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Neptune

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Neptune
Neptune imaged by Voyager 2 in August 1989. Colour and contrast have been enhanced to show atmospheric detail. NASA/JPL
Object type:
Ice giant
Planetary system:
Mass:
≈ 1.02409 × 1026 kg (17.15 Earth masses)[1]
Radius:
24,622 km (volumetric mean); 24,764 km (equatorial, 1-bar level)[1]
Age:
About 4.5 billion years[2]
Mean density:
≈ 1,638 kg/m³[1]
Surface gravity:
≈ 11.27 m/s² (mean gravity at the 1-bar level)[1]
Temperature:
≈ 72 K (−201 °C) at 1 bar; ≈ 55 K (−218 °C) at 0.1 bar[1]
Atmosphere:
Mainly hydrogen and helium; methane about 1–2% by volume[1]
Primary:
Orbital epoch:
J2000.0; J2000 ecliptic and equinox[1]
Semi-major axis:
30.06896348 AU (about 4.50 billion km)[1]
Eccentricity:
0.00858587 (J2000 mean element)[1]
Orbital inclination:
1.76917° to the J2000 ecliptic[1]
Orbital period:
≈ 60,189 Earth days (164.79 years)[1]
Rotation period:
≈ 16.11 hours (from Voyager 2 magnetic and radio measurements)[1]
Axial tilt:
≈ 28.32° from the normal to the orbital plane[1]
Natural satellites:
16 known in NASA's October 2026 summary; the largest is Triton[3]
Rings:
Five principal rings and dusty structures[4]
Discovery date:
23 September 1846[5]
Discoverer:
Johann Galle and Heinrich d'Arrest, observing from Urbain Le Verrier's prediction[6]
Related portals

Neptune is the eighth and most distant planet from the Sun. Together with Uranus, it belongs to the ice giants. Hot, dense layers lie beneath its cold atmosphere, while the cloud decks carry the fastest winds of any planet in the Solar System. Neptune was the first planet whose position was predicted mathematically before its official discovery.[2][5]

Size and physical characteristics

Neptune has a mean diameter of approximately 49,244 km, almost four times Earth's diameter. Its volume is about 58 times that of Earth, while its mass is 17 times greater. Neptune is slightly smaller than Uranus but substantially more massive.[1][7]

The planet's mean density is 1.64 g/cm³, the highest among the four giant planets. Its equatorial diameter is approximately 49,528 km, compared with a polar diameter of 48,682 km; rotation makes Neptune slightly flattened.[7][1]

Orbit, rotation and seasons

Neptune completes one orbit around the Sun in approximately 165 Earth years. Its orbit is close to circular, with a mean distance of about 4.5 billion km, 30 times the Earth–Sun distance. The mean orbital speed is 5.45 km/s, so the planet travels about 330 kilometres each minute.[1]

One rotation takes about 16 hours. The axis is tilted by approximately 28°, producing seasons. Because the orbital period is so long, each season lasts roughly 40 years.[2]

In 2011, Neptune completed its first full orbit around the Sun since its discovery in 1846.[8]

Atmosphere and colour

Hydrogen and helium are the main atmospheric gases. Methane absorbs red wavelengths of sunlight and contributes to the blue-green colour. Atmospheric haze and clouds also affect the visible shade.[9]

Neptune's deep blue colour in many familiar images was intensified during processing to reveal clouds. Its natural colour is much closer to that of Uranus: both planets are pale blue-green, although Neptune is somewhat bluer.[10]

Winds and cloud systems

Wind speeds on Neptune can exceed 2,000 km/h, or more than 550 metres per second. These flows carry clouds of methane ice and form a complex circulation system despite the weak sunlight.[2]

High clouds appear especially bright in Webb infrared images. Methane absorbs much of the infrared light, leaving the main disk comparatively dark while clouds above the absorbing layer stand out. In 2022, Webb obtained detailed images of these structures together with Neptune's rings.[11]

Dark atmospheric vortices

In 1989, Voyager 2 discovered a large dark vortex known as the Great Dark Spot. It disappeared within several years, while later observations revealed other similar formations. Neptune's dark spots can appear, move and break apart over comparatively short periods.[12]

One vortex discovered by Hubble in 2018 initially drifted toward the equator, but unexpectedly reversed direction by August 2020 and moved northward again. It was about 7,400 km across. A smaller spot appeared nearby for a time and may have been a fragment shed from the larger storm.[13]

In 2023, a Neptune dark spot was studied in detail from Earth for the first time using the Very Large Telescope. The darkening probably resulted from changes in particles below the main haze layer rather than from a simple opening in the clouds.[12]

Internal structure and heat

A substantial fraction of Neptune's mass consists of material heavier than hydrogen and helium, including compounds of water, ammonia and methane together with rocky material. Under extreme pressure and temperature, their properties differ greatly from familiar terrestrial substances. The planet has no solid surface like Earth's.[2]

