199 Byblis Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2000199Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1879 repertiAsteroides Cinguli PrincipalisAsteroides e mythologia Graeca appellati


Byblis (discretiva)asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam9 Iulii1879Christiano Henrico Friderico PetersObservatorio Litchfieldmythologia GraecaByblisMiletiCauniepochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana





Vide etiam paginam discretivam: Byblis (discretiva)







































199 Byblis



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
.1725700717102225

Axis semimaior

perihelion
aphelion

3.178025804985383 UA
2.629593663922118 UA
3.726457946048648 UA


Inclinatio orbitalis
15.42781588037059°

Longitudo nodi ascendentis
88.94837044421411°

Argumentum perihelii
180.3247740405142°

Anomalia media
27.39436554506999°

Periodus orbitalis
5.6655794111328 anni
Res physicae

Diameter

km

Massa

kg

Densitas media
g/cm3

Periodus rotationis
5 h 13.199987 m

Classis spectralis

Tholen
SMASS



—
X


Magnitudo absoluta
8.3

Albedo
—
De recognitione
Primus repertor

C. H. F. Peters
Repertum
die 9 Iulii 1879
Designationes aliae
1971 WB

199 Byblis,[1] olim designatione 1971 WB agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 8.3 monstrat. Die 9 Iulii 1879 a Christiano Henrico Friderico Peters in Observatorio Litchfield versato repertus est.[2] In mythologia Graeca Byblis, e qua asteroides appellatus est, fuit Mileti filia et fratris sui Cauni amatrix.


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 199 Byblis per dies 2069 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 3.18 et eccentricitatem 0.17, distans igitur a sole quam minime unitatibus 2.63, quam maxime unitatibus 3.73. Inclinatio orbitalis 15.43° reperiebatur, anomalia media 27.39°.



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: "2000199" 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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