m16a01
... 4 small satellites with orbits shown half size to fit on screen (and they are not circular). There are 4 more small satellites at about double this distance Viewed from the side, the 4+4 inner satellites all share the same plane. The outer 4+4 satellites are less than 200km diameter and have highly ...
... 4 small satellites with orbits shown half size to fit on screen (and they are not circular). There are 4 more small satellites at about double this distance Viewed from the side, the 4+4 inner satellites all share the same plane. The outer 4+4 satellites are less than 200km diameter and have highly ...
The Blurring Distinction between Asteroids and Comets
... are known with semi-major axes among the Jovian planets, though there are probably tens of thousands of them yet to be discovered. Because Chiron was the first discovered of this group, astronomers use it to define the centaurs, a class of small solar system bodies that orbit the sun between the orb ...
... are known with semi-major axes among the Jovian planets, though there are probably tens of thousands of them yet to be discovered. Because Chiron was the first discovered of this group, astronomers use it to define the centaurs, a class of small solar system bodies that orbit the sun between the orb ...
JWST Study of Planetary Systems and Solar System Objects
... capabilities will enable astronomers to use JWST to achieve the science goals described below. KBOs exhibit distinct dynamical classes, which can be generally sorted into four categories. Pluto is the archetype for "resonant" Kuiper Belt objects. It is locked into a 3:2 orbital resonance with Neptun ...
... capabilities will enable astronomers to use JWST to achieve the science goals described below. KBOs exhibit distinct dynamical classes, which can be generally sorted into four categories. Pluto is the archetype for "resonant" Kuiper Belt objects. It is locked into a 3:2 orbital resonance with Neptun ...
Jupiter Jupiter is the largest planet in the solar system. Its diameter is
... Mass and density Jupiter is heavier than any other planet. Its mass (quantity of matter) is 318 times larger than that of Earth. Although Jupiter has a large mass, it has a relatively low density. Its density averages 1.33 grams per cubic centimeter, slightly more than the density of water. The dens ...
... Mass and density Jupiter is heavier than any other planet. Its mass (quantity of matter) is 318 times larger than that of Earth. Although Jupiter has a large mass, it has a relatively low density. Its density averages 1.33 grams per cubic centimeter, slightly more than the density of water. The dens ...
Uranus
... • “Discovered” by William Herschel in 1781 (discovered by chance) – Herschel was an English musician and amateur astronomer – He used a 6.5” homemade reflector (it took him over 200 attempts to make it!) – Prior to its discovery, Uranus had been seen, but not recognized as a planet (it had been des ...
... • “Discovered” by William Herschel in 1781 (discovered by chance) – Herschel was an English musician and amateur astronomer – He used a 6.5” homemade reflector (it took him over 200 attempts to make it!) – Prior to its discovery, Uranus had been seen, but not recognized as a planet (it had been des ...
The Cosmic Perspective Asteroids, Comets, and Dwarf Planets
... a planet. b) The asteroids were too far apart to run into each other frequently enough to form a planet. c) A planet formed early in the solar system and was broken apart by a giant impact. d) Orbital resonances with Jupiter disrupted the orbits of the asteroids and prevented them from forming a ...
... a planet. b) The asteroids were too far apart to run into each other frequently enough to form a planet. c) A planet formed early in the solar system and was broken apart by a giant impact. d) Orbital resonances with Jupiter disrupted the orbits of the asteroids and prevented them from forming a ...
Lecture22-ASTA01 - University of Toronto
... rotates backwards (backwards and forwards and sideways) while it appears to “roll” along or across its orbit. ...
... rotates backwards (backwards and forwards and sideways) while it appears to “roll” along or across its orbit. ...
The Effect of a Planet in the Asteroid Belt on the Orbital Stability of
... minor perturbations. Indeed, simply displacing one (of over 100) embryo along its orbit by one meter can make the difference between forming three terrestrial planets or five (Chambers et al. 2002, in preparation). Even though most simulations are designed to produce configurations similar to those ...
... minor perturbations. Indeed, simply displacing one (of over 100) embryo along its orbit by one meter can make the difference between forming three terrestrial planets or five (Chambers et al. 2002, in preparation). Even though most simulations are designed to produce configurations similar to those ...
