“575 Renate”的意思、由来-开放百科全书

词条	575 Renate
释义	References External links {{Infobox planet \| minorplanet= yes \| background= #D6D6D6 \| name= 575 Renate \| mpc_name= (575) Renate \| alt_names= 1905 RE \| discoverer= M. F. Wolf \| discovered= 19 September 1905 \| discovery_site= Heidelberg \| orbit_ref= \| epoch= 31 July 2016 (JD 2457600.5) \| eccentricity= 0.12796 \| semimajor= {{Convert\|2.5545\|AU\|Gm\|abbr=on}} \| perihelion= {{Convert\|2.2276\|AU\|Gm\|abbr=on}} \| aphelion= {{Convert\|2.8814\|AU\|Gm\|abbr=on\|lk=on}} \| period= 4.08 yr (1491.3 d) \| inclination= 15.012° \| asc_node= 349.682° \| arg_peri= 333.921° \| mean_anomaly= 80.5375° \| rotation= {{Convert\|3.676\|h\|d\|abbr=on\|lk=on}}^[3] \| mean_motion= {{Deg2DMS\|0.24140\|sup=ms}} / day \| observation_arc= 110.31 yr (40292 d) \| uncertainty= 0 \| abs_magnitude= 10.8 \| albedo= {{val\|0.1706\|0.027}} \| mean_radius= {{val\|10.63\|0.75}} km }} Renate (minor planet designation: 575 Renate) is a minor planet orbiting the Sun which was discovered by German astronomer Max Wolf on September 19, 1905. Photometric observations at the Palmer Divide Observatory in Colorado Springs, Colorado in 1999 were used to build a light curve for this object. The asteroid displayed a rotation period of 3.676 ± 0.002 hours and a brightness variation of 0.15 ± 0.01 in magnitude.^[3] This is a member of the dynamic Maria family of asteroids that most likely formed as the result of a collisional breakup of a parent body.^[5] References 1. ^¹²{{Citation \| first1 = Brian D. \| last1 = Warner \| title = Upon Further Review: IV. An Examination of Previous Lightcurve Analysis from the Palmer Divide Observatory \| work = The Minor Planet Bulletin \| volume = 38 \| issue = 1 \| pages = 52–54 \|date=January 2011 \| bibcode = 2011MPBu...38...52W \| postscript= .}} 2. ^¹{{Citation \| last1 = Veeder \| first1 = G. J. \| last2 = Matson \| first2 = D. L. \| last3 = Owensby \| first3 = P. D. \| last4 = Gradie \| first4 = J. C. \| last5 = Bell \| first5 = J. F. \| last6 = Tedesco \| first6 = E. F. \| display-authors = 1 \| title = Eos, Koronis, and Maria family asteroids: Infrared (JHK) photometry \| work = Icarus \| volume = 114 \| pages = 186–196 \|date=March 1995 \| doi = 10.1006/icar.1995.1053 \| bibcode = 1995Icar..114..186V \| citeseerx = 10.1.1.31.2739 \| accessdate= \| postscript= .\| url= https://trs.jpl.nasa.gov/bitstream/2014/29296/1/95-0212.pdf }} ^[1]^[2] }} External links Lightcurve plot of 575 Renate, Palmer Divide Observatory, B. D. Warner (1999) Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center {{JPL small body}} {{Minor planets navigator\|574 Reginhild\|number=575\|576 Emanuela}}{{Small Solar System bodies}}{{DEFAULTSORT:000575}}{{beltasteroid-stub}} 5 : Maria asteroids\|Discoveries by Max Wolf\|Minor planets with names of unknown origin\|Named minor planets\|Astronomical objects discovered in 1905
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