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{{Infobox planet |
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| extrasolarplanet = no |
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| name = V774104 |
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| image = |
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| caption = |
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| apsis = |
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| discovery_ref = |
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| discoverer = |
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| discovery_site = |
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| discovered = <!--(Date)--> |
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| discovery_method = |
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| alt_names = |
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| periastron = |
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| apoastron = |
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| semimajor = |
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| avg_speed = |
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| eccentricity = |
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| inclination = |
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| angular_dist = |
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| long_periastron = |
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| time_periastron = |
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| semi-amplitude = |
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| mean_radius = |
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| surface_area = |
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| moment_of_inertia_factor = |
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| escape_velocity = |
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| albedo = |
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| single_temperature = |
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}} |
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{{Disputed|date=July 2019}} |
{{Disputed|date=July 2019}} |
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{{short description|Trans-Neptunian object}} |
{{short description|Trans-Neptunian object}} |
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{{Use dmy dates|date=July 2019}} |
{{Use dmy dates|date=July 2019}} |
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'''V774104''' is the internal designation for the [[trans-Neptunian object]] designated {{mpl|2015 TH|367}}, but in November 2015 press releases confused it with {{ |
'''V774104''' is the internal designation for the [[trans-Neptunian object]] designated {{mpl|2015 TH|367}}, but in November 2015 press releases confused it with [[541132 Leleākūhonua]], which was [[Provisional designation in astronomy|provisionally designated]] {{mp|2015 TG|387}} and internally designated V302126.<ref name=Trujillo2018/> as both objects were mentioned at the [[American Astronomical Society]]’s [[Division for Planetary Sciences]] meeting. Various news articles speculated that V774104 was currently {{Convert|103|AU|e9km|abbr=unit|lk=on}} from the Sun, but its [[observation arc]] was too short to know whether its [[Apsis|perihelion]] (closest approach to the Sun) was even outside Neptune's influence.<ref name=nature2015/> |
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{| class="wikitable sortable" style="font-size: 0.9em;" |
{| class="wikitable sortable" style="font-size: 0.9em;" |
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|Neptune<br/>(for comparison) || 30 || 30 || Planet |
|Neptune<br/>(for comparison) || 30 || 30 || Planet |
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|{{ |
|[[541132 Leleākūhonua]] ({{mp|2015 TG|387}}) || 65 || 79 || [[Sednoid]] |
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|{{mpl|2015 TH|367}} || 29 ± 6 || 89 || [[Scattered disc]] |
|{{mpl|2015 TH|367}} || 29 ± 6 || 89 || [[Scattered disc]] |
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}} <!-- end of reflist --> |
}} <!-- end of reflist --> |
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{{2015 in space}} |
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<!--- THE ARTICLE IS CURRENTLY UNDERGOING A REWRITE FOR HEAVILY DISPUTED CONTENT. PLEASE SEE THE TALK PAGE. ---> |
<!--- THE ARTICLE IS CURRENTLY UNDERGOING A REWRITE FOR HEAVILY DISPUTED CONTENT. PLEASE SEE THE TALK PAGE. ---> |
Latest revision as of 00:45, 15 February 2021
This article's factual accuracy is disputed. (July 2019) |
V774104 is the internal designation for the trans-Neptunian object designated 2015 TH367, but in November 2015 press releases confused it with 541132 Leleākūhonua, which was provisionally designated 2015 TG387 and internally designated V302126.[1] as both objects were mentioned at the American Astronomical Society’s Division for Planetary Sciences meeting. Various news articles speculated that V774104 was currently 103 AU (15.4 billion km) from the Sun, but its observation arc was too short to know whether its perihelion (closest approach to the Sun) was even outside Neptune's influence.[2]
Object | Perihelion (AU) |
Heliocentric distance (AU) |
Classification |
---|---|---|---|
Neptune (for comparison) |
30 | 30 | Planet |
541132 Leleākūhonua (2015 TG387) | 65 | 79 | Sednoid |
2015 TH367 | 29 ± 6 | 89 | Scattered disc |
References
[edit]- ^ Trujillo, Chadwick; et al. (2018). A New Inner Oort Cloud Object. 50th Annual Meeting of the Division for Planetary Sciences. 21-26 October 2018. Knoxville, Tennessee. Bibcode:2018DPS....5031109T.
- ^ Witze, Alexandra (10 November 2015). "Astronomers spy most distant Solar System object ever". Nature News. doi:10.1038/nature.2015.18770.