Neptune receives about 900 times less solar radiation than Earth, yet emits considerable internal heat. It radiates more than twice as much thermal energy as it absorbs from the Sun. The additional energy originates in its interior.[14][15]

Magnetic field and auroras

Neptune's magnetic axis is tilted about 47° relative to its rotation axis. This orientation affects the distribution of charged particles and the locations where auroras occur.[16]

Results published in 2025 from Webb observations made in June 2023 provided the first secure infrared detection of Neptune's auroras. The spectrum contained H3+ ions formed in the upper atmosphere. Bright regions appeared at middle latitudes, far from the geographic poles, because of the unusual geometry of the magnetic field.[16]

Rings

Neptune has five principal rings—Galle, Le Verrier, Lassell, Arago and Adams—together with fainter dusty structures. They are far dimmer than Saturn's rings. The Adams ring lies approximately 63,000 km from the planet's centre.[4]

The Adams ring contains arcs, sections with a higher concentration of material. Particles are therefore distributed unevenly around the ring. The existence and evolution of the arcs are connected with gravitational interactions between the rings and moons.[4][2]

Webb images published in 2022 showed narrow rings and faint dust bands with a level of detail not achieved since the Voyager 2 flyby.[11]

Moons

NASA's October 2026 summary lists 16 known moons of Neptune. The largest, Triton, was discovered by William Lassell on 10 October 1846, only 17 days after Neptune itself was found.[3][5]

Triton follows a retrograde orbit, moving opposite to Neptune's rotation. It is the largest moon in the Solar System with this type of motion. Its orbit and physical properties indicate that it probably formed as an independent body and was later captured by Neptune.[17]

During the 1989 flyby, Voyager 2 discovered active plumes on Triton and an exceptionally cold surface at about −235 °C. The moon is surrounded by a thin nitrogen atmosphere.[17]

Discovery and exploration

In the nineteenth century, Uranus's observed motion did not fully agree with calculations. Urbain Le Verrier in France and John Couch Adams in Britain independently investigated where another planet capable of perturbing its orbit might lie.[5]

On 23 September 1846, Johann Galle and Heinrich d'Arrest discovered Neptune at the Berlin Observatory using Le Verrier's prediction. The planet lay less than one degree from the calculated position, a celebrated confirmation of the predictive power of celestial mechanics.[5][6]

Voyager 2 became the first spacecraft to explore Neptune at close range on 25 August 1989. It returned images of clouds, rings and moons, measured the magnetic field and then passed close to Triton.[18]

As of November 2026, Voyager 2 remains the only spacecraft to have visited Neptune. Hubble, Webb and ground-based telescopes continue to reveal atmospheric changes, the structure of the rings and the planet's magnetic environment.[19][16]

See also

References

  1. ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 1.11 1.12 1.13 1.14 1.15 Neptune Fact Sheet // NASA, National Space Science Data Center.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 2.5 Neptune Facts // NASA Science.
  3. ↑ 3.0 3.1 Neptune Moons // NASA Science.
  4. ↑ 4.0 4.1 4.2 Neptunian Rings Fact Sheet // NASA, National Space Science Data Center.
  5. ↑ 5.0 5.1 5.2 5.3 5.4 175 Years Ago: Astronomers Discover Neptune, the Eighth Planet // NASA. 23 September 2021.
  6. ↑ 6.0 6.1 Neptune // NASA Goddard Space Flight Center.
  7. ↑ 7.0 7.1 Planetary Fact Sheet — Metric // NASA, National Space Science Data Center.
  8. ↑ Neptune's Anniversary Portraits // NASA Science. 2011.
  9. ↑ Scientists explain why Uranus and Neptune are different colours // University of Oxford. 31 May 2022.
  10. ↑ New images reveal what Neptune and Uranus really look like // University of Oxford. 5 January 2024.
  11. ↑ 11.0 11.1 New Webb Image Captures Clearest View of Neptune's Rings in Decades // NASA Science. 21 September 2022.
  12. ↑ 12.0 12.1 Mysterious Neptune dark spot detected from Earth for the first time // European Southern Observatory. 24 August 2023.
  13. ↑ Dark Storm on Neptune Reverses Direction, Possibly Shedding a Fragment // NASA Science. 15 December 2020.
  14. ↑ Neptune // NASA Goddard Space Flight Center.
  15. ↑ NASA, Oxford Discover Warmer Uranus Than Once Thought // NASA Science. 2025.
  16. ↑ 16.0 16.1 16.2 NASA's Webb Captures Neptune's Auroras For First Time // NASA Science. 26 March 2025.
  17. ↑ 17.0 17.1 Triton // NASA Science.
  18. ↑ 30 Years Ago: Voyager 2's Historic Neptune Flyby // NASA. 22 August 2019.
  19. ↑ Neptune Exploration // NASA Science.