Large planets – little moons
... in the same direction as the planet is rotating, while some of the moons are irregular, or going round the other way. The irregular moons are thought of as ‘captured’, rather than formed out of the same material as the mother planet itself, which is the way the regular moons are imagined to have for ...
... in the same direction as the planet is rotating, while some of the moons are irregular, or going round the other way. The irregular moons are thought of as ‘captured’, rather than formed out of the same material as the mother planet itself, which is the way the regular moons are imagined to have for ...
Exam 3
... a hurricane-like storm that has periodically appeared and disappeared over the past 300 years. b) a hurricane-like storm that has been continuously visible on the surface for over 300 years. c) a hurricane-like storm that was first seen after Jupiter was hit by a series of comet fragments. d) a larg ...
... a hurricane-like storm that has periodically appeared and disappeared over the past 300 years. b) a hurricane-like storm that has been continuously visible on the surface for over 300 years. c) a hurricane-like storm that was first seen after Jupiter was hit by a series of comet fragments. d) a larg ...
Astronomy Notes: Planets and Moons
... Red crust, Dust storms (giving color variation seen from Earth) Small Moons (2) Phobos & Deimos JUPITER R = 5 AU T = 12 years D = 140,000 km d = 1.3 ...
... Red crust, Dust storms (giving color variation seen from Earth) Small Moons (2) Phobos & Deimos JUPITER R = 5 AU T = 12 years D = 140,000 km d = 1.3 ...
Guided Notes Section 18.3 Day 2 (Planets)
... b. Competing gravitational forces from ____________ and its many _______ hold the particles in place around the ____________. c. Jupiter, Uranus, and Neptune also have _________, but they are much _____________ and harder to detect than Saturn’s rings. 11. Uranus and Neptune are _________ giants. a. ...
... b. Competing gravitational forces from ____________ and its many _______ hold the particles in place around the ____________. c. Jupiter, Uranus, and Neptune also have _________, but they are much _____________ and harder to detect than Saturn’s rings. 11. Uranus and Neptune are _________ giants. a. ...
16gasgiants2s
... The gas giants have a low density because they are made up mostly of hydrogen and helium the 2 ...
... The gas giants have a low density because they are made up mostly of hydrogen and helium the 2 ...
The Solar System
... than twice as massive as all the other planets combined (the mass of Jupiter is 318 times that of Earth). • Jupiter probably has a core of rocky material amounting to something like 10 to 15 Earth-masses. ...
... than twice as massive as all the other planets combined (the mass of Jupiter is 318 times that of Earth). • Jupiter probably has a core of rocky material amounting to something like 10 to 15 Earth-masses. ...
Our Solar System!!! - Natural History Museum of Los Angeles
... of Venus’ surface. There are many craters, active volcanoes and solidified lava fields. ...
... of Venus’ surface. There are many craters, active volcanoes and solidified lava fields. ...
here
... Jupiter • Jupiter is by far the most massive planet in the solar system (it contains about 2/3 of the solar system mass outside the Sun). • It has the largest radius of any solar system planet, and it rotates the fastest (once every 10 hours). • It has at least 63 moons. • In many categories, Jupit ...
... Jupiter • Jupiter is by far the most massive planet in the solar system (it contains about 2/3 of the solar system mass outside the Sun). • It has the largest radius of any solar system planet, and it rotates the fastest (once every 10 hours). • It has at least 63 moons. • In many categories, Jupit ...
Same and Different - Passport to Knowledge
... *Terrestrial objects: includes the rocky planets Earth, Mercury, Venus, Mars and icy Pluto, Earth’s Moon and the moons of other planets such as Jupiter’s mini-solar system of large satellites, as well as comets, and asteroids—all composed of solid matter. This Activity is a challenging Compare and C ...
... *Terrestrial objects: includes the rocky planets Earth, Mercury, Venus, Mars and icy Pluto, Earth’s Moon and the moons of other planets such as Jupiter’s mini-solar system of large satellites, as well as comets, and asteroids—all composed of solid matter. This Activity is a challenging Compare and C ...
Homework 3
... much larger ground based telescopes than the Hubble. Although option (b) is technically correct, the relative distance change of the Hubble Space Telescope from the Earth’s surface is entirely negligible when compared to the vast distance to our nearest star. The atmosphere is highly volatile and di ...
... much larger ground based telescopes than the Hubble. Although option (b) is technically correct, the relative distance change of the Hubble Space Telescope from the Earth’s surface is entirely negligible when compared to the vast distance to our nearest star. The atmosphere is highly volatile and di ...
A journey through the solar system - Natural History Museum of Los
... of Venus’ surface. There are many craters, active volcanoes and solidified lava fields. ...
... of Venus’ surface. There are many craters, active volcanoes and solidified lava fields. ...
Astronomy 1001/1005 Midterm (200 points) Name:
... 14) What do we conclude if a planet has a lot of impact craters? a) b) c) d) e) ...
... 14) What do we conclude if a planet has a lot of impact craters? a) b) c) d) e) ...
Giant Planets - Wayne State University Physics and Astronomy
... Because of their large sizes, all the giant planets are believed to be strongly heated during their formation The contraction due to gravity produced heat Being the largest, Jupiter was the hottest Some of this primordial heat still remains inside them ...
... Because of their large sizes, all the giant planets are believed to be strongly heated during their formation The contraction due to gravity produced heat Being the largest, Jupiter was the hottest Some of this primordial heat still remains inside them ...
