“110 Lydia”的意思、由来-开放百科全书

Lydia (minor planet designation: (110 Lydia) is a large belt asteroid with an M-type spectrum,^[6] and thus may be metallic in composition, consisting primarily of nickel-iron. It was discovered by French astronomer Alphonse Borrelly on April 19, 1870 and was named for Lydia, the Asia Minor country populated by Phrygians.^[13] The Lydia family of asteroids is named after it.

Observations made during 1958–1959 at the McDonald Observatory and in 1969 at the Kitt Peak National Observatory found an uneven light curve with a period of 10.9267 hours.^[14] In the late 1990s, a network of astronomers worldwide used light curves to derive spin states and shape models of 10 new asteroids, including (110) Lydia. They obtained a period of 10.92580 hours, with the brightness varying by no more than 0.2 in magnitude.^[5]

In the Tholen classification system, it is categorized as an M-type asteroid, while the Bus asteroid taxonomy system lists it as an Xk asteroid.^[16] Absorption features in the near infrared are attributed to low-iron, low-calcium orthopyroxene minerals. Water content on the surface is estimated at 0.14–0.27 by mass fraction (wt%).^[17] Measurements of the thermal inertia of 110 Lydia give a value between 70 and 200 J m⁻² K⁻¹ s^−1/2, compared to 50 for lunar regolith and 400 for coarse sand in an atmosphere.^[3] It is a likely interloper in the Padua family of minor planets that share similar dynamic properties.^[19]

References

1. ^¹²³⁴⁵{{Citation | first1 = Donald K. | last1 = Yeomans | title = 110 Lydia | work = JPL Small-Body Database Browser | publisher = NASA Jet Propulsion Laboratory | url = http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=110 | accessdate= 12 May 2016 | postscript= .}}
2. ^¹{{Citation | first1 = Lutz D. | last1 = Schmadel | title = Dictionary of Minor Planet Names | publisher = Springer | edition = 5th | page = 23 | date = 2003 | isbn = 3-540-00238-3 | postscript= .}}
3. ^¹{{Citation | last1 = Carruba | first1 = V. | title = The (not so) peculiar case of the Padua family | journal = Monthly Notices of the Royal Astronomical Society | volume = 395 | issue = 1 | pages = 358–377 |date=May 2009 | bibcode = 2009MNRAS.395..358C | postscript= .|doi = 10.1111/j.1365-2966.2009.14523.x }}
4. ^¹²{{Citation |first1 = Francesca E. |last1 = DeMeo |first2 = Richard P. |last2 = Binzel |first3 = Stephen M. |last3 = Slivan |first4 = Schelte J. |last4 = Bus |display-authors = 1 |title = An extension of the Bus asteroid taxonomy into the near-infrared |journal = Icarus |volume = 202 |issue = 1 |pages = 160–180 |date = 2011 |doi = 10.1016/j.icarus.2009.02.005 |bibcode = 2009Icar..202..160D |url = http://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016%252Fj.icarus.2009.02.005.pdf |accessdate = 2013-12-11 |postscript = . |deadurl = yes |archiveurl = https://web.archive.org/web/20140317200310/https://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016/j.icarus.2009.02.005.pdf |archivedate = 2014-03-17 |df = }} See appendix A.
5. ^¹{{Citation | last1 = Taylor | first1 = R. C. | last2 = Gehrels | first2 = T. | last3 = Silvester | first3 = A. B. | display-authors = 1 | title = Minor Planets and Related Objects. VI. Asteroid (110) Lydia | work = Astronomical Journal | volume = 76 | page = 141 |date=March 1971 | doi = 10.1086/111097 | bibcode = 1971AJ.....76..141T | postscript= .}}
6. ^¹²{{Citation | last1 = Durech | first1 = J. | last2 = Kaasalainen | first2 = M. | last3 = Marciniak | first3 = A. | display-authors = 1 | title = Physical models of ten asteroids from an observers' collaboration network | work = Astronomy and Astrophysics | volume = 465 | issue = 1 | pages = 331–337 |date=April 2007 | doi = 10.1051/0004-6361:20066347 | bibcode = 2007A&A...465..331D | postscript= .}}
7. ^¹²³⁴{{Citation | last1 = Delbo' | first1 = Marco | last2 = Tanga | first2 = Paolo | title = Thermal inertia of main belt asteroids smaller than 100 km from IRAS data | work = Planetary and Space Science | volume = 57 | issue = 2 | pages = 259–265 |date=February 2009 | doi = 10.1016/j.pss.2008.06.015 | bibcode = 2009P&SS...57..259D | postscript= .|arxiv = 0808.0869 }}
8. ^¹{{Citation |last1=Hardersen |first1=Paul S. |last2=Gaffey |first2=Michael J. |last3=Abell |first3=Paul A. |title=Near-IR spectral evidence for the presence of iron-poor orthopyroxenes on the surfaces of six M-type asteroids |work=Icarus |volume=175 |issue=1 |pages=141–158 |date=January 1983 |doi=10.1016/j.icarus.2004.10.017 |bibcode=2005Icar..175..141H |url= |postscript=. }}
9. ^¹{{Citation |last1 = DeMeo |first1 = Francesca E. |last2 = Binzel |first2 = Richard P. |last3 = Slivan |first3 = Stephen M. |last4 = Bus |first4 = Schelte J. |display-authors = 1 |title = An extension of the Bus asteroid taxonomy into the near-infrared |work = Icarus |volume = 202 |issue = 1 |pages = 160–180 |date = July 2009 |doi = 10.1016/j.icarus.2009.02.005 |bibcode = 2009Icar..202..160D |url = http://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016%252Fj.icarus.2009.02.005.pdf |accessdate = 2013-04-08 |postscript = . |deadurl = yes |archiveurl = https://web.archive.org/web/20140317200310/https://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016/j.icarus.2009.02.005.pdf |archivedate = 2014-03-17 |df = }} See appendix A.

References

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