 = Yeomans |
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| title = 264 Libussa |
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| work = JPL Small-Body Database Browser |
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| publisher = NASA Jet Propulsion Laboratory |
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| url = http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=264 |
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| accessdate= 11 May 2016 |
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| postscript= . |
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}}</ref> |
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<ref name="Pilcher2009">{{Citation | bibcode=2009MPBu...36...52P | first1=Frederick | last1=Pilcher | last2=Jardine | first2=Don | title=Period Determinations for 31 Euphrosyne, 35 Leukothea 56 Melete, 137 Meliboea, 155 Scylla, and 264 Libussa | journal=The Minor Planet Bulletin | volume=36 | issue=2 | date=April 2009 | pages=52–54}}</ref> |
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<ref name="Pilcher2009">{{citation |
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| last1=Pilcher |
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| first1=Frederick |
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| last2=Jardine |
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| first2=Don |
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| title=Period Determinations for 31 Euphrosyne, 35 Leukothea 56 Melete, 137 Meliboea, 155 Scylla, and 264 Libussa |
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| journal=The Minor Planet Bulletin |
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| volume=36 |
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| issue=2 |
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| pages=52–54 |
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|date=April 2009 |
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| bibcode=2009MPBu...36...52P |
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}}</ref> |
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<ref name="Marchis2006">{{Citation | bibcode=2006Icar..185...39M | display-authors=1 | first1=F. | first2=M. | first3=E. F. Y. | first4=J. | first5=J. | first6=D. | first7=D. | first8=I. | last1=Marchis | last2=Kaasalainen | last3=Hom | last4=Berthier | last5=Enriquez | last6=Hestroffer | last7=Le Mignant | last8=de Pater | pmc=2600456 | pmid=19081813 | url=http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006Icar..185...39M&link_type=EJOURNAL&db_key=AST&high= | title=Shape, size and multiplicity of main-belt asteroids. I. Keck Adaptive Optics survey | journal=Icarus | volume=185 | issue=1 | date=November 2006 | pages=39–63 | doi=10.1016/j.icarus.2006.06.001 | accessdate=2013-03-27 | postscript=.}}</ref> |
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<ref name="Marchis2006">{{Citation |
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| first1 = F. |
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| last1 = Marchis |
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| first2 = M. |
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| last2 = Kaasalainen |
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| first3 = E. F. Y. |
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| last3 = Hom |
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| first4 = J. |
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| last4 = Berthier |
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| first5 = J. |
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| last5 = Enriquez |
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| first6 = D. |
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| last6 = Hestroffer |
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| first7 = D. |
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| last7 = Le Mignant |
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| first8 = I. |
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| last8 = de Pater |
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| display-authors = 1 |
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| title = Shape, size and multiplicity of main-belt asteroids. I. Keck Adaptive Optics survey |
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| work = Icarus |
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| volume = 185 |
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| issue = 1 |
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| pages = 39–63 |
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| date = November 2006 |
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| accessdate= 2013-03-27 |
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| url = http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006Icar..185...39M&link_type=EJOURNAL&db_key=AST&high= |
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| bibcode = 2006Icar..185...39M |
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| doi = 10.1016/j.icarus.2006.06.001 |
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| postscript= . |
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| pmid=19081813 |
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| pmc=2600456 |
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}}</ref> |
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}} |
}} |
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==External links== |
==External links== |
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* [ |
* [http://ftp.lowell.edu/pub/elgb/astorb.html The Asteroid Orbital Elements Database] |
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* [http://cfa-www.harvard.edu/iau/lists/NumberedMPs.html Minor Planet Discovery Circumstances] |
* [http://cfa-www.harvard.edu/iau/lists/NumberedMPs.html Minor Planet Discovery Circumstances] |
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* [http://spiff.rit.edu/richmond/parallax/phot/LCSUMPUB.TXT Asteroid Lightcurve Data File] |
* [http://spiff.rit.edu/richmond/parallax/phot/LCSUMPUB.TXT Asteroid Lightcurve Data File] |
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* {{AstDys|264}} |
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* {{JPL small body}} |
* {{JPL small body}} |
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{{Minor planets navigator|263 Dresda|number=264|265 Anna}} |
{{Minor planets navigator |263 Dresda |number=264 |265 Anna}} |
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{{Small Solar System bodies}} |
{{Small Solar System bodies}} |
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{{Authority control}} |
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{{DEFAULTSORT:000264}} |
{{DEFAULTSORT:000264}} |
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[[Category: |
[[Category:Background asteroids]] |
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[[Category:Numbered minor planets]] |
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[[Category:Discoveries by Christian Peters|Libussa]] |
[[Category:Discoveries by Christian Peters|Libussa]] |
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[[Category:Named minor planets|Libussa]] |
[[Category:Named minor planets|Libussa]] |
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[[Category:S-type asteroids (SMASS)]] |
[[Category:S-type asteroids (SMASS)]] |
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[[Category:Astronomical objects discovered in 1886|18861222]] |
[[Category:Astronomical objects discovered in 1886|18861222]] |
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[[Category:Objects observed by stellar occultation]] |
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![]()
A three-dimensional model of 264 Libussa based on its light curve
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Discovery | |
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Discovered by | C. H. F. Peters |
Discovery date | 22 December 1886 |
Designations | |
(264) Libussa | |
Pronunciation | German: [ˈliːbʊsaː] |
Named after | Libuše |
A886 YA | |
Main belt | |
Orbital characteristics[1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 123.02 yr (44934 d) |
Aphelion | 3.1799 AU (475.71 Gm) |
Perihelion | 2.41375 AU (361.092 Gm) |
2.79681 AU (418.397 Gm) | |
Eccentricity | 0.13696 |
4.68 yr (1708.4 d) | |
Average orbital speed | 17.81 km/s |
254.88° | |
0° 12m 38.592s / day | |
Inclination | 10.426° |
49.608° | |
340.891° | |
Physical characteristics | |
Dimensions | 50.48±2.7 km |
9.2276 h (0.38448 d)[1][2] | |
0.2971±0.034 | |
S | |
8.42 | |
Libussa (minor planet designation: 264 Libussa) is a Main belt asteroid that was discovered by C. H. F. Peters on December 22, 1886, in Clinton, New York and was named after Libussa, the legendary founder of Prague.[3] It is classified as an S-type asteroid.
Photometric observations of this asteroid at the Organ Mesa Observatory in Las Cruces, New Mexico, in 2008 gave an asymmetrical, bimodal light curve with a period of 9.2276 ± 0.0002 hours and a brightness variation of 0.33 ± 0.03 in magnitude.[2] Observation from the W. M. Keck Observatory show an angular size of 57 mas, which is close to the resolution limit of the instrument. The estimated maximum size of the asteroid is about 66 ± 7 km. It has an asymmetrical shape with a size ratio of more than 1.22 between the major and minor axes.[4]
Between 2005 and 2021, 264 Libussa has been observed to occult five stars.
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