“3099 Hergenrother”的意思、由来-开放百科全书

In January 2008, a rotational lightcurve of Hergenrother was obtained from photometric observations by French amateur astronomer Pierre Antonini. Lightcurve analysis gave a rotation period of 24.266 hours with a brightness variation of 0.28 magnitude ({{small|U=2}}).^[8]

Diameter and albedo

According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Hergenrother measures 14.73 kilometers in diameter and its surface has an albedo of 0.224,^[5]^[6] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and consequently calculates a diameter of 29.21 kilometers, as the lower the albedo, the larger the body's diameter at a certain absolute magnitude.^[3]

Naming

This minor planet was named in honor of American astronomer Carl W. Hergenrother (born 1973). At Lunar and Planetary Laboratory, he has been a discoverer of minor planets with high inclinations during the Bigelow Sky Survey, precursor to the Catalina Sky Survey. The naming was proposed by MPC director Brian G. Marsden among others.^[2] The official naming citation was published by the Minor Planet Center on 3 May 1996 ({{small|M.P.C. 27124}}).^[25]

References

1. ^¹²³{{cite book |title = Dictionary of Minor Planet Names – (3099) Hergenrother |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |page = 255 |date = 2007 |isbn = 978-3-540-00238-3 |doi = 10.1007/978-3-540-29925-7_3100 |chapter = (3099) Hergenrother }}
2. ^¹²{{cite web |title = 3099 Hergenrother (1940 GF) |work = Minor Planet Center |url = http://www.minorplanetcenter.net/db_search/show_object?object_id=3099 |accessdate = 8 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 = 8 March 2017}}
4. ^¹²{{cite web |title = Asteroids and comets rotation curves – (3099) Hergenrother |last = Behrend |first = Raoul |publisher = Geneva Observatory |url = http://obswww.unige.ch/~behrend/page4cou.html#003099 |accessdate = 8 March 2017}}
5. ^¹²³{{cite journal |display-authors = 6 |first1 = Joseph R. |last1 = Masiero |first2 = A. K. |last2 = Mainzer |first3 = T. |last3 = Grav |first4 = J. M. |last4 = Bauer |first5 = R. M. |last5 = Cutri |first6 = J. |last6 = Dailey |first7 = P. R. M. |last7 = Eisenhardt |first8 = R. S. |last8 = McMillan |first9 = T. B. |last9 = Spahr |first10 = M. F. |last10 = Skrutskie |first11 = D. |last11 = Tholen |first12 = R. G. |last12 = Walker |first13 = E. L. |last13 = Wright |first14 = E. |last14 = DeBaun |first15 = D. |last15 = Elsbury |first16 = T., IV |last16 = Gautier |first17 = S. |last17 = Gomillion |first18 = A. |last18 = Wilkins |date = November 2011 |title = Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 20 |bibcode = 2011ApJ...741...68M |doi = 10.1088/0004-637X/741/2/68 |arxiv = 1109.4096 |access-date= 8 March 2017}}
6. ^¹²³⁴⁵⁶{{cite web |title = LCDB Data for (3099) Hergenrother |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=3099%7CHergenrother |accessdate = 8 March 2017}}
7. ^¹²³⁴{{cite journal |display-authors = 6 |first1 = A. |last1 = Mainzer |first2 = T. |last2 = Grav |first3 = J. |last3 = Masiero |first4 = E. |last4 = Hand |first5 = J. |last5 = Bauer |first6 = D. |last6 = Tholen |first7 = R. S. |last7 = McMillan |first8 = T. |last8 = Spahr |first9 = R. M. |last9 = Cutri |first10 = E. |last10 = Wright |first11 = J. |last11 = Watkins |first12 = W. |last12 = Mo |first13 = C. |last13 = Maleszewski |date = November 2011 |title = NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 25 |bibcode = 2011ApJ...741...90M |doi = 10.1088/0004-637X/741/2/90 |arxiv = 1109.6407 }}

