“1767 Lampland”的意思、由来-开放百科全书

The asteroid was first identified as {{mp|1941 SP}} at Uccle Observatory in September 1941. The body's observation arc begins with a precovery at Palomar Observatory in August 1951, more than 11 years prior to its official discovery observation at Goethe Link.^[11]

Physical characteristics

In the Tholen classification, its spectral type is ambiguous, closest to the X-type asteroid and with some resemblance to the C-type asteroids, while the overall spectral type of the Eos family is that of a K-type.^[14]{{rp|23}}

Rotation period

As of 2017, no rotational lightcurve of Lampland has been obtained from photometric observations. The asteroid's rotation period, poles and shape remain unknown.^[19]

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Lampland measures 15.448 kilometers in diameter and its surface has an albedo of 0.116.^[5]^[6]

Naming

This minor planet was named after American astronomer Carl Lampland (1873–1951), a graduate of Indiana University, best known for his radiometric measurements of planetary temperatures.^[2]

Lampland is also honored by a lunar and by a a Martian crater. The name was proposed by Frank K. Edmondson, who initiated the Indiana Asteroid Program.^[2] The official naming citation was published by the Minor Planet Center before November 1977 ({{small|M.P.C. 3144}}).^[24]

References

1. ^¹²³⁴{{cite book |title = Dictionary of Minor Planet Names – (1767) Lampland |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |page = 141 |date = 2007 |isbn = 978-3-540-00238-3 |doi = 10.1007/978-3-540-29925-7_1768 |chapter = (1767) Lampland }}
2. ^¹²{{cite web |title = 1767 Lampland (1962 RJ) |work = Minor Planet Center |url = http://www.minorplanetcenter.net/db_search/show_object?object_id=1767 |accessdate = 6 September 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 = 6 September 2017}}
4. ^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 = 6 September 2017}}
5. ^¹²{{Cite book |first1 = D. |last1 = Nesvorný |first2 = M. |last2 = Broz |first3 = V. |last3 = Carruba |date = December 2014 |title = Identification and Dynamical Properties of Asteroid Families |journal = Asteroids IV |pages = 297–321 |bibcode = 2015aste.book..297N |doi = 10.2458/azu_uapress_9780816532131-ch016 |arxiv = 1502.01628 |isbn = 9780816532131 }}
6. ^¹²{{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 = C. |last6 = Nugent |first7 = M. S. |last7 = Cabrera |date = November 2012 |title = Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M |journal = The Astrophysical Journal Letters |volume = 759 |issue = 1 |page = 5 |bibcode = 2012ApJ...759L...8M |doi = 10.1088/2041-8205/759/1/L8 |arxiv = 1209.5794 |access-date= 6 September 2017}}
7. ^¹²{{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= 6 September 2017}}
8. ^¹{{cite web |title = LCDB Data for (1767) Lampland |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=1767%7CLampland |accessdate = 6 September 2017}}

