Triton (moon)

Triton is the largest natural satellite of the planet Neptune , and the first Neptunian moon to be discovered. The discovery was made on October 10, 1846, by English astronomer William Lassell . It is the only large moon in the Solar System with a retrograde orbit , an orbit in the direction opposite to its planet's rotation. [2] [11] At 2,710 kilometres (1,680 mi) [5] in diameter, it is the seventh-largest moon in the Solar System. Because of its retrograde orbit and composition similar to Pluto 's, Triton is thought to have been a dwarf planet captured from the Kuiper belt . [12] It has a surface of mostly frozen nitrogen , a mostly water-ice crust, [13] an icy mantle and a substantial core of rock and metal. The core makes up two-thirds of its total mass. The mean density is 2.061 g/cm 3, [5] reflecting a composition of approximately 15–35% water ice. [6]

Page Revisions

Year Metadata Sections Top Words First Paragraph
2018

255072 characters

16 sections

42 paragraphs

28 images

408 internal links

156 external links

1. Discovery and naming

2. Orbit and rotation

3. Capture

4. Physical characteristics

5. Atmosphere

6. Surface features

7. Observation and exploration

8. Maps

9. See also

10. Notes

11. References

12. External links

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1989 0.044

Triton is the largest natural satellite of the planet Neptune , and the first Neptunian moon to be discovered. The discovery was made on October 10, 1846, by English astronomer William Lassell . It is the only large moon in the Solar System with a retrograde orbit , an orbit in the direction opposite to its planet's rotation. [2] [11] At 2,710 kilometres (1,680 mi) [5] in diameter, it is the seventh-largest moon in the Solar System. Because of its retrograde orbit and composition similar to Pluto 's, Triton is thought to have been a dwarf planet captured from the Kuiper belt . [12] It has a surface of mostly frozen nitrogen , a mostly water-ice crust, [13] an icy mantle and a substantial core of rock and metal. The core makes up two-thirds of its total mass. The mean density is 2.061 g/cm 3, [5] reflecting a composition of approximately 15–35% water ice. [6]

2017

253448 characters

16 sections

42 paragraphs

28 images

405 internal links

155 external links

1. Discovery and naming

2. Orbit and rotation

3. Capture

4. Physical characteristics

5. Atmosphere

6. Surface features

7. Observation and exploration

8. Maps

9. See also

10. Notes

11. References

12. External links

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pluto 0.048

cantaloupe 0.044

maculae 0.044

1989 0.044

Triton is the largest natural satellite of the planet Neptune , and the first Neptunian moon to be discovered. It was discovered on October 10, 1846, by English astronomer William Lassell . It is the only large moon in the Solar System with a retrograde orbit , an orbit in the opposite direction to its planet's rotation. [2] [11] At 2,710 kilometres (1,680 mi) [5] in diameter, it is the seventh-largest moon in the Solar System. Because of its retrograde orbit and composition similar to Pluto 's, Triton is thought to have been a dwarf planet captured from the Kuiper belt . [12] Triton has a surface of mostly frozen nitrogen , a mostly water-ice crust, [13] an icy mantle and a substantial core of rock and metal. The core makes up two-thirds of its total mass. Triton has a mean density of 2.061 g/cm 3 [5] and is composed of approximately 15–35% water ice. [6]

2016

238012 characters

16 sections

40 paragraphs

26 images

400 internal links

146 external links

1. Discovery and naming

2. Orbit and rotation

3. Capture

4. Physical characteristics

5. Atmosphere

6. Surface features

7. Observation and exploration

8. Maps

9. See also

10. Notes

11. References

12. External links

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sulci 0.039

observed 0.038

Triton is the largest natural satellite of the planet Neptune . It was discovered on October 10, 1846, by English astronomer William Lassell . It is the only large moon in the Solar System with a retrograde orbit , an orbit in the opposite direction to its planet's rotation. [2] [11] At 2,700 kilometres (1,700 mi) in diameter, it is the seventh-largest moon in the Solar System. Because of its retrograde orbit and composition similar to Pluto 's, Triton is thought to have been a dwarf planet captured from the Kuiper belt . [12] Triton has a surface of mostly frozen nitrogen , a mostly water-ice crust, [13] an icy mantle and a substantial core of rock and metal. The core makes up two-thirds of its total mass. Triton has a mean density of 2.061 g/cm 3 [5] and is composed of approximately 15–35% water ice. [6]