词条	3099 Hergenrother
释义	Orbit and classification Physical characteristics Rotation period Diameter and albedo Naming References External links {{Infobox planet \| minorplanet = yes \| name = 3099 Hergenrother \| background = #D6D6D6 \| image = \| image_size = \| caption = \| discovery_ref = \| discovered = 3 April 1940 \| discoverer = Y. Väisälä \| discovery_site = Turku Obs. \| mpc_name = (3099) Hergenrother \| alt_names = 1940 GF{{·}}{{mp\|1969 EF\|1}} 1972 VV{{·}}1979 KE 1980 NT{{·}}1984 HB 1984 JG \| pronounced = \| named_after = Carl Hergenrother {{small\|(American astronomer)}}^[2] \| mp_category = main-belt{{·}}{{small\|(outer)}} ^[3] \| orbit_ref = \| epoch = 4 September 2017 (JD 2458000.5) \| uncertainty = 0 \| observation_arc = 76.96 yr (28,111 days) \| aphelion = 3.4563 AU \| perihelion = 2.3048 AU \| semimajor = 2.8805 AU \| eccentricity = 0.1999 \| period = 4.89 yr (1,786 days) \| mean_anomaly = 309.42° \| mean_motion = {{Deg2DMS\|0.2016\|sup=ms}} / day \| inclination = 15.496° \| asc_node = 31.100° \| arg_peri = 148.52° \| dimensions = {{val\|14.732\|0.110}} km^[5]^[6] 29.21 km {{small\|(calculated)}}^[3] \| rotation = {{val\|24.266\|0.007}} h^[8] \| albedo = 0.057 {{small\|(assumed)}}^[3] {{val\|0.224\|0.016}}^[5]^[6] \| spectral_type = C ^[3] \| abs_magnitude = 11.4^[3]^[5] }}3099 Hergenrother, provisional designation {{mp\|1940 GF}}, is an asteroid from the outer region of the asteroid belt, approximately 15 kilometers in diameter. It was discovered on 3 April 1940, by Finnish astronomer Yrjö Väisälä at Turku Observatory in Southwest Finland,^[16] and named after American astronomer Carl Hergenrother in 1996.^[2] Orbit and classification Hergenrother orbits the Sun in the outer main-belt at a distance of 2.3–3.5 AU once every 4 years and 11 months (1,786 days). Its orbit has an eccentricity of 0.20 and an inclination of 15° with respect to the ecliptic. The body's observation arc begins 6 days after its official discovery observation at Turku.^[16] Physical characteristics Rotation period In January 2008, a rotational lightcurve of Hergenrother was obtained from photometric observations by French amateur astronomer Pierre Antonini. Lightcurve analysis gave a rotation period of 24.266 hours with a brightness variation of 0.28 magnitude ({{small\|U=2}}).^[8] Diameter and albedo According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Hergenrother measures 14.73 kilometers in diameter and its surface has an albedo of 0.224,^[5]^[6] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and consequently calculates a diameter of 29.21 kilometers, as the lower the albedo, the larger the body's diameter at a certain absolute magnitude.^[3] Naming This minor planet was named in honor of American astronomer Carl W. Hergenrother (born 1973). At Lunar and Planetary Laboratory, he has been a discoverer of minor planets with high inclinations during the Bigelow Sky Survey, precursor to the Catalina Sky Survey. The naming was proposed by MPC director Brian G. Marsden among others.^[2] The official naming citation was published by the Minor Planet Center on 3 May 1996 ({{small\|M.P.C. 27124}}).