133 Cyrene

{{Short description|Main-belt asteroid}}

{{Use dmy dates|date=July 2020}}

{{Infobox planet

| minorplanet=yes

| background=#D6D6D6

| name=133 Cyrene

| discoverer=James Craig Watson

| discovered=16 August 1873

| mpc_name=(133) Cyrene

| alt_names=A873 QA; 1910 NB;
1936 HO; 1948 QC;
1959 UR

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

| adjective=Cyrenean {{IPAc-en|s|aɪ|r|ᵻ|'|n|iː|ə|n}}, Cyrenian {{IPAc-en|s|aɪ|'|r|iː|n|i|ə|n}}{{OED|Cyrenean}}

| mp_category=Main belt

| epoch=31 July 2016 (JD 2457600.5)

| orbit_ref=

| semimajor={{Convert|3.06490|AU|Gm|abbr=on}}

| perihelion={{Convert|2.64706|AU|Gm|abbr=on}}

| aphelion={{Convert|3.48274|AU|Gm|abbr=on|lk=on}}

| eccentricity=0.13633

| period=5.37 yr (1959.9 d)

| inclination=7.21561°

| asc_node=319.066°

| arg_peri=289.646°

| mean_anomaly=316.166°

| avg_speed=17.03 km/s

| dimensions={{val|66.57|6.0|ul=km}}

| mass=3.1 × 1017 kg

| density=2.0? g/cm3

| surface_grav=0.0186 m/s²

| escape_velocity=0.0352 km/s

| rotation={{Convert|12.708|h|d|abbr=on|lk=on}}
12.707 h (0.5295 d)

| spectral_type=S

| abs_magnitude=7.98, 7.990

| albedo={{val|0.2563|0.053}}
0.2563

| single_temperature=~133 K

| mean_motion={{Deg2DMS|0.183687|sup=ms}} / day

| observation_arc=142.65 yr (52104 d)

| uncertainty=0

| moid={{Convert|1.64415|AU|Gm|abbr=on}}

| jupiter_moid={{Convert|1.65199|AU|Gm|abbr=on}}

| tisserand=3.206

|image= Орбита астероида 133.png

|caption=Orbital diagram

|named_after= Cyrene (nymph)

}}

133 Cyrene is a fairly large and very bright main-belt asteroid that was discovered by J. C. Watson on 16 August 1873 in Ann Arbor, Michigan, and named after Cyrene, a nymph, daughter of king Hypseus and beloved of Apollo in Greek mythology. It is classified as an S-type asteroid based upon its spectrum. It is listed as a member of the Hecuba group of asteroids that orbit near the 2:1 mean-motion resonance with Jupiter.

In the Tholen classification system, it is categorized as a stony SR-type asteroid. Photometric observations of this asteroid at the Altimira Observatory in 1985 gave a light curve with a period of 12.707 ± 0.015 hours and a brightness variation of 0.22 in magnitude. This result matches previous measurements reported in 1984 and 2005.

References

{{Reflist|refs=

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| publisher = NASA Jet Propulsion Laboratory

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{{Citation

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}}

{{Citation

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| work = Astronomical Journal

| volume = 53

| page = 199

|date=June 1948

| bibcode = 1948AJ.....53..199M

| postscript= .

|doi = 10.1086/106097 | url= http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1948AJ.....53..199M&link_type=ARTICLE&db_key=AST&high=

}}

{{Citation

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|last4=Bus

|first4=Schelte J.

|display-authors=1

|title=An extension of the Bus asteroid taxonomy into the near-infrared

|work=Icarus

|volume=202

|issue=1

|pages=160–180

|date=July 2009

|doi=10.1016/j.icarus.2009.02.005

|bibcode=2009Icar..202..160D

|url=http://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016%252Fj.icarus.2009.02.005.pdf

|accessdate=2013-04-08

|postscript=.

|url-status=dead

|archiveurl=https://web.archive.org/web/20140317200310/https://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016/j.icarus.2009.02.005.pdf

|archivedate=2014-03-17

}} See appendix A.

}}