“5026 Martes”的意思、由来-开放百科全书

A first precovery was taken at Palomar Observatory in 1953, extending the body's observation arc by 34 years prior to its official discovery observation at Klet.^[21]

Physical characteristics

Asteroid pair

Lightcurves

Between 2008 and 2010, several rotational lightcurves of Martes were obtained from photometric observations. Lightcurve analysis gave a well-defined rotation period of 4.4243 hours with a brightness amplitude of 0.69 magnitude ({{small|U=3-/3/2+/3/2}}).^[3]^[9]^[8]^[7]

Diameter and albedo

According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Martes measures 8.967 kilometers in diameter and its surface has an albedo of 0.066, which is typical for carbonaceous asteroids.^[6] The Collaborative Asteroid Lightcurve Link, however, assumes a standard albedo for stony asteroids of 0.20 and consequently calculates a much smaller diameter of 4.93 kilometers, due to the higher albedo.^[3]

Naming

This minor planet was named for the two species of the family Mustelidae, the pine marten and beech marten. They also live in the forests near the discovering Kleť Observatory.^[2] The official naming citation was published by the Minor Planet Center on 22 June 1999 ({{small|M.P.C. 34920}}).^[34]

References

1. ^¹²³{{cite book |title = Dictionary of Minor Planet Names – (5026) Martes |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |page = 432 |date = 2007 |isbn = 978-3-540-00238-3 |doi = 10.1007/978-3-540-29925-7_4893 |chapter = (5026) Martes }}
2. ^¹²{{cite web |title = 5026 Martes (1987 QL1) |work = Minor Planet Center |url = http://www.minorplanetcenter.net/db_search/show_object?object_id=5026 |accessdate = 28 March 2017}}
3. ^¹{{cite web |title = MPC/MPO/MPS Archive |work = Minor Planet Center |url = http://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html |accessdate = 28 March 2017}}
4. ^¹²³⁴⁵⁶⁷{{cite web |title = LCDB Data for (5026) Martes |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=5026%7CMartes |accessdate = 28 March 2017}}
5. ^¹²³⁴{{cite journal |display-authors = 6 |first1 = C. R. |last1 = Nugent |first2 = A. |last2 = Mainzer |first3 = J. |last3 = Masiero |first4 = J. |last4 = Bauer |first5 = R. M. |last5 = Cutri |first6 = T. |last6 = Grav |first7 = E. |last7 = Kramer |first8 = S. |last8 = Sonnett |first9 = R. |last9 = Stevenson |first10 = E. L. |last10 = Wright |date = December 2015 |title = NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJ...814..117N |journal = The Astrophysical Journal |volume = 814 |issue = 2 |page = 13 |bibcode = 2015ApJ...814..117N |doi = 10.1088/0004-637X/814/2/117 |arxiv = 1509.02522 |access-date= 28 March 2017}}
6. ^¹²³{{cite journal |display-authors = 6 |first1 = P. |last1 = Pravec |first2 = D. |last2 = Vokrouhlický |first3 = D. |last3 = Polishook |first4 = D. J. |last4 = Scheeres |first5 = A. W. |last5 = Harris |first6 = A. |last6 = Galád |first7 = O. |last7 = Vaduvescu |first8 = F. |last8 = Pozo |first9 = A. |last9 = Barr |first10 = P. |last10 = Longa |first11 = F. |last11 = Vachier |first12 = F. |last12 = Colas |first13 = D. P. |last13 = Pray |first14 = J. |last14 = Pollock |first15 = D. |last15 = Reichart |first16 = K. |last16 = Ivarsen |first17 = J. |last17 = Haislip |first18 = A. |last18 = Lacluyze |first19 = P. |last19 = Kusnirák |first20 = T. |last20 = Henych |first21 = F. |last21 = Marchis |first22 = B. |last22 = Macomber |first23 = S. A. |last23 = Jacobson |first24 = Yu. N. |last24 = Krugly |first25 = A. V. |last25 = Sergeev |first26 = A. |last26 = Leroy |date = August 2010 |title = Formation of asteroid pairs by rotational fission |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2010Natur.466.1085P |journal = Nature |volume = 466 |issue = 7310 |pages = 1085–1088 |bibcode = 2010Natur.466.1085P |doi = 10.1038/nature09315 |pmid = 20740010 |arxiv = 1009.2770 |access-date= 28 March 2017}}
7. ^¹²{{Cite journal |author = Polishook, D. |date = October 2014 |title = Spin axes and shape models of asteroid pairs: Fingerprints of YORP and a path to the density of rubble piles |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014Icar..241...79P |journal = Icarus |volume = 241 |pages = 79–96 |bibcode = 2014Icar..241...79P |doi = 10.1016/j.icarus.2014.06.018 |access-date= 28 March 2017|arxiv = 1406.3359 }}
8. ^¹²³{{cite journal |display-authors = 6 |first1 = Adam |last1 = Waszczak |first2 = Chan-Kao |last2 = Chang |first3 = Eran O. |last3 = Ofek |first4 = Russ |last4 = Laher |first5 = Frank |last5 = Masci |first6 = David |last6 = Levitan |first7 = Jason |last7 = Surace |first8 = Yu-Chi |last8 = Cheng |first9 = Wing-Huen |last9 = Ip |first10 = Daisuke |last10 = Kinoshita |first11 = George |last11 = Helou |first12 = Thomas A. |last12 = Prince |first13 = Shrinivas |last13 = Kulkarni |date = September 2015 |title = Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015AJ....150...75W |journal = The Astronomical Journal |volume = 150 |issue = 3 |page = 35 |bibcode = 2015AJ....150...75W |doi = 10.1088/0004-6256/150/3/75 |arxiv = 1504.04041 |access-date= 28 March 2017}}
9. ^¹²³{{cite journal |display-authors = 6 |first1 = Peter |last1 = Veres |first2 = Robert |last2 = Jedicke |first3 = Alan |last3 = Fitzsimmons |first4 = Larry |last4 = Denneau |first5 = Mikael |last5 = Granvik |first6 = Bryce |last6 = Bolin |first7 = Serge |last7 = Chastel |first8 = Richard J. |last8 = Wainscoat |first9 = William S. |last9 = Burgett |first10 = Kenneth C. |last10 = Chambers |first11 = Heather |last11 = Flewelling |first12 = Nick |last12 = Kaiser |first13 = Eugen A. |last13 = Magnier |first14 = Jeff S. |last14 = Morgan |first15 = Paul A. |last15 = Price |first16 = John L. |last16 = Tonry |first17 = Christopher |last17 = Waters |date = November 2015 |title = Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V |journal = Icarus |volume = 261 |pages = 34–47 |bibcode = 2015Icar..261...34V |doi = 10.1016/j.icarus.2015.08.007 |arxiv = 1506.00762 |access-date= 28 March 2017}}
10. ^¹²{{Cite journal |author = Ye, Q.-z. |date = February 2011 |title = BVRI Photometry of 53 Unusual Asteroids |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011AJ....141...32Y |journal = The Astronomical Journal |volume = 141 |issue = 2 |page = 8 |bibcode = 2011AJ....141...32Y |doi = 10.1088/0004-6256/141/2/32 |arxiv = 1011.0133 |access-date= 29 March 2017}}

