339 Dorothea

{{Short description|Main-belt asteroid}}

{{Use dmy dates|date=October 2019}}

{{Infobox planet

| minorplanet=yes

| background=#D6D6D6

| name=339 Dorothea

| discoverer=Max Wolf

| discovered=25 September 1892

| mpc_name=(339) Dorothea

| alt_names=1892 G

|image= Орбита астероида 339.png

|caption=Orbital diagram

| pronounced= {{IPAc-en|d|ɒ|ə|'|θ|iː|ə}}Noah Webster (1884) A Practical Dictionary of the English Language

| named_after=Dorothea Klumpke

| mp_category=Main belt (Eos)

| orbit_ref=

| epoch=31 July 2016 (JD 2457600.5)

| semimajor={{Convert|3.01176|AU|Gm|abbr=on}}

| perihelion={{Convert|2.71937|AU|Gm|abbr=on}}

| aphelion={{Convert|3.3041|AU|Gm|abbr=on|lk=on}}

| eccentricity=0.097082

| period=5.23 yr (1909.1 d)

| inclination=9.9640°

| asc_node=173.512°

| arg_peri=164.360°

| mean_anomaly=271.598°

| dimensions={{val|38.25|1.6|ul=km}}

| mass=

| density=

| rotation={{Convert|5.974|h|d|abbr=on|lk=on}}

| spectral_type=S {{small|(Tholen)}}
K {{small|(SMASSII)}}

| abs_magnitude=9.24

| albedo={{val|0.2431|0.021}}

| mean_motion={{Deg2DMS|0.188570|sup=ms}} / day

| observation_arc=123.55 yr (45128 d)

| uncertainty=0

}}

339 Dorothea is a large main belt asteroid that was discovered by German astronomer Max Wolf on 25 September 1892 in Heidelberg.

This is a member of the dynamic Eos family of asteroids that were probably formed as the result of a collisional breakup of a parent body.

This asteroid is named after astronomer Dorothea Klumpke,[https://www.vaticanobservatory.org/sacred-space-astronomy/specola-guestbook-december-29-1908/ Vatican Observatory website] as is 1040 Klumpkea.

References

{{Reflist|refs=

{{Citation

| first1 = Donald K.

| last1 = Yeomans

| title = 339 Dorothea

| work = JPL Small-Body Database Browser

| publisher = NASA Jet Propulsion Laboratory

| url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=339

| access-date= 11 May 2016

| postscript= .

}}

{{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

| url = http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995Icar..114..186V&link_type=EJOURNAL&db_key=AST&high=

| citeseerx = 10.1.1.31.2739

| access-date= 2013-04-06

| postscript= .

}}

}}