1 THE SMALL SATELLITES OF THE SOLAR SYSTEM: A WHITE
... satellites. The required observations include visible and IR spectroscopy to determine their composition, and imaging to determine size, crater frequency, and geologic history. Another important area is the dynamical interaction between the small inner satellites, Saturn’s rings, and the major satel ...
... satellites. The required observations include visible and IR spectroscopy to determine their composition, and imaging to determine size, crater frequency, and geologic history. Another important area is the dynamical interaction between the small inner satellites, Saturn’s rings, and the major satel ...
PLANETS
... Earth's eccentricity is 0.017, while Jupiter's is 0.094. In our solar system, the planet with the largest eccentricity is Pluto at 0.244, and Mercury with 0.205. The planet with the lowest eccentricity is Venus with 0.007. Unless there is some gravitational tugging (such as with the Galilean Satelli ...
... Earth's eccentricity is 0.017, while Jupiter's is 0.094. In our solar system, the planet with the largest eccentricity is Pluto at 0.244, and Mercury with 0.205. The planet with the lowest eccentricity is Venus with 0.007. Unless there is some gravitational tugging (such as with the Galilean Satelli ...
Document
... – Due Thursday, April 29, because of possible TAA strike • Put in box outside 6522 Sterling ...
... – Due Thursday, April 29, because of possible TAA strike • Put in box outside 6522 Sterling ...
Jovian Rings
... – Due Thursday, April 29, because of possible TAA strike • Put in box outside 6522 Sterling ...
... – Due Thursday, April 29, because of possible TAA strike • Put in box outside 6522 Sterling ...
Sorting the Solar System - Indianapolis Public Schools
... Earth, planet Earth is one of the four terrestrial (rocky) planets of the inner solar system (along with Mercury, Venus, and Mars). It has a thick atmosphere and is the only planet currently known to have life. Enceladus, satellite of Saturn Liquid water lies beneath the icy surface of Enceladus an ...
... Earth, planet Earth is one of the four terrestrial (rocky) planets of the inner solar system (along with Mercury, Venus, and Mars). It has a thick atmosphere and is the only planet currently known to have life. Enceladus, satellite of Saturn Liquid water lies beneath the icy surface of Enceladus an ...
Saturn - UpWardBoundGeneralScience
... Saturn Was The Roman Name for the Greek Cronos, god of farming, and the father of Zeus/Jupiter. Saturn is Also Considered the God of Agriculture. ...
... Saturn Was The Roman Name for the Greek Cronos, god of farming, and the father of Zeus/Jupiter. Saturn is Also Considered the God of Agriculture. ...
Our Solar System
... Jupiter's largest moon and the largest moon in the Solar System. It had plate tectonics like Earth. There are older, darker regions and newer areas with grooves where the plates have moved. Newer craters have bright rays around them from material thrown up by impacts. Older craters look flat and fad ...
... Jupiter's largest moon and the largest moon in the Solar System. It had plate tectonics like Earth. There are older, darker regions and newer areas with grooves where the plates have moved. Newer craters have bright rays around them from material thrown up by impacts. Older craters look flat and fad ...
e - DTM
... • The number of TNOs migrating to the inner regions of the Solar System can be evaluated on the basis of simple formulas and the results of numerical integration. Let NJ=PNpJNNTNO be the number of former TNOs with d>D reaching Jupiter's orbit for the given time span TSS, where NTNO is the number o ...
... • The number of TNOs migrating to the inner regions of the Solar System can be evaluated on the basis of simple formulas and the results of numerical integration. Let NJ=PNpJNNTNO be the number of former TNOs with d>D reaching Jupiter's orbit for the given time span TSS, where NTNO is the number o ...
Astronomy Test over Jovian Planets
... 2. Which of the following planets is similar to Uranus in terms of its size and mass? a. Pluto c. Saturn b. Neptune d. Jupiter 3. The least dense planet in the solar system is a. Jupiter c. Saturn b. Neptune d. Uranus 4. The smallest Jovian planet in the solar system is a. Jupiter c. Saturn b. Neptu ...
... 2. Which of the following planets is similar to Uranus in terms of its size and mass? a. Pluto c. Saturn b. Neptune d. Jupiter 3. The least dense planet in the solar system is a. Jupiter c. Saturn b. Neptune d. Uranus 4. The smallest Jovian planet in the solar system is a. Jupiter c. Saturn b. Neptu ...
