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{{Short description|Main-belt asteroid}}
{{Use dmy dates|date=October 2019}}
{{Infobox planet
| minorplanet=yes
| background=#D6D6D6
| name=444 Gyptis
| discoverer=[[Jérôme Eugène Coggia]]
| discovered=31 March 1899
| mpc_name=(444) Gyptis
| alt_names=1899 EL
| pronounced={{IPAc-en|'|dZ|I|p|t|I|s}}
|
| adjective = Gyptidian
| mp_category=[[Asteroid belt|Main belt]]
| epoch=31 July 2016 ([[Julian day|JD]] 2457600.5)
| semimajor={{Convert|2.77005|AU|Gm|abbr=on}}
| perihelion={{Convert|2.28337|AU|Gm|abbr=on}}
| aphelion={{Convert|3.25674|AU|Gm|abbr=on|lk=on}}
| eccentricity=0.17569
| period=4.61 [[Julian year (astronomy)|yr]] (1684.0 [[Julian year (astronomy)|d]])
| inclination=10.2775°
| asc_node=195.716°
| arg_peri=154.984°
| mean_anomaly=11.8852[[Degree (angle)|°]]
| dimensions=179×150 km<ref name=euraster/>
| mean_diameter = {{val|159.331|0.490|ul=km}}<ref name=jpldata>{{cite web
|type=2024-09-25 last obs
|title=JPL Small-Body Database Browser: 444 Gyptis (1899 EL)
|url=https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=444
|access-date=19 Dec 2024}}</ref><br>{{val|164.63|2.60|ul=km}}<ref name="Carry2012"/>
| mass=1.25{{e|19}} kg<ref name=Baer>
{{cite web
|date=2008
|title=Recent Asteroid Mass Determinations
|publisher=Personal Website
|author=Jim Baer
|url=http://home.earthlink.net/~jimbaer1/astmass.txt
|access-date=2008-11-27
|archive-url=https://web.archive.org/web/20130702212735/http://home.earthlink.net/~jimbaer1/astmass.txt
|archive-date=2013-07-02
|url-status=dead
}}
</ref><br>{{val|1.06|0.28|e=19|u=kg}}<ref name="Carry2012"/>
| density=5.53±1.46 g/cm<sup>3</sup><ref name=Baer/><br>{{val|4.55|1.23|u=g/cm3}}<ref name="Carry2012"/>
| rotation={{Convert|6.214|h|d|abbr=on|lk=on}}<ref name=jpldata/>
| spectral_type=[[C-type asteroid|C]]<ref name=jpldata/>
| abs_magnitude=8.07<ref name=jpldata/>
| albedo={{val|0.051|0.008}}<ref name=jpldata/>
| mean_motion={{Deg2DMS|0.213782|sup=ms}} / day
| orbit_ref=<ref name=jpldata />
| observation_arc=116.54 yr (42568 d)
| uncertainty=0
}}
'''444 Gyptis''' is a
In 2004, Kochetova estimated Gyptis to have a mass of 1.25{{e|19}} kg with a high density of 5.53 g/cm<sup>3</sup>.<ref name=Baer/> In 2012 Carry estimated the mass as {{val|1.06|0.28|e=19|u=kg}} with a high density of {{val|4.55|1.23|u=g/cm3}}.<ref name="Carry2012"/> The [[adaptive optics]] instrument at the [[W. M. Keck Observatory]] showed an object with a diameter of 129 km, which is much smaller than the estimate of 160 km from the [[IRAS]] observatory measurements, indicating an irregular shape. The size ratio between the major and minor axes is estimated at 1.40.<ref name="Marchis2006"/> Observations of an [[occultation]] on October 14, 2007, produced six [[Chord (astronomy)|chords]] indicating a cross-section ellipsoid of 179×150 km.<ref name=euraster>{{cite web|date=2007-10-14|title=2007 European Asteroidal Occultation Results|publisher=euraster.net (a website for Asteroidal Occultation Observers in Europe)|url=http://www.euraster.net/results/2007/index.html#1014-444|access-date=2008-12-01}} [http://www.euraster.net/results/2007/20071014-Gyptis-crd.gif (Chords)]</ref>
Between 1990 and 2021, 444 Gyptis has been observed to [[occultation|occult]] 17 stars.
==References==
{{Reflist|refs=
<ref name=Fornasier1999>{{citation
| title=Spectroscopic comparison of aqueous altered asteroids with CM2 carbonaceous chondrite meteorites
| display-authors=1 | postscript=.
| last1=Fornasier | first1=S. | last2=Lazzarin | first2=M.
| last3=Barbieri | first3=C. | last4=Barucci | first4=M. A.
| journal=Astronomy and Astrophysics Supplement
| volume=135 | pages=65−73 | date=February 1999
| doi=10.1051/aas:1999161 | bibcode=1999A&AS..135...65F | doi-access=free }}</ref>
<ref name="Marchis2006">{{Citation
| first1 = F.
| last1 = Marchis
| first2 = M.
| last2 = Kaasalainen
| first3 = E. F. Y.
| last3 = Hom
| first4 = J.
| last4 = Berthier
| first5 = J.
| last5 = Enriquez
| first6 = D.
| last6 = Hestroffer
| first7 = D.
| last7 = Le Mignant
| first8 = I.
| last8 = de Pater
| display-authors = 1
| title = Shape, size and multiplicity of main-belt asteroids. I. Keck Adaptive Optics survey
| journal = Icarus
| volume = 185
| issue = 1
| pages = 39–63
| date=November 2006
| bibcode = 2006Icar..185...39M
| doi = 10.1016/j.icarus.2006.06.001
| postscript= .
| pmid=19081813
| pmc=2600456
}}</ref>
<ref name="Carry2012">{{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.</ref>
}} <!-- end of reflist -->
== External links ==
* {{AstDys|444}}
* {{JPL small body}}
{{Minor planets navigator |443 Photographica |number=444 |445 Edna}}
{{Small Solar System bodies}}
{{Authority control}}
{{DEFAULTSORT:000444}}
[[Category:Background asteroids]]
[[Category:Discoveries by Jérôme Coggia|Gyptis]]
[[Category:Named minor planets|Gyptis]]
[[Category:C-type asteroids (Tholen)]]
[[Category:C-type asteroids (SMASS)]]
[[Category:Astronomical objects discovered in 1899|18990331]]
[[Category:Objects observed by stellar occultation]]
{{C-beltasteroid-stub}}
|