2015

237407 characters

16 sections

40 paragraphs

26 images

398 internal links

147 external links

1. Discovery and naming

2. Orbit and rotation

3. Capture

4. Physical characteristics

5. Atmosphere

6. Surface features

7. Observation and exploration

8. Maps

9. See also

10. Notes

11. References

12. External links

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ice 0.037

Triton is the largest natural satellite of the planet Neptune . It was discovered on October 10, 1846, by English astronomer William Lassell . It is the only large moon in the Solar System with a retrograde orbit , an orbit in the opposite direction to its planet's rotation. [2] [11] At 2,700 kilometres (1,700 mi) in diameter, it is the seventh-largest moon in the Solar System. Because of its retrograde orbit and composition similar to Pluto 's, Triton is thought to have been a dwarf planet captured from the Kuiper belt . [12] Triton has a surface of mostly frozen nitrogen , a mostly water-ice crust, [13] an icy mantle and a substantial core of rock and metal. [6] The core makes up two-thirds of its total mass. Triton has a mean density of 2.061 grams per cubic centimetre (0.0745 lb/cu in) [5] and is composed of approximately 15–35% water ice. [6]

2014

200691 characters

16 sections

39 paragraphs

25 images

285 internal links

113 external links

1. Discovery and naming

2. Orbit and rotation

3. Capture

4. Physical characteristics

5. Atmosphere

6. Surface features

7. Observation and exploration

8. Maps

9. See also

10. Notes

11. References

12. External links

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cantaloupe 0.047

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Triton is the largest moon of the planet Neptune , discovered on October 10, 1846, by English astronomer William Lassell . It is the only large moon in the Solar System with a retrograde orbit , which is an orbit in the opposite direction to its planet's rotation. [2] [11] At 2,700 kilometres (1,700 mi) in diameter, it is the seventh-largest moon in the Solar System. Because of its retrograde orbit and composition similar to Pluto 's, Triton is thought to have been captured from the Kuiper belt . [12] Triton has a surface of mostly frozen nitrogen , a mostly water ice crust, [13] an icy mantle and a substantial core of rock and metal. [6] The core makes up two-thirds of its total mass. Triton has a mean density of 2.061 grams per cubic centimetre (0.0745 lb/cu in) [5] and is composed of approximately 15–35% water ice. [6]

2013

200555 characters

15 sections

39 paragraphs

22 images

281 internal links

123 external links

1. Discovery and naming

2. Orbit and rotation

3. Capture

4. Physical characteristics

5. Atmosphere

6. Surface features

7. Observation and exploration

8. See also

9. Notes

10. References

11. External links

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cantaloupe 0.049

maculae 0.049

surface 0.048

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Triton is the largest moon of the planet Neptune , discovered on October 10, 1846, by English astronomer William Lassell . It is the only large moon in the Solar System with a retrograde orbit , which is an orbit in the opposite direction to its planet's rotation. At 2,700 kilometres (1,700 mi) in diameter, it is the seventh-largest moon in the Solar System. Because of its retrograde orbit and composition similar to Pluto 's, Triton is thought to have been captured from the Kuiper belt . [10] Triton has a surface of mostly frozen nitrogen , a mostly water ice crust, [11] an icy mantle and a substantial core of rock and metal. [5] The core makes up two-thirds of its total mass. Triton has a mean density of 2.061 grams per cubic centimetre (0.0745 lb/cu in) [4] and is composed of approximately 15–35% water ice. [5]

