About: 246P/NEAT     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:Whole100003553, within Data Space : dbpedia.org associated with source document(s)
QRcode icon
http://dbpedia.org/describe/?url=http%3A%2F%2Fdbpedia.org%2Fresource%2F246P%2FNEAT

246P/NEAT is a periodic comet discovered on 2004 March 28 by Near-Earth Asteroid Tracking (NEAT) using the 1.2-metre (47 in) reflector at Haleakala. It was given the permanent number 246P on 2011 January 14. It is a Quasi-Hilda comet. Due to perturbations by Jupiter, the 2005, 2013 and 2021 perihelion passages will be closer to the Sun. The comet is observable all through its orbit.

AttributesValues
rdf:type
rdfs:label
  • 246P/NEAT (en)
  • 246P/NEAT (fr)
  • 246P/NEAT (it)
  • 246P/NEAT (pl)
  • 246P/NEAT (zh)
rdfs:comment
  • 246P/NEAT is a periodic comet discovered on 2004 March 28 by Near-Earth Asteroid Tracking (NEAT) using the 1.2-metre (47 in) reflector at Haleakala. It was given the permanent number 246P on 2011 January 14. It is a Quasi-Hilda comet. Due to perturbations by Jupiter, the 2005, 2013 and 2021 perihelion passages will be closer to the Sun. The comet is observable all through its orbit. (en)
  • 246P/NEAT est une comète périodique du système solaire. Elle fut découverte le 28 mars 2004 par le programme Near Earth Asteroid Tracking (NEAT) grâce au télescope de 1,2 mètre au Haleakalā. Elle a reçu sa désignation permanente 246P le 14 janvier 2011.Il s'agit d'une comète quasi-Hilda. En raison de perturbations de Jupiter, les passages au périhélie de 2005, 2013 et 2021 seront plus proches du Soleil. La comète est observable tout le long de son orbite. (fr)
  • 246P/NEAT, o anche cometa NEAT 20, è una cometa periodica scoperta il 15 marzo 2004, in seguito si sono trovate immagini di prescoperta risalenti al 29 gennaio 2004: la cometa ha ricevuto la sua denominazione definitiva dopo la sua riscoperta avvenuta il 2 novembre 2010. La cometa fa parte della famiglia delle comete gioviane e della famiglia di comete quasi-Hilda. La cometa ha avuto nel 2001 un lungo passaggio ravvicinato col pianeta Giove. (it)
  • 246P/NEAT – kometa krótkookresowa, należąca do rodziny Jowisza. (pl)
  • 246/NEAT是一颗周期彗星，由近地小行星追踪和的1.2米反射望远镜与2004年3月28日发现。它于2011年1月14日获得了永久编号246P。 它是一颗。因为木星的摄动，2005年、2013年和2021年通过近日点时一次比一次更接近太阳。这颗彗星在轨道上运转的全过程都是可以观测到的。 (zh)
name
dcterms:subject
Wikipage page ID
Wikipage revision ID
Link from a Wikipage to another Wikipage
Link from a Wikipage to an external page
sameAs
dbp:wikiPageUsesTemplate
aphelion
designations
discoverer
discovery date
eccentricity
epoch
inclination
last p
next p
perihelion
period
semimajor
has abstract
  • 246P/NEAT is a periodic comet discovered on 2004 March 28 by Near-Earth Asteroid Tracking (NEAT) using the 1.2-metre (47 in) reflector at Haleakala. It was given the permanent number 246P on 2011 January 14. It is a Quasi-Hilda comet. Due to perturbations by Jupiter, the 2005, 2013 and 2021 perihelion passages will be closer to the Sun. The comet is observable all through its orbit. (en)
  • 246P/NEAT est une comète périodique du système solaire. Elle fut découverte le 28 mars 2004 par le programme Near Earth Asteroid Tracking (NEAT) grâce au télescope de 1,2 mètre au Haleakalā. Elle a reçu sa désignation permanente 246P le 14 janvier 2011.Il s'agit d'une comète quasi-Hilda. En raison de perturbations de Jupiter, les passages au périhélie de 2005, 2013 et 2021 seront plus proches du Soleil. La comète est observable tout le long de son orbite. (fr)
  • 246P/NEAT, o anche cometa NEAT 20, è una cometa periodica scoperta il 15 marzo 2004, in seguito si sono trovate immagini di prescoperta risalenti al 29 gennaio 2004: la cometa ha ricevuto la sua denominazione definitiva dopo la sua riscoperta avvenuta il 2 novembre 2010. La cometa fa parte della famiglia delle comete gioviane e della famiglia di comete quasi-Hilda. La cometa ha avuto nel 2001 un lungo passaggio ravvicinato col pianeta Giove. (it)
  • 246P/NEAT – kometa krótkookresowa, należąca do rodziny Jowisza. (pl)
  • 246/NEAT是一颗周期彗星，由近地小行星追踪和的1.2米反射望远镜与2004年3月28日发现。它于2011年1月14日获得了永久编号246P。 它是一颗。因为木星的摄动，2005年、2013年和2021年通过近日点时一次比一次更接近太阳。这颗彗星在轨道上运转的全过程都是可以观测到的。 (zh)
gold:hypernym
prov:wasDerivedFrom
page length (characters) of wiki page
foaf:isPrimaryTopicOf
is Link from a Wikipage to another Wikipage of
is foaf:primaryTopic of
Faceted Search & Find service v1.17_git139 as of Feb 29 2024


Alternative Linked Data Documents: ODE     Content Formats:   [cxml] [csv]     RDF   [text] [turtle] [ld+json] [rdf+json] [rdf+xml]     ODATA   [atom+xml] [odata+json]     Microdata   [microdata+json] [html]    About   
This material is Open Knowledge   W3C Semantic Web Technology [RDF Data] Valid XHTML + RDFa
OpenLink Virtuoso version 08.03.3330 as of Mar 19 2024, on Linux (x86_64-generic-linux-glibc212), Single-Server Edition (378 GB total memory, 53 GB memory in use)
Data on this page belongs to its respective rights holders.
Virtuoso Faceted Browser Copyright © 2009-2024 OpenLink Software