3915 Fukushima Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2003915Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1988 repertiAsteroides Cinguli Principalis


asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam15 Augusti1988Masayuki YanaiKazuro WatanabeObservatorium Kitamiepochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana








































3915 Fukushima



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
0.0398281

Axis semimaior

perihelion
aphelion

2.4388969 UA
2.3417603 UA
2.5360335 UA


Inclinatio orbitalis
14.44026°

Longitudo nodi ascendentis
173.58739°

Argumentum perihelii
144.26631°

Anomalia media
233.14058°

Periodus orbitalis
3.8088894442163 anni
Res physicae

Diameter

km

Massa

kg

Densitas media
g/cm3

Periodus rotationis
8 h 23.999977 m

Classis spectralis

Tholen
SMASS






Magnitudo absoluta
12.20

Albedo
0.0561
De recognitione
Primi repertores

M. Yanai, K. Watanabe
Repertum
die 15 Augusti 1988
Designationes aliae
1988 PA1, 1926 GQ, 1935 UL, 1935 UX, 1950 QT, 1975 EX5, 1977 TV7, 1977 TW3, 1979 FH1, 1983 EM

3915 Fukushima,[1] olim designationibus 1988 PA1, 1926 GQ, 1935 UL, 1935 UX, 1950 QT, 1975 EX5, 1977 TV7, 1977 TW3, 1979 FH1, et 1983 EM agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 12.20 monstrat. Die 15 Augusti 1988 a Masayuki Yanai et Kazuro Watanabe, astronomis apud Observatorium Kitami versatis, repertus est.[2]


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 3915 Fukushima per dies 1391 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 2.44 et eccentricitatem 0.04, distans igitur a sole quam minime unitatibus 2.34, quam maxime unitatibus 2.54. Inclinatio orbitalis 14.44° reperiebatur, anomalia media 233.14°.



Notae |



  1. Nomina asteroidum iussu Unionis Astronomicae Internationalis imposita sunt.


  2. "Discovery Circumstances: Numbered Minor Planets" .mw-parser-output .existinglinksgray a,.mw-parser-output .existinglinksgray a:visitedcolor:gray.mw-parser-output .existinglinksgray a.newcolor:#ba0000.mw-parser-output .existinglinksgray a.new:visitedcolor:#a55858
    (Anglice). IAU Minor Planet Center. Universitas Harvardiana 




Nexus externi |





Wikidata-logo.svg

Data astronomica: "2003915" apud JPL Small-Body Database.

P literature.svgHaec commentatio, automatice praeparata, res astronomicas colligit excerptas e pagina [1] sitús Small-Body Database, quem elaboraverunt NASA et JPL apud Institutum Technologiae Californiense.






Systema Solare nostrum



SolMercuriusVenusLunaTellus/TerraMarsPhobos et DeimosCeresCingulus asteroidum principalisIuppiterSatellites IuppiterisAnuli IuppiterisSaturnusSatellites SaturniAnuli SaturniUranusSatellites UraniAnuli UraniNeptunusSatellites NeptuniAnuli NeptuniPlutoSatellites PlutonisHaumeaSatellites HaumeaeMakemakeZona KuiperiErisDysnomiaDiscus RarusNubes HillsNubes OortSolar System Template Final.png


Sol

Planetae: Mercurius | Venus | Tellus (Terra) | Mars | Iuppiter | Saturnus | Uranus | Neptunus



Planetulae: Ceres | Pluto | Haumea | Makemake | Eris

Corpora alia: Satellites | Luna | Asteroides (+ indices) | Corpora transneptuniana


Vide etiam indices corporum Systematis Solaris redactos secundum radium et massam.

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