Triton Article

Triton summary

verifiedCite
While every effort has been made to follow citation style rules, there may be some discrepancies. Please refer to the appropriate style manual or other sources if you have any questions.
Select Citation Style
Share
Share to social media
URL
https://mainten.top/summary/Triton-astronomy
Feedback
Corrections? Updates? Omissions? Let us know if you have suggestions to improve this article (requires login).
Thank you for your feedback

Our editors will review what you’ve submitted and determine whether to revise the article.

External Websites
Below is the article summary. For the full article, see Triton.

Triton , Largest of Neptune’s moons. Its diameter is about 1,680 mi (2,700 km), nearly 80% that of Earth’s Moon. Unique among the large moons of the solar system, Triton moves in a retrograde orbit, opposite the direction of Neptune’s rotation. Its orbital period of 5.9 Earth days is the same as its rotation period; as a result it always keeps the same face toward Neptune. It has a very thin atmosphere of nitrogen and methane and a surface temperature of −390 °F (−235 °C). Its surface is covered with enormous expanses of ice sculpted with fissures, puckers, and ridge-crossed depressions. Geyser-like plumes observed by the Voyager 2 spacecraft may be gas venting through fissures when the surface is warmed by sunlight. Triton appears to have formed elsewhere in the solar system and to have been gravitationally captured by Neptune in the planet’s early history.