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词条 3268 De Sanctis
释义

  1. Orbit and classification

  2. Physical characteristics

      Rotation period    Diameter and albedo  

  3. Naming

  4. References

  5. External links

{{Infobox planet
| minorplanet = yes
| name = 3268 De Sanctis
| background = #D6D6D6
| image =
| image_size =
| caption =
| discovery_ref =  [1]
| discoverer = H. Debehogne
G. de Sanctis
| discovery_site = La Silla Obs.
| discovered = 26 February 1981
| mpc_name = (3268) De Sanctis
| alt_names = 1981 DD{{·}}{{mp|1979 UQ|4}}
{{nowrap|{{mp|1979 WZ|1}}{{·}}{{mp|1990 WV|15}}}}
| pronounced =
| named_after = Giovanni de Sanctis [1]
{{small|(second discoverer)}}
| mp_category = main-belt{{·}}{{small|(inner)}}
Flora [3]{{·}}Vesta [4]
| orbit_ref =  
| epoch = 23 March 2018 (JD 2458200.5)
| uncertainty = 0
| observation_arc = 65.44 yr (23,902 d)
| aphelion = 2.6447 AU
| perihelion = 2.0490 AU
| semimajor = 2.3469 AU
| eccentricity = 0.1269
| period = 3.60 yr (1,313 d)
| mean_anomaly = 329.92°
| mean_motion = {{Deg2DMS|0.2741|sup=ms}} / day
| inclination = 6.3522°
| asc_node = 221.63°
| arg_peri = 74.723°
| mean_diameter = {{val|5.88|u=km}} {{small|(derived)}}[3]
{{val|6.033|0.120|u=km}}[7][8]
| rotation = {{val|17|ul=h}}[9]
| albedo = {{val|0.2280|0.0056}}[8]
{{val|0.228|0.006}}[7]
0.24 {{small|(assumed)}}[3]
| spectral_type = S {{small|(assumed)}}[3]
| abs_magnitude = 13.1{{·}}{{val|13.10|0.29}}[15]
13.32[3][8][9]
}}3268 De Sanctis, provisional designation {{mp|1981 DD}}, is a Vestian asteroid from the inner regions of the asteroid belt, approximately {{convert|6|km|mi|abbr=off|sp=us}} in diameter. It was discovered on 26 February 1981, by European astronomers Henri Debehogne and Giovanni de Sanctis at ESO's La Silla Observatory in northern Chile. The asteroid was named after the second discoverer.[1] The assumed S-type asteroid has a rotation period of 17 hours.[3]

Orbit and classification

De Sanctis a member of the Vesta family ({{small|401}}) when applying the hierarchical clustering method to its proper orbital elements.[4] Vestian asteroids have a composition akin to cumulate eucrites 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.[22][23] Based on osculating Keplerian orbital elements, De Sanctis has also been classified as a member of the Flora family ({{small|402}}), a giant asteroid family and the largest family of stony asteroids in the main-belt.[3]

The asteroid orbits the Sun in the inner main-belt at a distance of 2.0–2.6 AU once every 3 years and 7 months (1,313 days; semi-major axis of 2.35 AU). Its orbit has an eccentricity of 0.13 and an inclination of 6° with respect to the ecliptic.

The body's observation arc begins with a precovery taken at Palomar Observatory in December 1951, nearly three decades prior to its official discovery observation La Silla.[1]

Physical characteristics

De Sanctis is an assumed stony S-type asteroid.[3]

Rotation period

A first rotational lightcurve of De Sanctis was obtained from photometric observations by Polish astronomer Wiesław Wiśniewski at the University of Arizona. Lightcurve analysis gave a rotation period of 17 hours with a brightness amplitude of 0.4 magnitude ({{small|U=2}}).[9]

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, De Sanctis measures 6.033 kilometers in diameter and its surface has an albedo of 0.228,[7][8] while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora, the parent body of the Flora family – and derives a diameter of 5.88 kilometers based on an absolute magnitude of 13.32.[3]

Naming

This minor planet was named by the first discoverer after the second, Giovanni de Sanctis (born 1949), an Italian astronomer at the Observatory of Turin, who closely collaborated with Henri Debehogne at the European Southern Observatory in La Silla, Chile, during the early 1980s. The official naming citation was published by the Minor Planet Center on 22 June 1986 ({{small|M.P.C. 10849}}).[32]

References

1. ^{{cite web |title = 3268 De Sanctis (1981 DD) |work = Minor Planet Center |url = https://www.minorplanetcenter.net/db_search/show_object?object_id=3268 |accessdate = 15 March 2018}}
2. ^{{cite web |title = MPC/MPO/MPS Archive |work = Minor Planet Center |url = https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html |accessdate = 15 March 2018}}
3. ^{{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= 15 March 2018}}
4. ^{{cite web |title = Small Bodies Data Ferret |work = Nesvorny HCM Asteroid Families V3.0 |url = https://sbntools.psi.edu/ferret/PropertySearch/familyForm.action |accessdate = 15 March 2018}}
5. ^{{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= 15 March 2018}}
6. ^{{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 = 15 March 2018}}
7. ^{{cite web |title = LCDB Data for (3268) De Sanctis |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=3268%7CDe%20Sanctis |accessdate = 15 March 2018}}
8. ^{{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 = https://arxiv.org/pdf/1109.6407v1.pdf |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= 15 March 2018}}
9. ^{{Cite journal |author = Wisniewski, W. Z. |date = March 1991 |title = Physical studies of small asteroids. I - Lightcurves and taxonomy of 10 asteroids |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1991Icar...90..117W |journal = Icarus |pages = 117–122 |issn = 0019-1035 |bibcode = 1991Icar...90..117W |doi = 10.1016/0019-1035(91)90073-3 |access-date= 15 March 2018}}
10. ^{{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= 15 March 2018}}
[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 (1)-(5000) – Minor Planet Center
  • {{AstDys|3268}}
  • {{JPL small body}}
{{Use dmy dates|date=March 2018}}{{Minor planets navigator |3267 Glo |number=3268 |3269 Vibert-Douglas }}{{Small Solar System bodies}}{{DEFAULTSORT:De Sanctis}}

6 : Vesta asteroids|Discoveries by Henri Debehogne|Discoveries by Giovanni de Sanctis|Minor planets named for people|Named minor planets|Astronomical objects discovered in 1981

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