词条	5026 Martes
释义	Orbit and classification Physical characteristics Asteroid pair Lightcurves Diameter and albedo Naming References External links {{Infobox planet \| minorplanet = yes \| name = 5026 Martes \| background = #D6D6D6 \| image = \| image_size = \| caption = \| discovery_ref = \| discovered = 22 August 1987 \| discoverer = A. Mrkos \| discovery_site = Kleť Obs. \| mpc_name = (5026) Martes \| alt_names = {{mp\|1987 QL\|1}}{{·}}1965 QE 1976 QL{{·}}{{mp\|1980 VA\|2}} \| pronounced = \| named_after = pine marten beech marten {{small\|(Mustelidae mammals)}}^[2] \| mp_category = main-belt{{·}}{{small\|(inner)}} ^[3] \| orbit_ref = \| epoch = 4 September 2017 (JD 2458000.5) \| uncertainty = 0 \| observation_arc = 63.37 yr (23,145 days) \| aphelion = 2.9540 AU \| perihelion = 1.8020 AU \| semimajor = 2.3780 AU \| eccentricity = 0.2422 \| period = 3.67 yr (1,339 days) \| mean_anomaly = 75.131° \| mean_motion = {{Deg2DMS\|0.2688\|sup=ms}} / day \| inclination = 4.2831° \| asc_node = 304.77° \| arg_peri = 17.652° \| dimensions = 4.93 km {{small\|(calculated)}}^[3] {{val\|8.967\|2.335}} km^[6] \| rotation = {{val\|4.423\|0.0011}} h^[7] {{val\|4.424087\|0.000002}} h^[8] {{val\|4.4243\|0.005}} h^[9] \| albedo = {{val\|0.066\|0.072}}^[6] 0.20 {{small\|(assumed)}}^[3] \| spectral_type = B–V = {{val\|0.863\|0.042}}^[12] V–R = {{val\|0.440\|0.047}}^[12] C ^[14]{{·}}S ^[3] \| abs_magnitude = 13.80^[6]{{·}}13.9^[3]{{·}}{{val\|14.065\|0.010}} {{small\|(R)}}^[7]{{·}}{{val\|14.17\|0.36}}^[14] }}5026 Martes, provisional designation {{mp\|1987 QL\|1}}, is a carbonaceous asteroid from the inner region of the asteroid belt, approximately 9 kilometers in diameter. It was discovered on 22 August 1987, by Czech astronomer Antonín Mrkos at Kleť Observatory in the Czech Republic.^[21] It is named after the two weasel-like animal species: pine marten and beech marten.^[2] Orbit and classification Martes is the namesake member of a small asteroid family, named the Martes family.{{citation needed\|date=March 2017}} It orbits the Sun in the inner main-belt at a distance of 1.8–3.0 AU once every 3 years and 8 months (1,339 days). Its orbit has an eccentricity of 0.24 and an inclination of 4° with respect to the ecliptic. A first precovery was taken at Palomar Observatory in 1953, extending the body's observation arc by 34 years prior to its official discovery observation at Klet.^[21] Physical characteristics Martes has been characterized as a carbonaceous C-type asteroid by PanSTARRS{{'}} photometric survey.^[14] Asteroid pair Martes forms an asteroid pair with {{mp\|2005 WW\|113}}, and was part of the 35 sample asteroid pairs in Petr Pravec's study Formation of asteroid pairs by rotational fission, published in the journal Nature.^[9] Lightcurves Between 2008 and 2010, several rotational lightcurves of Martes were obtained from photometric observations. Lightcurve analysis gave a well-defined rotation period of 4.4243 hours with a brightness amplitude of 0.69 magnitude ({{small\|U=3-/3/2+/3/2}}).^[3]^[9]^[8]^[7] Diameter and albedo According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Martes measures 8.967 kilometers in diameter and its surface has an albedo of 0.066, which is typical for carbonaceous asteroids.^[6] The Collaborative Asteroid Lightcurve Link, however, assumes a standard albedo for stony asteroids of 0.20 and consequently calculates a much smaller diameter of 4.93 kilometers, due to the higher albedo.