2012

200417 characters

15 sections

39 paragraphs

24 images

278 internal links

123 external links

1. Discovery and naming

2. Orbit and rotation

3. Capture

4. Physical characteristics

5. Atmosphere

6. Surface features

7. Observation and exploration

8. See also

9. Notes

10. References

11. External links

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orbit 0.057

moons 0.056

retrograde 0.056

cantaloupe 0.049

maculae 0.049

surface 0.048

sulci 0.042

temperature 0.041

Triton is the largest moon of the planet Neptune , discovered on October 10, 1846, by English astronomer William Lassell . It is the only large moon in the Solar System with a retrograde orbit , which is an orbit in the opposite direction to its planet's rotation. At 2,700 km in diameter, it is the seventh-largest moon in the Solar System. Because of its retrograde orbit and composition similar to Pluto 's, Triton is thought to have been captured from the Kuiper belt . [10] Triton has a surface of mostly frozen nitrogen , a mostly water ice crust, [11] an icy mantle and a substantial core of rock and metal. [5] The core makes up two-thirds of its total mass. Triton has a mean density of 2.061 grams per cubic centimetre (0.0745 lb/cu in) [4] and is composed of approximately 15–35% water ice. [5]

2011

199262 characters

15 sections

39 paragraphs

22 images

279 internal links

120 external links

1. Discovery and naming

2. Orbit and rotation

3. Capture

4. Physical characteristics

5. Atmosphere

6. Surface features

7. Observation and exploration

8. See also

9. Notes

10. References

11. External links

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Triton is the largest moon of the planet Neptune , discovered on October 10, 1846, by English astronomer William Lassell . It is the only large moon in the Solar System with a retrograde orbit , which is an orbit in the opposite direction to its planet's rotation. At 2,700 km in diameter, it is the seventh-largest moon in the Solar System. Because of its retrograde orbit and composition similar to Pluto 's, Triton is thought to have been captured from the Kuiper belt . [10] Triton has a surface of mostly frozen nitrogen , a mostly water ice crust, [11] an icy mantle and a substantial core of rock and metal. [5] The core makes up two-thirds of its total mass. Triton has a mean density of 2.061 grams per cubic centimetre (0.0745 lb/cu in) [4] and is composed of approximately 15–35% water ice. [5]

2010

176283 characters

15 sections

37 paragraphs

22 images

266 internal links

86 external links

1. Discovery and naming

2. Orbit and rotation

3. Capture

4. Physical characteristics

5. Atmosphere

6. Surface features

7. Observation and exploration

8. See also

9. Notes

10. References

11. External links

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Triton is the largest moon of the planet Neptune , discovered on October 10, 1846, by William Lassell . It is the only large moon in the Solar System with a retrograde orbit , which is an orbit in the opposite direction to its planet's rotation. [9] At 2700 km in diameter, it is the seventh-largest moon in the Solar System. Because of its retrograde orbit and composition similar to Pluto 's, Triton is thought to have been captured from the Kuiper belt . [10] Triton consists of a crust of frozen nitrogen over an icy mantle believed to cover a substantial core of rock and metal. [4] The core makes up two-thirds of its total mass. Triton has a mean density of 2.061 g/cm 3 [3] and is composed of approximately 15–35% water ice. [4]

2009

171664 characters

15 sections

36 paragraphs

21 images

266 internal links

73 external links

1. Discovery and naming

2. Observation

3. Orbit and rotation

4. Capture

5. Physical characteristics

6. Atmosphere

7. Surface features

8. See also

9. Notes

10. References

11. External links

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Triton is the largest moon of the planet Neptune , discovered on October 10, 1846 by William Lassell . It is the only large moon in the Solar System with a retrograde orbit , which is an orbit in the opposite direction to its planet's rotation. At 2700 km in diameter, it is the seventh-largest moon in the Solar System. Because of its retrograde orbit (unique in the Solar System for an object of its size) [9] and composition similar to Pluto 's, Triton is thought to have been captured from the Kuiper belt . [10] Triton consists of a crust of frozen nitrogen over an icy mantle believed to cover a substantial core of rock and metal. [4] The core makes up two-thirds of its total mass. Triton has a mean density of 2.061 g/cm 3 [3] and is composed of approximately 15–35% water ice. [4]

