540 Rosamunde

{{Use dmy dates|date=June 2017}}

{{Infobox planet

| minorplanet= yes

| image= 540Rosamunde (Lightcurve Inversion).png

| image_scale =

| caption= A three-dimensional model of 540 Rosamunde based on its light curve

| background= #D6D6D6

| name= 540 Rosamunde

| mpc_name= (540) Rosamunde

| pronounced= {{IPA|de|ʁoːzɐˈmʊndə|lang}}[https://www.germannames.de/wiki/Rosamunde (German Names)]

| alt_names= 1904 ON

| discoverer= Max Wolf

| discovered= 3 August 1904

| discovery_site= Heidelberg

| epoch= 31 July 2016 (JD 2457600.5)

| eccentricity= 0.089767

| semimajor= {{Convert|2.2187|AU|Gm|abbr=on}}

| perihelion= {{Convert|2.0195|AU|Gm|abbr=on}}

| aphelion= {{Convert|2.4178|AU|Gm|abbr=on|lk=on}}

| period= 3.30 yr (1207.1 d)

| inclination= 5.5831°

| asc_node= 202.174°

| arg_peri= 337.564°

| mean_anomaly= 85.2863°

| mean_motion= {{Deg2DMS|0.29824|sup=ms}} / day

| orbit_ref= {{Cite web |url=https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=540;cad=1 |title=540 Rosamunde (1904 ON) |work=JPL Small-Body Database |publisher=NASA/Jet Propulsion Laboratory |access-date=5 May 2016}}

| observation_arc= 111.67 yr (40788 d)

| uncertainty= 0

| abs_magnitude= 10.76

| rotation= {{Convert|9.351|+/-|0.001|h|d|abbr=on|lk=on}}

| albedo= {{val|0.2426|0.088}}

| mean_radius= {{val|9.51|1.35}} km

}}

540 Rosamunde is an S-type asteroid[https://web.archive.org/web/20061201092811/http://www.psi.edu/pds/resource/taxonomy.html] belonging to the Flora family in the Main Belt. Its diameter is about 19 km and it has an albedo of 0.243 [https://web.archive.org/web/20070119015129/http://www.psi.edu/pds/resource/imps.html]. Its rotation period is 9.336 hours[https://archive.today/20060614093519/http://www.psi.edu/pds/archive/lc.html].

Rosamunde is named for a character in a play of the same title for which Franz Schubert wrote incidental music.{{cite book|author=Lutz D. Schmadel|title=Dictionary of Minor Planet Names|url=https://books.google.com/books?id=eHv1CAAAQBAJ&pg=PA87|year=2013|publisher=Springer Science & Business Media|isbn=978-3-662-06615-7|page=87}}

References

{{Reflist|refs=

{{cite journal

| display-authors=1

| last1=Kryszczynska | first1=A. | last2=Colas | first2=F.

| last3=Polinska | first3=M. | last4=Hirsch | first4=R.

| last5=Ivanova | first5=V. | last6=Apostolovska | first6=G.

| last7=Bilkina | first7=B. | last8=Velichko | first8=F. P.

| last9=Kwiatkowski | first9=T. | last10=Kankiewicz | first10=P.

| last11=Vachier | first11=F. | last12=Umlenski | first12=V.

| last13=Michalowski | first13=T. | last14=Marciniak | first14=A.

| last15=Maury | first15=A. | last16=Kaminski | first16=K.

| last17=Fagas | first17=M. | last18=Dimitrov | first18=W.

| last19=Borczyk | first19=W. | last20=Sobkowiak | first20=K.

| last21=Lecacheux | first21=J. | last22=Behrend | first22=R.

| last23=Klotz | first23=A. | last24=Bernasconi | first24=L.

| last25=Crippa | first25=R. | last26=Manzini | first26=F.

| last27=Poncy | first27=R. | last28=Antonini | first28=P.

| last29=Oszkiewicz | first29=D. | last30=Santana-Ros | first30=T.

| title=Do Slivan states exist in the Flora family?. I. Photometric survey of the Flora region

| journal=Astronomy & Astrophysics

| volume=546 | id=A72 | pages=51 | date=October 2012

| bibcode=2012A&A...546A..72K | doi=10.1051/0004-6361/201219199

| doi-access=free }}

}}