^[3] Naming This minor planet was named for the two species of the family Mustelidae, the pine marten and beech marten. They also live in the forests near the discovering Kleť Observatory.^[2] The official naming citation was published by the Minor Planet Center on 22 June 1999 ({{small\|M.P.C. 34920}}).^[34] References 1. ^¹²³{{cite book \|title = Dictionary of Minor Planet Names – (5026) Martes \|last = Schmadel \| first = Lutz D. \|publisher = Springer Berlin Heidelberg \|page = 432 \|date = 2007 \|isbn = 978-3-540-00238-3 \|doi = 10.1007/978-3-540-29925-7_4893 \|chapter = (5026) Martes }} 2. ^¹²{{cite web \|title = 5026 Martes (1987 QL1) \|work = Minor Planet Center \|url = http://www.minorplanetcenter.net/db_search/show_object?object_id=5026 \|accessdate = 28 March 2017}} 3. ^¹{{cite web \|title = MPC/MPO/MPS Archive \|work = Minor Planet Center \|url = http://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html \|accessdate = 28 March 2017}} 4. ^¹²³⁴⁵⁶⁷{{cite web \|title = LCDB Data for (5026) Martes \|publisher = Asteroid Lightcurve Database (LCDB) \|url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=5026%7CMartes \|accessdate = 28 March 2017}} 5. ^¹²³⁴{{cite journal \|display-authors = 6 \|first1 = C. R. \|last1 = Nugent \|first2 = A. \|last2 = Mainzer \|first3 = J. \|last3 = Masiero \|first4 = J. \|last4 = Bauer \|first5 = R. M. \|last5 = Cutri \|first6 = T. \|last6 = Grav \|first7 = E. \|last7 = Kramer \|first8 = S. \|last8 = Sonnett \|first9 = R. \|last9 = Stevenson \|first10 = E. L. \|last10 = Wright \|date = December 2015 \|title = NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos \|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJ...814..117N \|journal = The Astrophysical Journal \|volume = 814 \|issue = 2 \|page = 13 \|bibcode = 2015ApJ...814..117N \|doi = 10.1088/0004-637X/814/2/117 \|arxiv = 1509.02522 \|access-date= 28 March 2017}} 6. ^¹²³{{cite journal \|display-authors = 6 \|first1 = P. \|last1 = Pravec \|first2 = D. \|last2 = Vokrouhlický \|first3 = D. \|last3 = Polishook \|first4 = D. J. \|last4 = Scheeres \|first5 = A. W. \|last5 = Harris \|first6 = A. \|last6 = Galád \|first7 = O. \|last7 = Vaduvescu \|first8 = F. \|last8 = Pozo \|first9 = A. \|last9 = Barr \|first10 = P. \|last10 = Longa \|first11 = F. \|last11 = Vachier \|first12 = F. \|last12 = Colas \|first13 = D. P. \|last13 = Pray \|first14 = J. \|last14 = Pollock \|first15 = D. \|last15 = Reichart \|first16 = K. \|last16 = Ivarsen \|first17 = J. \|last17 = Haislip \|first18 = A. \|last18 = Lacluyze \|first19 = P. \|last19 = Kusnirák \|first20 = T. \|last20 = Henych \|first21 = F. \|last21 = Marchis \|first22 = B. \|last22 = Macomber \|first23 = S. A. \|last23 = Jacobson \|first24 = Yu. N. \|last24 = Krugly \|first25 = A. V. \|last25 = Sergeev \|first26 = A. \|last26 = Leroy \|date = August 2010 \|title = Formation of asteroid pairs by rotational fission \|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2010Natur.466.1085P \|journal = Nature \|volume = 466 \|issue = 7310 \|pages = 1085–1088 \|bibcode = 2010Natur.466.1085P \|doi = 10.1038/nature09315 \|pmid = 20740010 \|arxiv = 1009.2770 \|access-date= 28 March 2017}} 7. ^¹²{{Cite journal \|author = Polishook, D. \|date = October 2014 \|title = Spin axes and