Minor Members of the Solar System
... the Earth and one-third its volume Highly eccentric and highly inclined orbit Charon is classified as its moon Has two known smaller moons, Nix and Hydra ...
... the Earth and one-third its volume Highly eccentric and highly inclined orbit Charon is classified as its moon Has two known smaller moons, Nix and Hydra ...
Universe Now - Course Pages of Physics Department
... dynamics of the outer Solar System during 100 years (with a time step of 200 days). White: plutinos (Pluto as large, white circle) Blue squares: comets (in perihelion around year 2002) Orange: centaurs Red: Classical TNOs Magenta: scattered disc objects Cyan: higheccentricity objects Planets: Jupite ...
... dynamics of the outer Solar System during 100 years (with a time step of 200 days). White: plutinos (Pluto as large, white circle) Blue squares: comets (in perihelion around year 2002) Orange: centaurs Red: Classical TNOs Magenta: scattered disc objects Cyan: higheccentricity objects Planets: Jupite ...
The International Astronomical Union Defines
... process to name these objects. IAU Resolution: Definition of a Planet in the Solar System Contemporary observations are changing our understanding of planetary systems, and it is important that our nomenclature for objects reflect our current understanding. This applies, in particular, to the design ...
... process to name these objects. IAU Resolution: Definition of a Planet in the Solar System Contemporary observations are changing our understanding of planetary systems, and it is important that our nomenclature for objects reflect our current understanding. This applies, in particular, to the design ...
Goal: To understand what the Kuiper Belt is, and why it is
... further away (did I mention it gets VERY cold on Pluto!). • However… ...
... further away (did I mention it gets VERY cold on Pluto!). • However… ...
Orbit inclined 17º from Ecliptic, with a high eccentricity
... Discovery of Pluto Calculations indicated that Neptune’s orbit was being purturbed => another planet beyond Neptune. Found in 1930 by Clyde Tombaugh. Too small to account for the perturbations. They were later shown not to exist – no need to invoke planet beyond Neptune! ...
... Discovery of Pluto Calculations indicated that Neptune’s orbit was being purturbed => another planet beyond Neptune. Found in 1930 by Clyde Tombaugh. Too small to account for the perturbations. They were later shown not to exist – no need to invoke planet beyond Neptune! ...
My planet project
... Who needs 7% gravity on Earth when you can have 8% gravity. Pluto's orbit is inclined, or tilted, 17.1 degrees from the ecliptic -- the plane that Earth orbits in. Except for Mercury's inclination of 7 degrees, all the other planets orbit more closely to the ecliptic. Pluto’s average orbital speed i ...
... Who needs 7% gravity on Earth when you can have 8% gravity. Pluto's orbit is inclined, or tilted, 17.1 degrees from the ecliptic -- the plane that Earth orbits in. Except for Mercury's inclination of 7 degrees, all the other planets orbit more closely to the ecliptic. Pluto’s average orbital speed i ...
Unit 3
... Mercury is the second smallest planet in our solar system. Only the planet Pluto is smaller. Mercury is about the same size as the Earth’s Moon. Mercury is very close to the Sun. Mercury travels around the Sun faster than any other planet. (Note: That is how Mercury got its name. It was named af ...
... Mercury is the second smallest planet in our solar system. Only the planet Pluto is smaller. Mercury is about the same size as the Earth’s Moon. Mercury is very close to the Sun. Mercury travels around the Sun faster than any other planet. (Note: That is how Mercury got its name. It was named af ...
Pluto Planet Brochure
... coats, and electric blankets because it’s -375° to -370°c BRR! So just come on and get you’re tickets. ...
... coats, and electric blankets because it’s -375° to -370°c BRR! So just come on and get you’re tickets. ...
Pluto, the Kuiper Belt, and Trans- Neptunian Objects
... • Characteristic of objects formed in the outer solar system. • The discovery of more, similar objects beginning in early 1990’s means that Pluto is just one of the “Trans-Neptunian Objects – icy bodies orbiting beyond Neptune. The “Kuiper Belt” is a zone from 30 to 50 AU containing great majority ...
... • Characteristic of objects formed in the outer solar system. • The discovery of more, similar objects beginning in early 1990’s means that Pluto is just one of the “Trans-Neptunian Objects – icy bodies orbiting beyond Neptune. The “Kuiper Belt” is a zone from 30 to 50 AU containing great majority ...