Neptune - Midland ISD
... modern one being called the disk instability model. In this process, clumps of dust and gas are bound together early in the life of the solar system. Over time, they combine to form into a giant planet. This could take as little as a thousand years, allowing time for the planet ...
... modern one being called the disk instability model. In this process, clumps of dust and gas are bound together early in the life of the solar system. Over time, they combine to form into a giant planet. This could take as little as a thousand years, allowing time for the planet ...
Planets - Etiwanda E
... • In our Solar System, Saturn is planet number _______ ? • How long is a day on Saturn? • Is a Saturn day longer or shorter than an earth day? • Why is Saturn slightly flattened? • Saturn is well-known for it’s ____________ system. • How many moons does Saturn have? ...
... • In our Solar System, Saturn is planet number _______ ? • How long is a day on Saturn? • Is a Saturn day longer or shorter than an earth day? • Why is Saturn slightly flattened? • Saturn is well-known for it’s ____________ system. • How many moons does Saturn have? ...
Solar System Quiz
... ____ 10. A region of the solar system just beyond Neptune’s orbit, which contains small bodies made mostly of ice, is called a. the Kuiper belt. c. an asteroid belt. b. the outer atmosphere. d. Quasar. ____ 11. Which of the following planets is similar to Uranus in terms of its size and mass? a. Pl ...
... ____ 10. A region of the solar system just beyond Neptune’s orbit, which contains small bodies made mostly of ice, is called a. the Kuiper belt. c. an asteroid belt. b. the outer atmosphere. d. Quasar. ____ 11. Which of the following planets is similar to Uranus in terms of its size and mass? a. Pl ...
Jupiter and its moons
... However, the Europa Orbiter was cancelled in 2003. Further exploration of Europa may have to wait for the Jupiter Icy Moons Orbiter, a large-scale spacecraft carrying yet-to-be-developed technology and driven by electric propulsion powered by a nuclear fission reactor. The mission would launch some ...
... However, the Europa Orbiter was cancelled in 2003. Further exploration of Europa may have to wait for the Jupiter Icy Moons Orbiter, a large-scale spacecraft carrying yet-to-be-developed technology and driven by electric propulsion powered by a nuclear fission reactor. The mission would launch some ...
Jupiter, the dominant Gas Giant Planet
... This diagram shows Galileo’s 11 orbits amongst the satellites of Jupiter. Many detailed photographs and information on the structure of natural satellites were obtained by Galileo (covered later in the Unit Satellites & Rings of the Jovian Planets) The Galileo mission ended on 21 September 2003. Ga ...
... This diagram shows Galileo’s 11 orbits amongst the satellites of Jupiter. Many detailed photographs and information on the structure of natural satellites were obtained by Galileo (covered later in the Unit Satellites & Rings of the Jovian Planets) The Galileo mission ended on 21 September 2003. Ga ...
Exploration Strategy for the Outer Planets 2013
... solar system is unlikely to be visited more than a few times during the professional lifetime of a researcher. This contrasts with missions to the Moon, inner planets and small bodies, where major scientific goals can be reached by accumulating results from multiple smaller missions in the course of ...
... solar system is unlikely to be visited more than a few times during the professional lifetime of a researcher. This contrasts with missions to the Moon, inner planets and small bodies, where major scientific goals can be reached by accumulating results from multiple smaller missions in the course of ...
Document
... They are much bigger, more massive, and less dense than the inner, terrestrial planets. Their internal structure is entirely different from that of the four inner planets. In this chapter, we also discuss a set of moons of these giant planets, some of which range in diameter between ½ and ¼ the size ...
... They are much bigger, more massive, and less dense than the inner, terrestrial planets. Their internal structure is entirely different from that of the four inner planets. In this chapter, we also discuss a set of moons of these giant planets, some of which range in diameter between ½ and ¼ the size ...
ASTRO-114--Lecture 28-
... the time. Once the cloud begins to collapse, it can’t stop. It just starts falling in on itself and it keeps falling in. The only thing that happens is that it begins to spin. Now, this is maybe hard to visualize. But all clouds are moving in one direction or another. They’re all floating through th ...
... the time. Once the cloud begins to collapse, it can’t stop. It just starts falling in on itself and it keeps falling in. The only thing that happens is that it begins to spin. Now, this is maybe hard to visualize. But all clouds are moving in one direction or another. They’re all floating through th ...