词条	1767 Lampland
释义	Orbit and classification Physical characteristics Rotation period Diameter and albedo Naming References External links {{Infobox planet \| minorplanet = yes \| name = 1767 Lampland \| background = #D6D6D6 \| image = \| image_size = \| caption = \| discovery_ref = \| discoverer = Indiana University {{nowrap\|{{small\|(Indiana Asteroid Program)}}}} \| discovery_site = Goethe Link Obs. \| discovered = 7 September 1962 \| mpc_name = (1767) Lampland \| alt_names = 1962 RJ{{·}}1941 SP 1967 SC \| pronounced = \| named_after = Carl Lampland ^[2] {{small\|(American astronomer)}} \| mp_category = main-belt{{·}}{{small\|(outer)}} Eos ^[3] \| orbit_ref = \| epoch = 4 September 2017 (JD 2458000.5) \| uncertainty = 0 \| observation_arc = 75.52 yr (27,585 days) \| aphelion = 3.3209 AU \| perihelion = 2.7160 AU \| semimajor = 3.0185 AU \| eccentricity = 0.1002 \| period = 5.24 yr (1,915 days) \| mean_anomaly = 201.21° \| mean_motion = {{Deg2DMS\|0.1879\|sup=ms}} / day \| inclination = 9.8418° \| asc_node = 192.22° \| arg_peri = 135.41° \| dimensions = {{val\|15.448\|2.805}} km^[5] \| rotation = \| albedo = {{val\|0.116\|0.057}}^[6] \| spectral_type = Tholen {{=}} XC B–V {{=}} 0.750 U–B {{=}} 0.340 \| abs_magnitude = 12.20 }}1767 Lampland, provisional designation {{mp\|1962 RJ}}, is an Eoan asteroid from the outer regions of the asteroid belt, approximately 15 kilometers in diameter. It was discovered on 7 September 1962, by astronomers of the Indiana Asteroid Program at Goethe Link Observatory in Indiana, United States.^[11] The asteroid was named after American astronomer Carl Lampland.^[2] Orbit and classification Lampland a member the Eos family ({{small\|606}}), the largest asteroid family in the outer main belt consisting of nearly 10,000 asteroids.^[3]^[14]{{rp\|23}} It orbits the Sun at a distance of 2.7–3.3 AU once every 5 years and 3 months (1,915 days). Its orbit has an eccentricity of 0.10 and an inclination of 10° with respect to the ecliptic. The asteroid was first identified as {{mp\|1941 SP}} at Uccle Observatory in September 1941. The body's observation arc begins with a precovery at Palomar Observatory in August 1951, more than 11 years prior to its official discovery observation at Goethe Link.^[11] Physical characteristics In the Tholen classification, its spectral type is ambiguous, closest to the X-type asteroid and with some resemblance to the C-type asteroids, while the overall spectral type of the Eos family is that of a K-type.^[14]{{rp\|23}} Rotation period As of 2017, no rotational lightcurve of Lampland has been obtained from photometric observations. The asteroid's rotation period, poles and shape remain unknown.^[19] Diameter and albedo According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Lampland measures 15.448 kilometers in diameter and its surface has an albedo of 0.116.^[5]^[6] Naming This minor planet was named after American astronomer Carl Lampland (1873–1951), a graduate of Indiana University, best known for his radiometric measurements of planetary temperatures.^[2] Lampland is also honored by a lunar and by a a Martian crater. The name was proposed by Frank K. Edmondson, who initiated the Indiana Asteroid Program.^[2] The official naming citation was published by the Minor Planet Center before November 1977 ({{small\|M.P.C. 3144}}).^[24] References 1. ^¹²³⁴{{cite book \|title = Dictionary of Minor Planet Names – (1767) Lampland \|last = Schmadel \| first = Lutz D. \|publisher = Springer Berlin Heidelberg \|page = 141 \|date = 2007 \|isbn = 978-3-540-00238-3 \|doi = 10.1007/978-3-540-29925-7_1768 \|chapter = (1767) Lampland }} 2. ^¹²{{cite web \|title = 1767 Lampland (1962 RJ) \|work = Minor Planet Center \|url = http://www.minorplanetcenter.net/db_search/show_object?object_id=1767 \|accessdate = 6 September 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 = 6 September 2017}} 4. ^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 = 6 September 2017}} 5. ^¹²{{Cite book \|first1 = D. \|last1 = Nesvorný \|first2 = M. \|last2 = Broz \|first3 = V. \|last3 = Carruba \|date = December 2014 \|title = Identification and Dynamical Properties of Asteroid Families \|journal = Asteroids IV \|pages = 297–321 \|bibcode = 2015aste.book..297N \|doi = 10.2458/azu_uapress_9780816532131-ch016 \|arxiv = 1502.01628 \|isbn = 9780816532131 }} 6. ^¹²{{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 = C. \|last6 = Nugent \|first7 = M. S. \|last7 = Cabrera \|date = November 2012 \|title = Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids \|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M \|journal = The Astrophysical Journal Letters \|volume = 759 \|issue = 1 \|page = 5 \|bibcode = 2012ApJ...759L...8M \|doi = 10.1088/2041-8205/759/1/L8 \|arxiv = 1209.5794 \|access-date= 6 September 2017}} 7. ^¹²{{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= 6 September 2017}} 8. ^¹{{cite web \|title = LCDB Data for (1767) Lampland \|publisher = Asteroid Lightcurve Database (LCDB) \|url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=1767%7CLampland \|accessdate = 6 September 2017}} ^[1]^[2]^[3]^[4]^[5]^[6]^[7]^[8] }} 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 (1)-(5000) – Minor Planet Center {{JPL small body}} {{Minor planets navigator \|1766 Slipher \|number=1767 \|1768 Appenzella}}{{Small Solar System bodies}}{{DEFAULTSORT:Lampland}} 6 : Eos asteroids\|Discoveries by Indiana University (Indiana Asteroid Program)\|Minor planets named for people\|Named minor planets\|XC-type asteroids (Tholen)\|Astronomical objects discovered in 1962
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Orbit and classification

Physical characteristics

Rotation period

Diameter and albedo

Naming

References

External links