^[25] References 1. ^¹²³{{cite book \|title = Dictionary of Minor Planet Names – (3099) Hergenrother \|last = Schmadel \| first = Lutz D. \|publisher = Springer Berlin Heidelberg \|page = 255 \|date = 2007 \|isbn = 978-3-540-00238-3 \|doi = 10.1007/978-3-540-29925-7_3100 \|chapter = (3099) Hergenrother }} 2. ^¹²{{cite web \|title = 3099 Hergenrother (1940 GF) \|work = Minor Planet Center \|url = http://www.minorplanetcenter.net/db_search/show_object?object_id=3099 \|accessdate = 8 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 = 8 March 2017}} 4. ^¹²{{cite web \|title = Asteroids and comets rotation curves – (3099) Hergenrother \|last = Behrend \|first = Raoul \|publisher = Geneva Observatory \|url = http://obswww.unige.ch/~behrend/page4cou.html#003099 \|accessdate = 8 March 2017}} 5. ^¹²³{{cite journal \|display-authors = 6 \|first1 = Joseph R. \|last1 = Masiero \|first2 = A. K. \|last2 = Mainzer \|first3 = T. \|last3 = Grav \|first4 = J. M. \|last4 = Bauer \|first5 = R. M. \|last5 = Cutri \|first6 = J. \|last6 = Dailey \|first7 = P. R. M. \|last7 = Eisenhardt \|first8 = R. S. \|last8 = McMillan \|first9 = T. B. \|last9 = Spahr \|first10 = M. F. \|last10 = Skrutskie \|first11 = D. \|last11 = Tholen \|first12 = R. G. \|last12 = Walker \|first13 = E. L. \|last13 = Wright \|first14 = E. \|last14 = DeBaun \|first15 = D. \|last15 = Elsbury \|first16 = T., IV \|last16 = Gautier \|first17 = S. \|last17 = Gomillion \|first18 = A. \|last18 = Wilkins \|date = November 2011 \|title = Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters \|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M \|journal = The Astrophysical Journal \|volume = 741 \|issue = 2 \|page = 20 \|bibcode = 2011ApJ...741...68M \|doi = 10.1088/0004-637X/741/2/68 \|arxiv = 1109.4096 \|access-date= 8 March 2017}} 6. ^¹²³⁴⁵⁶{{cite web \|title = LCDB Data for (3099) Hergenrother \|publisher = Asteroid Lightcurve Database (LCDB) \|url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=3099%7CHergenrother \|accessdate = 8 March 2017}} 7. ^¹²³⁴{{cite journal \|display-authors = 6 \|first1 = A. \|last1 = Mainzer \|first2 = T. \|last2 = Grav \|first3 = J. \|last3 = Masiero \|first4 = E. \|last4 = Hand \|first5 = J. \|last5 = Bauer \|first6 = D. \|last6 = Tholen \|first7 = R. S. \|last7 = McMillan \|first8 = T. \|last8 = Spahr \|first9 = R. M. \|last9 = Cutri \|first10 = E. \|last10 = Wright \|first11 = J. \|last11 = Watkins \|first12 = W. \|last12 = Mo \|first13 = C. \|last13 = Maleszewski \|date = November 2011 \|title = NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results \|journal = The Astrophysical Journal \|volume = 741 \|issue = 2 \|page = 25 \|bibcode = 2011ApJ...741...90M \|doi = 10.1088/0004-637X/741/2/90 \|arxiv = 1109.6407 }} ^[1]^[2]^[3]^[4]^[5]^[6]^[7] }} External links [https://www.lpl.arizona.edu/news/2015/fall/get-know-staff-scientist-carl-hergenrother Get to Know a Staff Scientist: Carl Hergenrother], Lunar & Planetary Laboratory, University of Arizona 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 (1)-(5000) – Minor Planet Center {{AstDys\|3099}} {{JPL small body}} {{Minor planets navigator\|3098 van Sprang \|number=3099 \|3100 Zimmerman}}{{Small Solar System bodies}}{{DEFAULTSORT:Hergenrother}} 5 : Background asteroids\|Discoveries by Yrjö Väisälä\|Minor planets named for people\|Named minor planets\|Astronomical objects discovered in 1940
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Orbit and classification

Physical characteristics

Rotation period

Diameter and albedo

Naming

References

External links