“6793 Palazzolo”的意思、由来-开放百科全书

In 1982, the asteroid was first identified as {{mp|1982 YS|2}} at Crimea–Nauchnij. Its observation arc begins 1990, with its identification as {{mp|1990 SZ|23}} at ESO's La Silla Observatory, 1 year prior to its official discovery observation at Bassano Bresciano.^[22]

Physical characteristics

Rotation period

In 2012, a rotational lightcurve of Palazzolo was obtained from photometric observations at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of {{val|6.2308}} hours with a brightness amplitude of 0.16 in magnitude ({{small|U=2}}).^[10]

Follow-up observations in 2013 and 2014, gave a similar period of {{val|6.190}} and {{val|6.2323}} hours with an amplitude of 0.16 and 0.14, respectively ({{small|U=2/2}}).^[10]^[8]

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, Palazzolo has a diameter of 9.9 kilometers and an albedo of 0.083,^[6]^[7] while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.10 and calculates a diameter of 8.0 kilometers.^[3]

Naming

This minor planet is named after the Italian city of Palazzolo sull'Oglio, located between Brescia and Bergamo, in northern parts of the country. Known for its industries, including the first Italian factories producing cement and buttons, the city is now famous for its of spinning machines and zippers. It was founded on the banks of river Oglio, with archaeological findings dating back to the Roman era.^[2] The approved naming citation was published by the Minor Planet Center on 4 April 1996 ({{small|M.P.C. 26933}}).^[34]

References

1. ^¹²³{{cite book |title = Dictionary of Minor Planet Names – (6793) Palazzolo |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |page = 557 |date = 2007 |isbn = 978-3-540-00238-3 |doi = 10.1007/978-3-540-29925-7_6105 |chapter = (6793) Palazzolo }}
2. ^¹²{{cite web |title = 6793 Palazzolo (1991 YE) |work = Minor Planet Center |url = http://www.minorplanetcenter.net/db_search/show_object?object_id=6793 |accessdate = 29 March 2016}}
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 = 17 May 2016}}
4. ^¹²³⁴⁵⁶⁷{{cite web |title = LCDB Data for (6793) Palazzolo |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=6793%7CPalazzolo |accessdate = 17 May 2016}}
5. ^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 |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...90M |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 |access-date= 17 May 2016}}
6. ^¹²³{{cite journal |display-authors = 6 |first1 = Chan-Kao |last1 = Chang |first2 = Wing-Huen |last2 = Ip |first3 = Hsing-Wen |last3 = Lin |first4 = Yu-Chi |last4 = Cheng |first5 = Chow-Choong |last5 = Ngeow |first6 = Ting-Chang |last6 = Yang |first7 = Adam |last7 = Waszczak |first8 = Shrinivas R. |last8 = Kulkarni |first9 = David |last9 = Levitan |first10 = Branimir |last10 = Sesar |first11 = Russ |last11 = Laher |first12 = Jason |last12 = Surace |first13 = Thomas. A. |last13 = Prince |date = August 2015 |title = Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJS..219...27C |journal = The Astrophysical Journal Supplement Series |volume = 219 |issue = 2 |page = 19 |bibcode = 2015ApJS..219...27C |doi = 10.1088/0067-0049/219/2/27 |arxiv = 1506.08493 |access-date= 17 May 2016}}
7. ^¹²³⁴⁵⁶{{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= 17 May 2016}}
8. ^¹{{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= 17 May 2016}}
9. ^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= 5 December 2016}}

