1737 Severny
Genus	Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010
Excentricitas	0.0505812
Axis semimaior perihelion aphelion	3.0122548 UA 2.8598913 UA 3.1646183 UA
Inclinatio orbitalis	9.37928°
Longitudo nodi ascendentis	327.50271°
Argumentum perihelii	225.70924°
Anomalia media	300.56887°
Periodus orbitalis	5.2281223863107 anni
Res physicae
Diameter	km
Massa	kg
Densitas media	g/cm3
Periodus rotationis	h m
Classis spectralis Tholen SMASS	— —
Magnitudo absoluta	10.8
Albedo	0.1811
De recognitione
Primus repertor	L. I. Chernykh
Repertum	die 13 Octobris 1966
Designationes aliae	1966 TJ, 1942 CA, 1944 OF, 1950 TM, 1950 TP4, 1951 YF2, 1963 DH

1737 Severny,^[1] olim designationibus 1966 TJ, 1942 CA, 1944 OF, 1950 TM, 1950 TP4, 1951 YF2, et 1963 DH agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 10.8 monstrat. Die 13 Octobris 1966 a Lyudmila Ivanovna Chernykh in Observatorio Astrophysico Crimaeae versato repertus est.^[2]

Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 1737 Severny per dies 1910 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 3.01 et eccentricitatem 0.05, distans igitur a sole quam minime unitatibus 2.86, quam maxime unitatibus 3.16. Inclinatio orbitalis 9.38° reperiebatur, anomalia media 300.57°.

Notae |

Nexus externi |

Data astronomica: "2001737" apud JPL Small-Body Database.

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

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Systema Solare nostrum

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

Planetulae: Ceres | Pluto | Haumea | Makemake | Eris | 225088 (2007 OR10) Corpora alia: Satellites | Luna | Asteroides (+ indices) | Corpora transneptuniana

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