Neptune: Difference between revisions

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{{Sidebar planet
{{Sidebar planet
|Name=Neptune
| Name= Neptune
|AffiliationImage=Unaligned.jpg
| AffiliationImage= Neptune (planet).png
|Class=[[SFC:PC|J]]
| Designation= Sol IX
|Native Species=none
| Affiliation= unaligned
|World Status=Non-Resource
| Location= [[Sol]]
|Affiliation=unaligned
| Sector= [[Sol Sector]]
|Location=[[Sol]]
| Quadrant= Alpha / Beta
|Sector=[[001]]
| World Status= Non-Resource
|Quadrant=[[Alpha]]/[[Beta]]
| Distance= 30.11
| Orbit=9
| Orbital Zone= Blue
| Orbital Duration= 164.8 years (60,182 days)
| Class= [[SFC:PC|I]]
| Rotation Duration= 16.1 hrs
| Satellites= 14
| Atmospheric Density= Thick
| Gravity= 1.15
| Diameter= 3.87
| Surface Area= 14.93
| Water Area=
| Landmasses=
| Tectonic Activity=
| Volcanic Activity=
| Temperature Ranges=
| Polar Zone=
| Temperate Zone=
| Tropical Zone=
| Equatorial Zone=
| Resource Availability=
| Normal Metals=
| Special Metals=
| Radioactives=
| Gem Stones=
| Industrial Crystals=
| Population Capacity=
| Dominant Lifeform= N/A
| Global Population=
| Lifeform Sentience=
| Sentient Species=
| Tech Level=
| Society Type=
| Production Type=
}}
}}
{| class="toc" class="toc"
|'''System Layout''':<br>
[[Sol]]: '''·''' [[Mercury]] '''·''' [[Venus]] '''·''' [[Earth]]<sup>([[Luna]])</sup> '''·''' [[Mars]]<sup>([[Phobos]], [[Deimos]])</sup>'''·''' [[Sol V|Main Belt]]<sup>([[Ceres]])</sup> '''·''' [[Jupiter]]<sup>([[Europa]])</sup> '''·''' [[Saturn]]<sup>([[Titan]], [[Enceladus]])</sup> '''·''' [[Uranus]] '''·''' [[Neptune]] '''·''' [[Pluto]]
|}
==Astronomical Data==
==Astronomical Data==
===Names===
*Sol VIII
*Neptune
*Janus
*Leverrier
*Oceanus
<br>
===Satellites===
===Satellites===
====Natural====
====Natural====
*Triton
* Triton
*12 lesser moons
* 12 lesser moons
*slight ring system
* slight ring system
<br>
 
====Artificial====
====Artificial====
*none
* none
<br>
 
{{SolIntrasystem}}
<br>
==History==
==History==
Galileo's drawings show that he first observed Neptune on December 28, 1612, and again on January 27, 1613; on both occasions, Galileo mistook Neptune for a fixed star when it appeared very close (in conjunction) to Jupiter in the night sky. Believing it to be a fixed star, he is not credited with its discovery. At the time of his first observation in December 1612, it was stationary in the sky because it had just turned retrograde that very day; because it was only beginning its yearly retrograde cycle, Neptune's motion was far too slight to be detected with Galileo's small telescope.
[[Galileo]]'s drawings show that he first observed '''Neptune''' on December 28, [[1612]], and again on January 27, [[1613]]; on both occasions, Galileo mistook Neptune for a fixed star when it appeared very close (in conjunction) to [[Jupiter]] in the night sky. Believing it to be a fixed star, he is not credited with its discovery. At the time of his first observation in December 1612, it was stationary in the sky because it had just turned retrograde that very day; because it was only beginning its yearly retrograde cycle, Neptune's motion was far too slight to be detected with Galileo's small telescope.
 
In [[1821]], [[Alexis Bouvard]] published astronomical tables of the orbit of [[Uranus]]. Subsequent observations revealed substantial deviations from the tables, leading Bouvard to hypothesize some perturbing body. In [[1843]], John Couch Adams calculated the orbit of an eighth planet that would account for Uranus' motion. He sent his calculations to Sir [[George Airy]], the Astronomer Royal, who asked Adams for a clarification. Adams began to draft a reply but never sent it and did not aggressively pursue work on the Uranus problem.


In 1821, Alexis Bouvard published astronomical tables of the orbit of Uranus. Subsequent observations revealed substantial deviations from the tables, leading Bouvard to hypothesize some perturbing body. In 1843, John Couch Adams calculated the orbit of an eighth planet that would account for Uranus' motion. He sent his calculations to Sir George Airy, the Astronomer Royal, who asked Adams for a clarification. Adams began to draft a reply but never sent it and did not aggressively pursue work on the Uranus problem.
In [[1845]]-[[1846|46]], [[Urbain Le Verrier]], independently of Adams, rapidly developed his own calculations but also experienced difficulties in encouraging any enthusiasm in his compatriots. In June, however, upon seeing Le Verrier's first published estimate of the planet's longitude and its similarity to Adams's estimate, Airy persuaded Cambridge Observatory director [[James Challis]] to search for the planet.