Pluto
... • Large distance makes it very difficult to study • Mass known from the orbital period of its moon, Charon (6.4 days, discovered in 1978) • Size and surface albedo mapped from occultations with Charon ...
... • Large distance makes it very difficult to study • Mass known from the orbital period of its moon, Charon (6.4 days, discovered in 1978) • Size and surface albedo mapped from occultations with Charon ...
WhatsInSolarSystem - School
... Planets and Dwarf Planets Planets According to the International Astronomical Union a planet is an object which: 1. Is in orbit around the Sun 2. Has a mass big enough so that its gravity pulls it into a nearly round shape 3. Has "cleared the neighbourhood" around its orbit. Dwarf Planets As telesco ...
... Planets and Dwarf Planets Planets According to the International Astronomical Union a planet is an object which: 1. Is in orbit around the Sun 2. Has a mass big enough so that its gravity pulls it into a nearly round shape 3. Has "cleared the neighbourhood" around its orbit. Dwarf Planets As telesco ...
Pluto`s Bald Cousin
... means it’s not able to hold on to the few sunrays it receives at its distant location, which is even farther away from the Sun than its cousin, Pluto. Until a few years ago, Pluto was considered to be the most distant planet in our Solar System, until it was downgraded to a dwarf planet like Makemak ...
... means it’s not able to hold on to the few sunrays it receives at its distant location, which is even farther away from the Sun than its cousin, Pluto. Until a few years ago, Pluto was considered to be the most distant planet in our Solar System, until it was downgraded to a dwarf planet like Makemak ...
Pluto`s Bald Cousin
... means it’s not able to hold on to the few sunrays it receives at its distant location, which is even farther away from the Sun than its cousin, Pluto. Until a few years ago, Pluto was considered to be the most distant planet in our Solar System, until it was downgraded to a dwarf planet like Makemak ...
... means it’s not able to hold on to the few sunrays it receives at its distant location, which is even farther away from the Sun than its cousin, Pluto. Until a few years ago, Pluto was considered to be the most distant planet in our Solar System, until it was downgraded to a dwarf planet like Makemak ...
here
... This is your fourth assignment using the Starry Night software. This is due in class by Tuesday, October 21st. You may turn this in any time prior to the due date. Homework is due at the start of class. Late homework is not accepted! If you will be unable to make it to class to turn this in, you mus ...
... This is your fourth assignment using the Starry Night software. This is due in class by Tuesday, October 21st. You may turn this in any time prior to the due date. Homework is due at the start of class. Late homework is not accepted! If you will be unable to make it to class to turn this in, you mus ...
Name of Planet
... • Pluto is a brownish blackish color from near by. If possible you might see some yellow • From far away planets like Earth, it seems very orangey red like the one you see in the beginning ...
... • Pluto is a brownish blackish color from near by. If possible you might see some yellow • From far away planets like Earth, it seems very orangey red like the one you see in the beginning ...
Dwarf planets
... After Eris and Pluto, Makemake is the third largest known dwarf planet. Along with fellow dwarf planets Pluto and Haumea, Makemake is located in the Kuiper Belt. Pluto and Makemake are the two brightest objects that have so far been discovered in the Kuiper Belt. It takes 310 Earth years for thi ...
... After Eris and Pluto, Makemake is the third largest known dwarf planet. Along with fellow dwarf planets Pluto and Haumea, Makemake is located in the Kuiper Belt. Pluto and Makemake are the two brightest objects that have so far been discovered in the Kuiper Belt. It takes 310 Earth years for thi ...
The Discovery of Planet X
... Kuiper belt objects are further classified into the following groups: Resonant objects---- are locked in an orbital resonance with Neptune. Objects with a 1:2 resonance are also called twotinos, and objects with a 2:3 resonance are called plutinos, after their most prominent member, Pluto. Classical ...
... Kuiper belt objects are further classified into the following groups: Resonant objects---- are locked in an orbital resonance with Neptune. Objects with a 1:2 resonance are also called twotinos, and objects with a 2:3 resonance are called plutinos, after their most prominent member, Pluto. Classical ...
Pluto Not A Planet
... Belt “scattered disc,” orbiting the sun around Neptune. Eris, another dwarf planet was found to be bigger than Pluto in the belt. This caused some havoc because Eris had speculation of being a planet. As Pluto has the same characteristics of other dwarf planets (which are not planets under its regul ...