2008

164313 characters

15 sections

36 paragraphs

21 images

255 internal links

68 external links

1. Discovery and naming

2. Orbit and rotation

3. Capture

4. Physical characteristics

5. Atmosphere

6. Surface features

7. Observation

8. See also

9. Notes

10. References

11. External links

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Triton ( Template:PronEng TRYE -tən , or as in Greek Τρίτων) [9] is the largest moon of the planet Neptune , discovered on October 10, 1846 by William Lassell . It is the only large moon in the Solar System with a retrograde orbit , which is an orbit in the opposite direction to its planet's rotation. At 2700 km in diameter, it is the seventh-largest moon in the Solar System. Triton comprises more than 99.5% of all the mass known to orbit Neptune, including the planet's rings and twelve other known moons. It is also more massive than all the Solar System's 159 known smaller moons combined. [f] [g]

2007

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12 sections

31 paragraphs

13 images

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22 external links

1. Name

2. Orbit

3. Capture

4. Physical characteristics

5. Planetary geology

6. History of observation and exploration

7. See also

8. References

9. External links

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Triton ( Template:PronEng trye'-tən, or as Greek Τρίτων), or Neptune I is the largest moon of the planet Neptune and the only large moon in the solar system known to have a retrograde orbit . At 2700 km diameter, it is the seventh largest moon in the Solar System . With bulk characteristics similar to dwarf planet Pluto , Triton is thought to be a captured Kuiper Belt object; it has the coldest known surface in the Solar System. [3]

2006

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10 sections

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11 images

294 internal links

14 external links

1. Name

2. Orbit

3. Physical characteristics

4. Planetary geology

5. History of observation and exploration

6. Potential for life

7. See also

8. References

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Triton (trye'-tən, IPA:  [ˈtraɪtn̩] , Greek Τρίτων), or Neptune I , is the planet Neptune 's largest moon . Triton has a complex geological history and it is believed to have a relatively young surface. It was discovered by British astronomer William Lassell on October 10 1846 , just 17 days after the planet itself was discovered by German astronomer Johann Gottfried Galle . It is also believed to be a captured Kuiper Belt object.

2005

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11 sections

35 paragraphs

10 images

247 internal links

10 external links

1. Name

2. Orbit

3. Physical characteristics

4. Seasons

5. Planetary geology

6. History of observation and exploration

7. Potential for life

8. See also

9. External links

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Triton ( trye'-tən , Greek Τρίτων ), also designated Neptune I , is the planet Neptune 's largest moon . Triton is one of the coldest bodies in the solar system and has a complex geological history with a relatively young surface. It was discovered by William Lassell on October 10, 1846, just 17 days after the planet itself was discovered. Lassell believed that he had also seen a ring around Neptune. Although the existence of Neptunian rings was later indeed established, Lassell's observation must have been spurious, as they are too faint to have been detected with his instruments.

2004

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7 external links

1. Name

2. Orbit

3. Seasons

4. Physical Characteristics

5. Potential for life

6. See also

7. External links

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Triton ("TRY ton") is the planet Neptune 's largest moon , discovered by William Lassell in 1846 just 17 days after the planet itself was discovered (Lassell incorrectly believed that he had also seen a ring around Neptune).

2003

10016 characters

0 sections

8 paragraphs

3 images

53 internal links

0 external links

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pluto 0.109

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Triton is the planet Neptune 's largest moon , discovered by William Lassell in 1846 just 17 days after the planet itself was discovered. It is named after Triton , from Greek mythology .

2002

6391 characters

0 sections

5 paragraphs

1 images

34 internal links

0 external links

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pluto 0.122

orbit 0.110

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heating 0.092

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ananke 0.076

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The planet Neptune 's largest moon , discovered by William Lassell in 1846 just 17 days after the planet itself was discovered. It is named after Triton , from Greek mythology .

2001

5637 characters

0 sections

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0 images

30 internal links

0 external links

triton 0.759

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pluto 0.127

orbit 0.114

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heating 0.096

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The planet Neptune 's largest moon , discovered by William Lassell in 1846 just 17 days after the planet itself was discovered.