In 1845-6, Urbain Le Verrier, independently of Adams, rapidly developed his own calculations but also experienced difficulties in encouraging any enthusiasm in his compatriots. In June, however, upon seeing Le Verrier's first published estimate of the planet's longitude and its similarity to Adams's estimate, Airy persuaded Cambridge Observatory director James Challis to search for the planet.
Challis vainly scoured the sky throughout August and September. Meantime, Le Verrier by letter urged Berlin Observatory astronomer [[Johann Gottfried Galle]] to search with the observatory's refractor. Though still a student at the Berlin Observatory, [[Heinrich d'Arrest]] suggested that a recently drawn chart of the sky, in the region of Le Verrier's predicted location, could be compared with the current sky to seek the displacement characteristic of a planet, as opposed to a fixed star. The very evening of the day of receipt of Le Verrier's letter, Neptune was discovered, September 23, [[1846]], within 1° of where Le Verrier had predicted it to be, and about 12° from Adams' prediction. Challis later realized that he had observed the planet twice in August, failing to identify it owing to his casual approach to the work.


Challis vainly scoured the sky throughout August and September. Meantime, Le Verrier by letter urged Berlin Observatory astronomer Johann Gottfried Galle to search with the observatory's refractor. Though still a student at the Berlin Observatory, Heinrich d'Arrest suggested that a recently drawn chart of the sky, in the region of Le Verrier's predicted location, could be compared with the current sky to seek the displacement characteristic of a planet, as opposed to a fixed star. The very evening of the day of receipt of Le Verrier's letter, Neptune was discovered, September 23, 1846, within 1° of where Le Verrier had predicted it to be, and about 12° from Adams' prediction. Challis later realized that he had observed the planet twice in August, failing to identify it owing to his casual approach to the work.
<br>
==Important Locations==
==Important Locations==
*None
* None
<br>
 
==Background==
==Notes==
<br>
*
[[Category:Planets|{{PAGENAME}}]][[Category:UnalignedPlanets|{{PAGENAME}}]][[Category:J Class Planets|{{PAGENAME}}]][[Category:Locations N|{{PAGENAME}}]]
 
==References==
<references/>
 
 
[[Category: Unaligned Planets]]
[[Category: I Class Planets]]
[[Category: Locations N]]

Latest revision as of 04:29, 12 July 2026

Neptune
Political Specifications
Designation Sol IX
Affiliation unaligned
Location Sol
Sector Sol Sector
Quadrant Alpha / Beta
World Status Non-Resource
Orbital Characteristics
Distance (AUs) 30.11
Orbit 9
Orbital Zone Blue
Orbital Duration 164.8 years (60,182 days)
Physical Characteristics
Class I
Rotation Duration 16.1 hrs
Satellites 14
Atmospheric Density Thick
Gravity (g) 1.15
Diameter (d) 3.87
Surface Area (a2) 14.93
Population Data
Dominant Lifeform N/A


System Layout:

Sol: · Mercury · Venus · Earth(Luna) · Mars(Phobos, Deimos)· Main Belt(Ceres) · Jupiter(Europa) · Saturn(Titan, Enceladus) · Uranus · Neptune · Pluto

Astronomical Data

Satellites

Natural

  • Triton
  • 12 lesser moons
  • slight ring system

Artificial

  • none

History

Galileo's drawings show that he first observed Neptune on December 28, 1612, and again on January 27, 1613; on both occasions, Galileo mistook Neptune for a fixed star when it appeared very close (in conjunction) to Jupiter in the night sky. Believing it to be a fixed star, he is not credited with its discovery. At the time of his first observation in December 1612, it was stationary in the sky because it had just turned retrograde that very day; because it was only beginning its yearly retrograde cycle, Neptune's motion was far too slight to be detected with Galileo's small telescope.

In 1821, Alexis Bouvard published astronomical tables of the orbit of Uranus. Subsequent observations revealed substantial deviations from the tables, leading Bouvard to hypothesize some perturbing body. In 1843, John Couch Adams calculated the orbit of an eighth planet that would account for Uranus' motion. He sent his calculations to Sir George Airy, the Astronomer Royal, who asked Adams for a clarification. Adams began to draft a reply but never sent it and did not aggressively pursue work on the Uranus problem.

In 1845-46, Urbain Le Verrier, independently of Adams, rapidly developed his own calculations but also experienced difficulties in encouraging any enthusiasm in his compatriots. In June, however, upon seeing Le Verrier's first published estimate of the planet's longitude and its similarity to Adams's estimate, Airy persuaded Cambridge Observatory director James Challis to search for the planet.

Challis vainly scoured the sky throughout August and September. Meantime, Le Verrier by letter urged Berlin Observatory astronomer Johann Gottfried Galle to search with the observatory's refractor. Though still a student at the Berlin Observatory, Heinrich d'Arrest suggested that a recently drawn chart of the sky, in the region of Le Verrier's predicted location, could be compared with the current sky to seek the displacement characteristic of a planet, as opposed to a fixed star. The very evening of the day of receipt of Le Verrier's letter, Neptune was discovered, September 23, 1846, within 1° of where Le Verrier had predicted it to be, and about 12° from Adams' prediction. Challis later realized that he had observed the planet twice in August, failing to identify it owing to his casual approach to the work.

Important Locations

  • None

Notes

References