Jump to content
 







Main menu
   


Navigation  



Main page
Contents
Current events
Random article
About Wikipedia
Contact us
Donate
 




Contribute  



Help
Learn to edit
Community portal
Recent changes
Upload file
 








Search  

































Create account

Log in
 









Create account
 Log in
 




Pages for logged out editors learn more  



Contributions
Talk
 



















Contents

   



(Top)
 


1 References  














S/2018 J 2






Deutsch
Español
Bahasa Indonesia
Italiano

Коми
Latviešu
Română
Svenska
Türkçe
Українська
 

Edit links
 









Article
Talk
 

















Read
Edit
View history
 








Tools
   


Actions  



Read
Edit
View history
 




General  



What links here
Related changes
Upload file
Special pages
Permanent link
Page information
Cite this page
Get shortened URL
Download QR code
Wikidata item
 




Print/export  



Download as PDF
Printable version
 
















Appearance
   

 






From Wikipedia, the free encyclopedia
 


S/2018 J 2
Discovery[1]
Discovered byScott S. Sheppard
Discovery siteCerro Tololo Obs.
Discovery date12 May 2018
Orbital characteristics[1][2]
Epoch 9 August 2022 (JD 2459800.5)
Observation arc19.48 yr (7,115 d)
Earliest precovery date27 March 2003

Semi-major axis

0.0766555 AU (11,467,500 km)
Eccentricity0.1184102

Orbital period (sidereal)

+250.88 days

Mean anomaly

99.239°

Mean motion

1° 26m 5.896s / day
Inclination29.40421° (toecliptic)

Longitude of ascending node

66.06734°

Argument of perihelion

342.09685°
Satellite ofJupiter
GroupHimalia group
Physical characteristics

Mean diameter

km[3]
Albedo0.04 (assumed)[3]

Apparent magnitude

23.3[3]

Absolute magnitude (H)

16.5[1]

S/2018 J 2 is a small outer natural satelliteofJupiter discovered by Scott S. Sheppard on 12 May 2018, using the 4.0-meter Víctor M. Blanco TelescopeatCerro Tololo Observatory, Chile. It was announced by the Minor Planet Center four years later on 20 December 2022, after observations were collected over a long enough time span to confirm the satellite's orbit. The satellite has been found in precovery observations as early as 27 March 2003.[1]

S/2018 J 2 is part of the Himalia group, a tight cluster of prograde irregular moons of Jupiter that follow similar orbits to Himaliaatsemi-major axes between 11–12 million km (6.8–7.5 million mi) and inclinations between 26–31°.[3] With an estimated diameter of 3 km (1.9 mi) for an absolute magnitude of 16.5, it is among the smallest known members of the Himalia group.[3]

References[edit]

  1. ^ a b c d "MPEC 2022-Y68 : S/2018 J 2". Minor Planet Electronic Circulars. Minor Planet Center. 20 December 2022. Retrieved 20 December 2022.
  • ^ "Planetary Satellite Discovery Circumstances". JPL Solar System Dynamics. NASA. Retrieved 20 December 2022.
  • ^ a b c d e Sheppard, Scott S. "Moons of Jupiter". Earth & Planets Laboratory. Carnegie Institution for Science. Retrieved 20 December 2022.

  • t
  • e

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=S/2018_J_2&oldid=1167966727"

    Categories: 
    Himalia group
    Moons of Jupiter
    Irregular satellites
    Astronomical objects discovered in 2018
    Discoveries by Scott S. Sheppard
    Moons with a prograde orbit
    Planetary science stubs
    Hidden categories: 
    Articles with short description
    Short description is different from Wikidata
    Use dmy dates from January 2023
    All stub articles
     



    This page was last edited on 30 July 2023, at 23:39 (UTC).

    Text is available under the Creative Commons Attribution-ShareAlike License 4.0; additional terms may apply. By using this site, you agree to the Terms of Use and Privacy Policy. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc., a non-profit organization.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Mobile view



    Wikimedia Foundation
    Powered by MediaWiki