词条 | 192 Nausikaa |
释义 |
| minorplanet= yes | mpc_name= (192) Nausikaa | background= #D6D6D6 | name= 192 Nausikaa | image= 192Nausikaa (Lightcurve Inversion).png | image_size = 265 | caption= A three-dimensional model of 192 Nausikaa based on its light curve. | pronounced= {{IPAc-en|n|ɔː|ˈ|s|ɪ|k|eɪ|.|ə}} {{Respell|naw|SIK|ay-ə}} | named_after= Nausicaä | mp_category= Main belt | semimajor= {{Convert|2.4028|AU|Gm|abbr=on}} | perihelion= {{Convert|1.8121|AU|Gm|abbr=on}} | aphelion= {{Convert|2.9934|AU|Gm|abbr=on|lk=on}} | period= 3.72 yr (1360.4 d) | inclination= 6.8137° | eccentricity= 0.24582 | dimensions= {{val|103.26|1.9|ul=km}}[1] 90.18 ± 2.80 km[2] | mass= {{nowrap|(1.79 ± 0.42) × 1018 kg[2]}} | density= 4.64 ± 1.17 g/cm3[2] | rotation= {{Convert|13.625|h|d|abbr=on|lk=on}} | spectral_type= S | magnitude= 8.2 | abs_magnitude= 7.13 | albedo= {{val|0.2330|0.009}} | discoverer= J. Palisa, 1879 | discovered= 17 February 1879 | epoch= 31 July 2016 (JD 2457600.5) | asc_node= 343.25° | arg_peri= 30.067° | mean_anomaly= 94.342° | mean_motion= {{Deg2DMS|0.26462|sup=ms}} / day | orbit_ref= [1] | observation_arc= 137.04 yr (50054 d) | uncertainty= 0 | moid= {{Convert|0.814558|AU|Gm|abbr=on}} | jupiter_moid= {{Convert|2.48275|AU|Gm|abbr=on}} | tisserand= 3.474 }} Nausikaa[2] (minor planet designation: 192 Nausikaa) is a large main-belt S-type asteroid. It was discovered by Johann Palisa on February 17, 1879, at Pula, then in Austria, now in Croatia. The name derives from Nausicaä, a princess in Homer's Odyssey. This is an S-type asteroid around 86 km with an elliptical ratio of 1.51. The sidereal rotation period is 13.6217 hours. Based on the lightcurve data obtained from Nausikaa, a possible satellite was reported in 1985. However, this has not been confirmed.[3] A shape model of Nausikaa has been constructed, also based on the lightcurve data. It indicates a roughly cut, but not very elongated body.[4] In 1998 an occultation of a star by the asteroid was observed from the United States. In 1988 a search for satellites or dust orbiting this asteroid was performed using the UH88 telescope at the Mauna Kea Observatories, but the effort came up empty.[10] Nausikaa's orbital period is 3.72 years, its distance from the Sun varying between 1.81 and 2.99 AU. The orbital eccentricity is 0.246. Nausikaa brightened to magnitude 8.3 at a quite favorable opposition on 2 September 2011, when it was 1.875 AU from the Sun and 0.866 AU from the Earth. References1. ^1 {{Cite web |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=192;cad=1 |title=192 Nausikaa |work=JPL Small-Body Database |publisher=NASA/Jet Propulsion Laboratory |access-date=12 May 2016}} [5][6]2. ^Stressed on the second syllable, {{IPAc-en|n|ɔː|ˈ|s|ɪ|k|eɪ|.|ə}} {{Respell|naw|SIK|ay-ə}}. 3. ^{{Citation|url=http://www.johnstonsarchive.net/astro/asteroidmoonsq.html |title=Other reports of asteroid/TNO companions |publisher=Johnstonsarchive.net |date= |accessdate=2012-09-01|postscript= }} 4. ^{{cite web |url=http://www.astro.helsinki.fi/~kaselain/asteroids.html |title=New worlds in our solar system|accessdate=2003-04-19 |deadurl=yes |archiveurl=https://web.archive.org/web/20030419143817/http://www.astro.helsinki.fi/~kaselain/asteroids.html |archivedate=2003-04-19 |df= }} 5. ^1 2 3 {{Citation | first1 = B. | last1 = Carry | title = Density of asteroids | work = Planetary and Space Science | volume = 73 | pages = 98–118 |date=December 2012 | doi = 10.1016/j.pss.2012.03.009 | bibcode = 2012P&SS...73...98C | postscript= .|arxiv = 1203.4336}} See Table 1. 6. ^1 {{Citation | last1 = Gradie | first1 = J. | last2 = Flynn | first2 = L. | title = A Search for Satellites and Dust Belts Around Asteroids: Negative Results | work = Abstracts of the Lunar and Planetary Science Conference | volume = 19 | pages = 405–406 |date=March 1988 | bibcode = 1988LPI....19..405G | postscript= .}} }} External links
8 : Background asteroids|Discoveries by Johann Palisa|Minor planets named from Greek mythology|Named minor planets|S-type asteroids (Tholen)|Sl-type asteroids (SMASS)|Astronomical objects discovered in 1879|Objects observed by stellar occultation |
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