... Belt “scattered disc,” orbiting the sun around Neptune. Eris, another dwarf planet was found to be bigger than Pluto in the belt. This caused some havoc because Eris had speculation of being a planet. As Pluto has the same characteristics of other dwarf planets (which are not planets under its regul ...
APOM 2014 April
... (its aphelion is 97.5 AU). It came to perihelion between 1698[5] and 1699,[41] to aphelion around 1977,[41] and will return to perihelion around 2256[41] to 2258.[42] Eris and its moon are currently the most distant known objects in the Solar System apart from long-period comets and space probes.[43 ...
... (its aphelion is 97.5 AU). It came to perihelion between 1698[5] and 1699,[41] to aphelion around 1977,[41] and will return to perihelion around 2256[41] to 2258.[42] Eris and its moon are currently the most distant known objects in the Solar System apart from long-period comets and space probes.[43 ...
What`s a Planet and Why is Pluto Not in the Planet Club Anymore?
... began calling them all asteroids or minor planets. The name was appropriate because these objects were all significantly smaller than any of the regular planets. But as you can see in the table at the bottom, for a while, schoolkids had to memorize Ceres, Juno, Pallas, and Vesta as full-fledged memb ...
... began calling them all asteroids or minor planets. The name was appropriate because these objects were all significantly smaller than any of the regular planets. But as you can see in the table at the bottom, for a while, schoolkids had to memorize Ceres, Juno, Pallas, and Vesta as full-fledged memb ...
The Inner Worlds - Stockton University
... his discovery, but by the time Bode looked for it, the object was too near the direction of the Sun for observation. • In November, Gauss predicted the location of this object based on Piazzi's observations; it was found on Dec 31, 1801 • Piazzi named the object "Ceres" after the protecting goddess ...
... his discovery, but by the time Bode looked for it, the object was too near the direction of the Sun for observation. • In November, Gauss predicted the location of this object based on Piazzi's observations; it was found on Dec 31, 1801 • Piazzi named the object "Ceres" after the protecting goddess ...
Introduction
... • orbit: 39.5 AU, period 248 years • perturbations of Uranus were not produced by Pluto ...
... • orbit: 39.5 AU, period 248 years • perturbations of Uranus were not produced by Pluto ...
butoday20050915
... 2003UB313, the heavenly body is a member of the Kuiper Asteroid Belt. It’s the farthestknown object in the solar system, and bigger than Pluto, which was spotted by astronomers in 1930 and named the solar system’s ninth planet. ...
... 2003UB313, the heavenly body is a member of the Kuiper Asteroid Belt. It’s the farthestknown object in the solar system, and bigger than Pluto, which was spotted by astronomers in 1930 and named the solar system’s ninth planet. ...
Eris (dwarf planet)
Eris (minor-planet designation 136199 Eris) is the most-massive and second-largest dwarf planet known in the Solar System. It is also the ninth-most-massive known body directly orbiting the Sun, and the largest known body in the Solar System not visited by a spacecraft. It was measured to be 2,326 ± 12 kilometers (1,445.3 ± 7.5 mi) in diameter. Eris is 27% more massive than dwarf planet Pluto, though Pluto is slightly larger by volume. Eris's mass is about 0.27% of the Earth's mass.Eris was discovered in January 2005 by a Palomar Observatory–based team led by Mike Brown, and its identity was verified later that year. It is a trans-Neptunian object (TNO) and a member of a high-eccentricity population known as the scattered disk. It has one known moon, Dysnomia. As of 2014, its distance from the Sun is 96.4 astronomical units (1.442×1010 km; 8.96×109 mi), roughly three times that of Pluto. With the exception of some comets, Eris and Dysnomia are currently the most distant known natural objects in the Solar System.Because Eris appeared to be larger than Pluto, NASA initially described it as the Solar System's tenth planet. This, along with the prospect of other objects of similar size being discovered in the future, motivated the International Astronomical Union (IAU) to define the term planet for the first time. Under the IAU definition approved on August 24, 2006, Eris is a ""dwarf planet"", along with objects such as Pluto, Ceres, Haumea and Makemake, thereby reducing the number of known planets in the Solar System to eight, the same as before Pluto's discovery in 1930. Observations of a stellar occultation by Eris in 2010 showed that its diameter was 2,326 ± 12 kilometers (1,445.3 ± 7.5 mi), not significantly different from that of Pluto. After New Horizons measured Pluto's diameter as 7006237200000000000♠2372±4 km in July 2015, it was determined that Eris is slightly smaller in diameter than Pluto.