Difference between revisions of "Mercury"

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== Geological features ==
 
== Geological features ==
In Orbiter 2016, Mercury is modeled as a sphere with no elevations, but visually, it has approximately 300 features on Mercury have been included in the stock Orbiter 2016, albedo features as well as craters, ridges, plains, escarpments, valleys, and one mountain.
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In Orbiter 2016, Mercury is modeled as a sphere with no elevations, but visually, it has a texture and approximately 300 named features on Mercury have been included in the stock Orbiter 2016, albedo features as well as craters, ridges, plains, escarpments, valleys, and one mountain.
  
See [[Geology of Mercury]].
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See [[Geology of Mercury]] for list of features.
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== Notice to pilots ==
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CAUTION! It is to be noted by pilots flying close to the ground at Mercury when approaching the North and South poles. If the vessel crosses either pole at low altitude and any great speed, errors in the simulator causes the scenario to freeze and may cause Crash to Desktop. However, if the pole is approached at very low speed, perhaps one or a few meters per second, the vessel can pass over and even land at the pole.
  
 
== Add-ons ==
 
== Add-ons ==
  
* Mariner 10 - Historically the first probe to use gravitational assists and first probe to visit Mercury. It made three fly-by's of Mercury between November 1973 and March 1974, but did not enter orbit. This probe is modeled in Orbiter in an add-on made by user "missleman01": GEP - Mariner 10 <ref>[http://www.orbithangar.com/searchid.php?ID=510 GEP Mariner 10 at Orbit Hangar]</ref>
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* Mariner 10 - Historically the first probe to use gravitational assists and first probe to visit Mercury. It made three fly-by's of Mercury between November 1973 and March 1974, but did not enter orbit. Two add-ons are available at OrbitHangar - [https://www.orbithangar.com/showAddon.php?id=52ff79a3-224f-45d3-b1c2-b3ee43ac0e74 GEP-Mariner 10 by missleman01] and [https://www.orbithangar.com/showAddon.php?id=adbe84c8-5d29-41d7-aac3-72310579cd4c GEP Mariner 10 to Orbiter 2010 by felipi1205]. It is unknown if these are compatible with Orbiter 2016.
* MESSENGER - Historically the first probe to enter orbit around Mercury. After three fly-by's between January 2008 and September 2009, it entered an highly elliptical orbit around Mercury on March 18th, 2011. This probe is modeled in Orbiter in several add-ons <ref>[https://www.orbithangar.com/showAddon.php?id=dfb4c010-d4c1-4be7-8237-28b42217229a Messenger Probe Add-on at Orbit Hangar]</ref>
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* MESSENGER - Historically the first probe to enter orbit around Mercury. After three fly-by's between January 2008 and September 2009, it entered an highly elliptical orbit around Mercury on March 18th, 2011. This probe is modeled in Orbiter in several add-ons [https://www.orbithangar.com/showAddon.php?id=dfb4c010-d4c1-4be7-8237-28b42217229a Messenger by Ëåäíåff], [https://www.orbithangar.com/showAddon.php?id=43753e2e-1acb-42a1-8cb3-74d0cc95f683 GEP-Messenger by thexfiles19], and [https://www.orbithangar.com/showAddon.php?id=531b7cf9-2a87-4c2d-9d6b-046a8eedfd1a MESSENGER MOI by nukeet]. It is unknown which versions these add-ons are compatible with.
 
* [https://www.orbithangar.com/showAddon.php?id=0f6275a0-ad1c-4e9b-a80e-a9f8823d3091 Mercury level 7 topography and level 8 textures at Orbit Hangar]
 
* [https://www.orbithangar.com/showAddon.php?id=0f6275a0-ad1c-4e9b-a80e-a9f8823d3091 Mercury level 7 topography and level 8 textures at Orbit Hangar]
 
* [https://www.orbithangar.com/showAddon.php?id=8d0f7087-971b-48d8-b84f-6ab43bfd5161 Mercury Level 8 texture at Orbit Hangar]
 
* [https://www.orbithangar.com/showAddon.php?id=8d0f7087-971b-48d8-b84f-6ab43bfd5161 Mercury Level 8 texture at Orbit Hangar]

