“10244 Thüringer Wald”的意思、由来-开放百科全书

The asteroid's spectral type is unknown. Vestian asteroids typically have a V- or S-type,^[12] with albedos higher than measured by the WISE telescope (see below). It has an absolute magnitude of 14.6. As of 2018, no rotational lightcurve of Thüringer Wald has been obtained from photometric observations. The body's rotation period, pole and shape remain unknown.

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Thüringer Wald measures 3.346 kilometers in diameter and its surface has an albedo of 0.190.^[7]

Palomar–Leiden survey

The survey designation "P-L" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with the discovery of several thousand asteroid discoveries.^[20]

Naming

This minor planet was named after the Thuringian Forest ({{lang-de|Thüringer Wald}}), a mountain range in central Germany.^[1] The official naming citation was published by the Minor Planet Center on 1 May 2003 ({{small|M.P.C. 48390}}).^[22]

References

1. ^¹²³⁴⁵⁶{{cite web |title = 10244 Thuringer Wald (4668 P-L) |work = Minor Planet Center |url = https://www.minorplanetcenter.net/db_search/show_object?object_id=10244 |accessdate = 30 April 2018}}
2. ^¹{{cite web |title = MPC/MPO/MPS Archive |work = Minor Planet Center |url = https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html |accessdate = 30 April 2018}}
3. ^¹²{{cite web |title = Small Bodies Data Ferret |work = Nesvorny HCM Asteroid Families V3.0 |url = https://sbntools.psi.edu/ferret/PropertySearch/familyForm.action |accessdate = 30 April 2018}}
4. ^¹²{{Cite journal |first1 = D. |last1 = Nesvorný |first2 = M. |last2 = Broz |first3 = V. |last3 = Carruba |date = December 2014 |title = Identification and Dynamical Properties of Asteroid Families |url = https://arxiv.org/pdf/1502.01628.pdf |journal = Asteroids IV |pages = 297–321 |bibcode = 2015aste.book..297N |doi = 10.2458/azu_uapress_9780816532131-ch016 |arxiv = 1502.01628 |access-date= 30 April 2018}}
5. ^¹{{cite journal |first1 = Michael S. |last1 = Kelley |first2 = Faith |last2 = Vilas |first3 = Michael J. |last3 = Gaffey |first4 = Paul A. |last4 = Abell |date = September 2003 |title = Quantified mineralogical evidence for a common origin of 1929 Kollaa with 4 Vesta and the HED meteorites |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2003Icar..165..215K |journal = Icarus |volume = 165 |issue = 1 |pages = 215–218 |bibcode = 2003Icar..165..215K |doi = 10.1016/S0019-1035(03)00149-0 |accessdate = 30 April 2018}}
6. ^¹{{cite web |title = Minor Planet Discoverers |work = Minor Planet Center |url = http://www.minorplanetcenter.net/iau/lists/MPDiscsNum.html |date = 2018 |accessdate = 30 April 2018}}
7. ^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= 30 April 2018}}