shape models of asteroid pairs: Fingerprints of YORP and a path to the density of rubble piles \|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014Icar..241...79P \|journal = Icarus \|volume = 241 \|pages = 79–96 \|bibcode = 2014Icar..241...79P \|doi = 10.1016/j.icarus.2014.06.018 \|access-date= 28 March 2017\|arxiv = 1406.3359 }} 8. ^¹²³{{cite journal \|display-authors = 6 \|first1 = Adam \|last1 = Waszczak \|first2 = Chan-Kao \|last2 = Chang \|first3 = Eran O. \|last3 = Ofek \|first4 = Russ \|last4 = Laher \|first5 = Frank \|last5 = Masci \|first6 = David \|last6 = Levitan \|first7 = Jason \|last7 = Surace \|first8 = Yu-Chi \|last8 = Cheng \|first9 = Wing-Huen \|last9 = Ip \|first10 = Daisuke \|last10 = Kinoshita \|first11 = George \|last11 = Helou \|first12 = Thomas A. \|last12 = Prince \|first13 = Shrinivas \|last13 = Kulkarni \|date = September 2015 \|title = Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry \|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015AJ....150...75W \|journal = The Astronomical Journal \|volume = 150 \|issue = 3 \|page = 35 \|bibcode = 2015AJ....150...75W \|doi = 10.1088/0004-6256/150/3/75 \|arxiv = 1504.04041 \|access-date= 28 March 2017}} 9. ^¹²³{{cite journal \|display-authors = 6 \|first1 = Peter \|last1 = Veres \|first2 = Robert \|last2 = Jedicke \|first3 = Alan \|last3 = Fitzsimmons \|first4 = Larry \|last4 = Denneau \|first5 = Mikael \|last5 = Granvik \|first6 = Bryce \|last6 = Bolin \|first7 = Serge \|last7 = Chastel \|first8 = Richard J. \|last8 = Wainscoat \|first9 = William S. \|last9 = Burgett \|first10 = Kenneth C. \|last10 = Chambers \|first11 = Heather \|last11 = Flewelling \|first12 = Nick \|last12 = Kaiser \|first13 = Eugen A. \|last13 = Magnier \|first14 = Jeff S. \|last14 = Morgan \|first15 = Paul A. \|last15 = Price \|first16 = John L. \|last16 = Tonry \|first17 = Christopher \|last17 = Waters \|date = November 2015 \|title = Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results \|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V \|journal = Icarus \|volume = 261 \|pages = 34–47 \|bibcode = 2015Icar..261...34V \|doi = 10.1016/j.icarus.2015.08.007 \|arxiv = 1506.00762 \|access-date= 28 March 2017}} 10. ^¹²{{Cite journal \|author = Ye, Q.-z. \|date = February 2011 \|title = BVRI Photometry of 53 Unusual Asteroids \|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011AJ....141...32Y \|journal = The Astronomical Journal \|volume = 141 \|issue = 2 \|page = 8 \|bibcode = 2011AJ....141...32Y \|doi = 10.1088/0004-6256/141/2/32 \|arxiv = 1011.0133 \|access-date= 29 March 2017}} ^[1]^[2]^[3]^[4]^[5]^[6]^[7]^[8]^[9]^[10] }} External links Asteroid Lightcurve Database (LCDB), query form (info) [https://books.google.com/books?id=aeAg1X7afOoC&pg Dictionary of Minor Planet Names], Google books Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend Discovery Circumstances: Numbered Minor Planets (5001)-(10000) – Minor Planet Center {{AstDys\|5026}} {{JPL small body}} {{Use dmy dates\|date=July 2018}}{{Minor planets navigator \|(5025) 1986 TS6 \|number=5026 \|5027 Androgeos}}{{Small Solar System bodies}}{{DEFAULTSORT:Martes}} 6 : Erigone asteroids\|Martes asteroids\|Discoveries by Antonín Mrkos\|Minor planets named for animals\|Named minor planets\|Astronomical objects discovered in 1987
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