Revision as of 11:56, 7 September 2021

Mercury
MercuryScrshot.jpg
Mercury in Orbiter
Designation
Name Mercury
Reference body Sun
Number of satellites 0
Planetary mean orbits
Epoch J2000 (1 January 2000)
Semimajor axis (a) 0.38709893 AU
5.790917567×107 km)
Eccentricity (e) 0.20563069
Inclination (i) 7.00487°
(0.122258 radian)
Longitude of the ascending node (LAN, ☊) 48.33167°
(0.8436468 radian)
Longitude of periapsis (ϖ) 77.45645°
(1.351870 radian)
Mean longitude (L) 252.25084°
(4.402608 radian)
Planetary orbital element centennial rates
Semimajor axis (a) 0.00000066 AU/Century
Eccentricity (e) 0.00002527 Century-1
Inclination (i) -23.51 seconds/Century
Longitude of the ascending node (LAN, ☊) -446.30 seconds/Century
Longitude of periapsis (ϖ) 573.57 seconds/Century
Mean longitude (L) 538101628.29 seconds/Century
Selected physical parameters
Mean radius 2440 km
Mass 3.301880×1023 kg
Density 5.427 g/cm3
Sidereal rotation period 1407.509 hours
Sidereal orbit period 0.2408445 years
Magnitude V(1,0) -0.42
Geometric albedo 0.106
Equatorial gravity 3.701 m/s2
Escape velocity 4.435 km/s
Rotation elements
North pole right ascension (α1) 280.99°
North pole declination (δ1) 61.44°
Obliqutiy of ecliptic 7.01°
Longitude of Sun's transit 228.31°
Note *Elements given are from Orbiter.pdf (2016)


Mercury is the smallest planet in the solar system and is the closest to the sun. Mercury is a rocky planet appearing much like the moon and has virtually no atmosphere (none is modeled in Orbiter), and has no natural satellites.

Mercury was visited in 1974 and 1975 by Mariner 10 in two flybys and was again visited by MESSENGER spacecraft orbiting Mercury from 2011 to 2015 when it was deorbited. There is a plan for the BepiColombo spacecraft to visit in 2025.

Orbital characteristics

Mercury is the innermost planet in the system with a semimajor axis of 5.79×107 km. But, the orbital eccentricity is the largest of all the planets, about 0.2056, its distance ranging from 46 million to almost 70 million km from the Sun, and the inclination of its orbit is just over 7°, also largest of all the planets.

Physical characteristics

Mercury's mean radius is 2440 km, smaller than Ganymede and Titan, but more massive at a bit more than 3.3×1023 kg.[1] Mercury is unique in the solar system in that it is tidally locked with the Sun in a 3:2 spin-orbit resonance; it rotates three times for each two orbits around the Sun, which means that one day on Mercury is two of its years.[1] It also has the smallest axial tilt with respect to its orbit, about 2 arcminutes.

Geological features

In Orbiter 2016, Mercury is modeled as a sphere with no elevations, but visually, it has a texture and approximately 300 named features on Mercury have been included in the stock Orbiter 2016, albedo features as well as craters, ridges, plains, escarpments, valleys, and one mountain.

See Geology of Mercury for list of features.

Notice to pilots

CAUTION! It is to be noted by pilots flying close to the ground at Mercury when approaching the North and South poles. If the vessel crosses either pole at low altitude and any great speed, errors in the simulator causes the scenario to freeze and may cause Crash to Desktop. However, if the pole is approached at very low speed, perhaps one or a few meters per second, the vessel can pass over and even land at the pole.

Add-ons

External links

References

  1. 1.0 1.1 Orbiter.pdf (2016)


edit The Solar System
Central star

Sun (Sol)

Planets

Mercury - Venus - Earth - Mars - Jupiter - Saturn - Uranus - Neptune

Natural satellites

Moon - Phobos - Deimos - Io - Europa - Ganymede - Titan - more...

Add-ons

Planets - Dwarf Planets - Small objects - Natural satellites - Alternative star systems

EarthScrshot.jpg This article, about a planet, is a stub. You can help Orbiterwiki by expanding it.