200 Dynamene

{{Short description|Main-belt asteroid}}

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

{{Infobox planet

| minorplanet= yes

| mpc_name= (200) Dynamene

| background= #D6D6D6

| image= Орбита астероида 200.png

| caption=Orbital diagram

| name= 200 Dynamene

| alt_names= A879 OA; 1904 CA;
1955 HZ; {{mp|1961 TO|1}};
{{mp|1974 HE|1}}

| pronounced={{IPAc-en|d|aɪ|'|n|æ|m|ᵻ|n|iː}}Noah Webster (1884) A Practical Dictionary of the English Language

| discoverer= C. H. F. Peters, 1879

| mp_category= Main belt

| orbit_ref=

| semimajor= {{Convert|2.7374|AU|Gm|abbr=on}}

| perihelion= {{Convert|2.3728|AU|Gm|abbr=on}}

| aphelion= {{Convert|3.1020|AU|Gm|abbr=on|lk=on}}

| period= 4.53 yr (1654.3 d)

| inclination= 6.8957°

| eccentricity= 0.13320

| dimensions= {{val|128.36|2.1|ul=km}}
130.71 ± 3.01 km

| mass= {{nowrap|(1.07 ± 0.16) × 1019 kg}}

| density= 9.14 ± 1.51 g/cm3

| rotation= {{Convert|37.394|h|d|abbr=on|lk=on}}

| spectral_type= C

| abs_magnitude= 8.26

| albedo= {{val|0.0533|0.002}}

| discovered= 27 July 1879

| epoch= 31 July 2016 (JD 2457600.5)

| asc_node= 324.57°

| arg_peri= 85.089°

| mean_anomaly= 10.506°

| mean_motion= {{Deg2DMS|0.21762|sup=ms}} / day

| observation_arc= 136.47 yr (49845 d)

| uncertainty= 0

| moid= {{Convert|1.39358|AU|Gm|abbr=on}}

| jupiter_moid= {{Convert|2.2934|AU|Gm|abbr=on}}

| tisserand= 3.328

}}

200 Dynamene is a large dark main-belt asteroid that was discovered by German-American astronomer Christian Heinrich Friedrich Peters on July 27, 1879, in Clinton, New York. The name derives from Dynamene, one of the fifty Nereids in Greek mythology. Based upon its spectrum, 200 Dynamene is classified as a C-type asteroid, indicating that it probably has a primitive composition similar to the carbonaceous chondrite meteorites. The spectra of the asteroid displays evidence of aqueous alteration.

Photometric observations of this asteroid at the Organ Mesa Observatory in Las Cruces, New Mexico in 2011 gave a light curve with a period of 37.394 ± 0.002 hours and a brightness variation of 0.10 ± 0.01 in magnitude. The curve is asymmetrical with four uneven minima and maxima.

Occultation data from October 9, 2006, using 15 chords shows the asteroid is about 130 km in diameter.

References

{{Reflist|refs=

{{Citation

| title = 200 Dynamene

| work = JPL Small-Body Database Browser

| publisher = NASA Jet Propulsion Laboratory

| url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=200

| accessdate= 12 May 2016

| postscript= .}}

{{citation

| title=Spectroscopic comparison of aqueous altered asteroids with CM2 carbonaceous chondrite meteorites

| display-authors=1 | postscript=.

| last1=Fornasier | first1=S. | last2=Lazzarin | first2=M.

| last3=Barbieri | first3=C. | last4=Barucci | first4=M. A.

| journal=Astronomy and Astrophysics Supplement

| volume=135 | pages=65−73 | date=February 1999

| doi=10.1051/aas:1999161 | bibcode=1999A&AS..135...65F | doi-access=free | url=https://ui.adsabs.harvard.edu/link_gateway/1999A&AS..135...65F/PUB_PDF }}

{{Citation

| first1 = B.

| last1 = Carry

| title = Density of asteroids

| journal = Planetary and Space Science

| volume = 73

| issue = 1

| pages = 98–118

|date=December 2012

| doi = 10.1016/j.pss.2012.03.009

| bibcode = 2012P&SS...73...98C

| postscript= .

|arxiv = 1203.4336 }} See Table 1.

{{Citation

| last1 = Pilcher

| first1 = Frederick

| title = Rotation Period Determinations for 31 Euphrosyne, 65 Cybele, 154 Bertha 177 Irma, 200 Dynamene, 724 Hapag, 880 Herba, and 1470 Carla

| journal = The Minor Planet Bulletin

| volume = 39

| issue = 2

| pages = 57–60

|date=April 2012

| bibcode = 2012MPBu...39...57P

| postscript= .}}

{{cite web

|publisher=IOTA (International Occultation Timing Association)

|title=2006 Asteroid Occultation Reports for North America

|url=http://www.asteroidoccultation.com/observations/Results/index2006.html

|accessdate=2015-06-08

|archive-url=https://web.archive.org/web/20120428111824/http://www.asteroidoccultation.com/observations/Results/index2006.html

|archive-date=2012-04-28

|url-status=dead

}} [http://www.asteroidoccultation.com/observations/Results/Data2006/20061009OCCULTDynameneProfile.jpg (chords)] {{Webarchive|url=https://web.archive.org/web/20150910101607/http://www.asteroidoccultation.com/observations/Results/Data2006/20061009OCCULTDynameneProfile.jpg |date=10 September 2015 }}

}}