词条	6793 Palazzolo
释义	Orbit and classification Physical characteristics Rotation period Diameter and albedo Naming References External links {{Infobox planet \| minorplanet = yes \| name = 6793 Palazzolo \| background = #D6D6D6 \| image = \| image_size = \| caption = \| discovery_ref = \| discovered = 30 December 1991 \| discoverer = U. Quadri L. Strabla \| discovery_site = Bassano Bresciano Obs. \| mpc_name = (6793) Palazzolo \| alt_names = 1991 YE{{·}}{{mp\|1982 YS\|2}} {{mp\|1990 SZ\|23}} \| named_after = Palazzolo sull'Oglio {{small\|(Italian city)}}^[2] \| mp_category = main-belt{{·}}{{small\|(middle)}} ^[3] \| orbit_ref = \| epoch = 4 September 2017 (JD 2458000.5) \| uncertainty = 0 \| observation_arc = 33.90 yr (12,382 days) \| aphelion = 3.1007 AU \| perihelion = 2.2594 AU \| semimajor = 2.6800 AU \| eccentricity = 0.1569 \| period = 4.39 yr (1,603 days) \| mean_anomaly = 273.56° \| mean_motion = {{Deg2DMS\|0.2246\|sup=ms}} / day \| inclination = 4.9244° \| asc_node = 106.38° \| arg_peri = 46.196° \| dimensions = 8.01 km {{small\|(calculated)}}^[3] {{val\|9.882\|0.051}} km^[6]^[7] \| rotation = {{val\|6.190\|0.040}} h^[8] {{val\|6.2308\|0.0072}} h^[3]^[10] {{val\|6.2323\|0.0072}} h^[10] \| albedo = {{val\|0.083\|0.004}}^[6]^[7] 0.10 {{small\|(assumed)}}^[3] \| spectral_type = S ^[3] \| abs_magnitude = 13.6{{·}}{{val\|13.78\|0.23}}^[17]{{·}}{{val\|13.520\|0.110}}^[8]{{·}}13.3^[6]{{·}}{{val\|14.143\|0.005}} {{small\|(S)}}^[10]{{·}}{{val\|13.709\|0.002}} {{small\|(R)}}^[10] }}6793 Palazzolo, provisional designation {{mp\|1991 YE}}, is a stony asteroid from the middle region of the asteroid belt, approximately 9 kilometers in diameter. It was discovered on 30 December 1991, by Italian amateur astronomers Ulisse Quadri and Luca Strabla at the Bassano Bresciano Observatory in northern Italy.^[22] The asteroid was named after the Italian city of Palazzolo sull'Oglio.^[2] Orbit and classification Palazzolo orbits the Sun in the central main-belt at a distance of 2.3–3.1 AU once every 4 years and 5 months (1,603 days). Its orbit has an eccentricity of 0.16 and an inclination of 5° with respect to the ecliptic. In 1982, the asteroid was first identified as {{mp\|1982 YS\|2}} at Crimea–Nauchnij. Its observation arc begins 1990, with its identification as {{mp\|1990 SZ\|23}} at ESO's La Silla Observatory, 1 year prior to its official discovery observation at Bassano Bresciano.^[22] Physical characteristics Palazzolo is an assumed S-type asteroid.^[3] Rotation period In 2012, a rotational lightcurve of Palazzolo was obtained from photometric observations at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of {{val\|6.2308}} hours with a brightness amplitude of 0.16 in magnitude ({{small\|U=2}}).^[10] Follow-up observations in 2013 and 2014, gave a similar period of {{val\|6.190}} and {{val\|6.2323}} hours with an amplitude of 0.16 and 0.14, respectively ({{small\|U=2/2}}).^[10]^[8] Diameter and albedo According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, Palazzolo has a diameter of 9.9 kilometers and an albedo of 0.083,^[6]^[7] while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.10 and calculates a diameter of 8.0 kilometers.^[3] Naming This minor planet is named after the Italian city of Palazzolo sull'Oglio, located between Brescia and Bergamo, in northern parts of the country. Known for its industries, including the first Italian factories producing cement and buttons, the city is now famous for its of spinning machines and zippers. It was founded on the banks of river Oglio, with archaeological findings dating back to the Roman era.^[2] The approved naming citation was published by the Minor Planet Center on 4 April 1996 ({{small\|M.P.C. 26933}}).^[34] References 1. ^¹²³{{cite book \|title = Dictionary of Minor Planet Names – (6793) Palazzolo \|last = Schmadel \| first = Lutz D. \|publisher = Springer Berlin Heidelberg \|page = 557 \|date = 2007 \|isbn = 978-3-540-00238-3 \|doi = 10.1007/978-3-540-29925-7_6105 \|chapter = (6793) Palazzolo }} 2. ^¹²{{cite web \|title = 6793 Palazzolo (1991 YE) \|work = Minor Planet Center \|url = http://www.minorplanetcenter.net/db_search/show_object?object_id=6793 \|accessdate = 29 March 2016}} 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 = 17 May 2016}} 4. ^¹²³⁴⁵⁶⁷{{cite web \|title = LCDB Data for (6793) Palazzolo \|publisher = Asteroid Lightcurve Database (LCDB) \|url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=6793%7CPalazzolo \|accessdate = 17 May 2016}} 5. ^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 \|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...90M \|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 \|access-date= 17 May 2016}} 6. ^¹²³{{cite journal \|display-authors = 6 \|first1 = Chan-Kao \|last1 = Chang \|first2 = Wing-Huen \|last2 = Ip \|first3 = Hsing-Wen \|last3 = Lin \|first4 = Yu-Chi \|last4 = Cheng \|first5 = Chow-Choong \|last5 = Ngeow \|first6 = Ting-Chang \|last6 = Yang \|first7 = Adam \|last7 = Waszczak \|first8 = Shrinivas R. \|last8 = Kulkarni \|first9 = David \|last9 = Levitan \|first10 = Branimir \|last10 = Sesar \|first11 = Russ \|last11 = Laher \|first12 = Jason \|last12 = Surace \|first13 = Thomas. A. \|last13 = Prince \|date = August 2015 \|title = Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory \|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJS..219...27C \|journal = The Astrophysical Journal Supplement Series \|volume = 219 \|issue = 2 \|page = 19 \|bibcode = 2015ApJS..219...27C \|doi = 10.1088/0067-0049/219/2/27 \|arxiv = 1506.08493 \|access-date= 17 May 2016}} 7. ^¹²³⁴⁵⁶{{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= 17 May 2016}} 8. ^¹{{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= 17 May 2016}} 9. ^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= 5 December 2016}} ^[1]^[2]^[3]^[4]^[5]^[6]^[7]^[8]^[9] }} 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\|6793}} {{JPL small body}} {{Minor planets navigator \|6792 Akiyamatakashi \|number=6793 \|6794 Masuisakura}}{{Small Solar System bodies}}{{DEFAULTSORT:Palazzolo}} 6 : Vibilia asteroids\|Leonidas asteroids\|Discoveries by the Osservatorio Astronomico di Bassano Bresciano\|Minor planets named for places\|Named minor planets\|Astronomical objects discovered in 1991
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Orbit and classification

Physical characteristics

Rotation period

Diameter and albedo

Naming

References

External links