词条	10244 Thüringer Wald
释义	Orbit and classification Physical characteristics Diameter and albedo Palomar–Leiden survey Naming References External links {{Infobox planet \| minorplanet = yes \| name = 10244 Thüringer Wald \| background = #D6D6D6 \| image = \| image_size = \| caption = \| discovery_ref = ^[1] \| discoverer = C. J. van Houten I. van Houten-G. Tom Gehrels \| discovery_site = Palomar Obs. \| discovered = 26 September 1960 \| mpc_name = {{nowrap\|(10244) Thüringer Wald}} \| alt_names = 4668 P-L{{·}}{{mp\|1990 TB\|14}} \| pronounced = \| named_after = Thuringian Forest ^[1] {{small\|(German mountain range)}} \| mp_category = main-belt ^[1]{{·}}{{small\|(inner)}} Vesta ^[5] \| orbit_ref = \| epoch = 23 March 2018 (JD 2458200.5) \| uncertainty = 0 \| observation_arc = 57.42 yr (20,973 d) \| aphelion = 2.6482 AU \| perihelion = 2.1598 AU \| semimajor = 2.4040 AU \| eccentricity = 0.1016 \| period = 3.73 yr (1,361 d) \| mean_anomaly = 109.85° \| mean_motion = {{Deg2DMS\|0.2644\|sup=ms}} / day \| inclination = 7.4739° \| asc_node = 28.159° \| arg_peri = 27.932° \| mean_diameter = {{val\|3.346\|0.207\|ul=km}}^[7] \| rotation = \| albedo = {{val\|0.190\|0.054}}^[7] \| spectral_type = \| abs_magnitude = 14.6 }}10244 Thüringer Wald, provisional designation {{mp\|4668 P-L}}, is a Vestian asteroid from the inner regions of the asteroid belt, approximately {{convert\|3.3\|km\|mi\|abbr=off\|sigfig=2\|sp=us}} in diameter. It was discovered on 26 September 1960, by Ingrid and Cornelis van Houten at Leiden, and Tom Gehrels at Palomar Observatory in California, United States. The asteroid was named after the Thuringian Forest, a German mountain range.^[1] Orbit and classification Thüringer Wald is a member of the Vesta family ({{small\|401}}).^[5] Vestian asteroids have a composition akin to cumulate eucrites (HED meteorites) and are thought to have originated deep within 4 Vesta's crust, possibly from the Rheasilvia crater, a large impact crater on its southern hemisphere near the South pole, formed as a result of a subcatastrophic collision. Vesta is the main belt's second-largest and second-most-massive body after {{Dp\|Ceres}}.^[12]^[13]Thüringer Wald orbits the Sun in the inner main-belt at a distance of 2.2–2.6 AU once every 3 years and 9 months (1,361 days; semi-major axis of 2.4 AU). Its orbit has an eccentricity of 0.10 and an inclination of 7° with respect to the ecliptic. Its observation arc begins with its official discovery observation at Palomar in September 1960.^[1] Physical characteristics The asteroid's spectral type is unknown. Vestian asteroids typically have a V- or S-type,^[12] with albedos higher than measured by the WISE telescope (see below). It has an absolute magnitude of 14.6. As of 2018, no rotational lightcurve of Thüringer Wald has been obtained from photometric observations. The body's rotation period, pole and shape remain unknown. Diameter and albedo According to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Thüringer Wald measures 3.346 kilometers in diameter and its surface has an albedo of 0.190.^[7] Palomar–Leiden survey The survey designation "P-L" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with the discovery of several thousand asteroid discoveries.^[20] Naming This minor planet was named after the Thuringian Forest ({{lang-de\|Thüringer Wald}}), a mountain range in central Germany.^[1] The official naming citation was published by the Minor Planet Center on 1 May 2003 ({{small\|M.P.C. 48390}}).^[22] References 1. ^¹²³⁴⁵⁶{{cite web \|title = 10244 Thuringer Wald (4668 P-L) \|work = Minor Planet Center \|url = https://www.minorplanetcenter.net/db_search/show_object?object_id=10244 \|accessdate = 30 April 2018}} 2. ^¹{{cite web \|title = MPC/MPO/MPS Archive \|work = Minor Planet Center \|url = https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html \|accessdate = 30 April 2018}} 3. ^¹²{{cite web \|title = Small Bodies Data Ferret \|work = Nesvorny HCM Asteroid Families V3.0 \|url = https://sbntools.psi.edu/ferret/PropertySearch/familyForm.action \|accessdate = 30 April 2018}} 4. ^¹²{{Cite journal \|first1 = D. \|last1 = Nesvorný \|first2 = M. \|last2 = Broz \|first3 = V. \|last3 = Carruba \|date = December 2014 \|title = Identification and Dynamical Properties of Asteroid Families \|url = https://arxiv.org/pdf/1502.01628.pdf \|journal = Asteroids IV \|pages = 297–321 \|bibcode = 2015aste.book..297N \|doi = 10.2458/azu_uapress_9780816532131-ch016 \|arxiv = 1502.01628 \|access-date= 30 April 2018}} 5. ^¹{{cite journal \|first1 = Michael S. \|last1 = Kelley \|first2 = Faith \|last2 = Vilas \|first3 = Michael J. \|last3 = Gaffey \|first4 = Paul A. \|last4 = Abell \|date = September 2003 \|title = Quantified mineralogical evidence for a common origin of 1929 Kollaa with 4 Vesta and the HED meteorites \|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2003Icar..165..215K \|journal = Icarus \|volume = 165 \|issue = 1 \|pages = 215–218 \|bibcode = 2003Icar..165..215K \|doi = 10.1016/S0019-1035(03)00149-0 \|accessdate = 30 April 2018}} 6. ^¹{{cite web \|title = Minor Planet Discoverers \|work = Minor Planet Center \|url = http://www.minorplanetcenter.net/iau/lists/MPDiscsNum.html \|date = 2018 \|accessdate = 30 April 2018}} 7. ^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= 30 April 2018}} ^[1]^[2]^[3]^[4]^[5]^[6]^[7] }} External links Asteroid Lightcurve Database (LCDB), query form (info) [https://books.google.com/books?id=aeAg1X7afOoC&pg Dictionary of Minor Planet Names], Google books Discovery Circumstances: Numbered Minor Planets (10001)-(15000) – Minor Planet Center {{AstDys\|10244}} {{JPL small body}} {{Use dmy dates\|date=April 2018}}{{Minor planets navigator \|10243 Hohe Meissner \|number=10244 \|10245 Inselsberg }}{{Small Solar System bodies}}{{DEFAULTSORT:Thuringer Wald}} 8 : Vesta asteroids\|Discoveries by Cornelis Johannes van Houten\|Discoveries by Ingrid van Houten-Groeneveld\|Discoveries by Tom Gehrels\|Discoveries by the Palomar–Leiden survey\|Minor planets named for places\|Named minor planets\|Astronomical objects discovered in 1960
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Orbit and classification

Physical characteristics

Diameter and albedo

Palomar–Leiden survey

Naming

References

External links