The Solar System The Sun is the star at the center of the Solar S
... more than 1,300 Earths). It also weighs more than twice as much as all the other planets. Jupiter is five times as far from the Sun as the Earth, so its surface temperature is low, around –145 °C. Jupiter is a giant ball of gas, with no solid surface. It is mainly made of the very light gases, hydro ...
... more than 1,300 Earths). It also weighs more than twice as much as all the other planets. Jupiter is five times as far from the Sun as the Earth, so its surface temperature is low, around –145 °C. Jupiter is a giant ball of gas, with no solid surface. It is mainly made of the very light gases, hydro ...
a moon with atmosphere - University of Iowa Astrophysics
... primitive forms of life, or at least give us some insight into the astro-biochemical processes which gave rise (or didn’t) to life. Future spacecraft will have much to explore. Stay tuned. ...
... primitive forms of life, or at least give us some insight into the astro-biochemical processes which gave rise (or didn’t) to life. Future spacecraft will have much to explore. Stay tuned. ...
THE SOLAR SYSTEM
... Dwarf Planets: Pluto is now classified as a dwarf planet because of its small size and distant location. It also overlaps Neptune's orbit because it orbits around the sun in a long elliptical (oval shape) manner rather than a circular one like the other planets. Pluto: Pluto is named after the Roman ...
... Dwarf Planets: Pluto is now classified as a dwarf planet because of its small size and distant location. It also overlaps Neptune's orbit because it orbits around the sun in a long elliptical (oval shape) manner rather than a circular one like the other planets. Pluto: Pluto is named after the Roman ...
Inner and Outer Planets - Sonoma Valley High School
... • 4.6 billion years ago, the solar system was a nebula, a cloud of dust and gas • It began to rotate and flatten, with heavier particles moving toward the center of the disc ...
... • 4.6 billion years ago, the solar system was a nebula, a cloud of dust and gas • It began to rotate and flatten, with heavier particles moving toward the center of the disc ...
Understanding the Outer Planets and Planetary Atmospheres
... new ring systems were discovered by both spacecraft and ground-based observers, often surprising us by contradicting our expectations. The rings’ appearance and composition vary among the planets and within each ring system. The broadest set of rings and the most identified processes are found aroun ...
... new ring systems were discovered by both spacecraft and ground-based observers, often surprising us by contradicting our expectations. The rings’ appearance and composition vary among the planets and within each ring system. The broadest set of rings and the most identified processes are found aroun ...
The Outer Solar System - Super Teacher Worksheets
... hydrogen and helium and a few other gasses, there are violent wind storms that circle around Jupiter. The most famous storm is called the Great Red Spot. It has been churning for more than four hundred years and scientists don’t think it will be slowing down any time soon. Jupiter has its own system ...
... hydrogen and helium and a few other gasses, there are violent wind storms that circle around Jupiter. The most famous storm is called the Great Red Spot. It has been churning for more than four hundred years and scientists don’t think it will be slowing down any time soon. Jupiter has its own system ...
![Overview of the Planets February 4 − Overview: The nine planets [6.1]](http://s1.studyres.com/store/data/008909761_1-5315a2b19f78af295cb3a1fbdc653553-300x300.png)
Overview of the Planets February 4 − Overview: The nine planets [6.1]
... Satellites & rings Asteroids Cosmic dust ...
... Satellites & rings Asteroids Cosmic dust ...
The Planets
... Mercury has no atmosphere and no surface water; the high temperatures prevent these from forming. EXCEPT-Frozen water was found at the poles!!!! The surface of Mercury looks like our Moon. It is covered by craters, indicating its long history of bombardment by asteroids and other impactors. Othe ...
... Mercury has no atmosphere and no surface water; the high temperatures prevent these from forming. EXCEPT-Frozen water was found at the poles!!!! The surface of Mercury looks like our Moon. It is covered by craters, indicating its long history of bombardment by asteroids and other impactors. Othe ...
Planetary Science - Laboratory for Atmospheric and Space Physics
... planets is one of the major scientific findings of the last 25 years. The new ring systems were discovered by both spacecraft and ground-based observers, often surprising us by contradicting our expectations. The rings’ appearance and their composition vary among the planets, and likewise within eac ...
... planets is one of the major scientific findings of the last 25 years. The new ring systems were discovered by both spacecraft and ground-based observers, often surprising us by contradicting our expectations. The rings’ appearance and their composition vary among the planets, and likewise within eac ...
source - UC Berkeley Astronomy w
... Shepherd Moons – Generally small moons that orbit between a planet's rings. Material orbiting near these moons ultimately gets pushed away by the moon's gravitational effects. A single moon will clear a gap in the rings, two moons will confine material into a very narrow ring in between them. Resona ...
... Shepherd Moons – Generally small moons that orbit between a planet's rings. Material orbiting near these moons ultimately gets pushed away by the moon's gravitational effects. A single moon will clear a gap in the rings, two moons will confine material into a very narrow ring in between them. Resona ...
Astronomy 12 Final Review Sheet Sun
... Shepherd Moons – Generally small moons that orbit between a planet's rings. Material orbiting near these moons ultimately gets pushed away by the moon's gravitational effects. A single moon will clear a gap in the rings, two moons will confine material into a very narrow ring in between them. Resona ...
... Shepherd Moons – Generally small moons that orbit between a planet's rings. Material orbiting near these moons ultimately gets pushed away by the moon's gravitational effects. A single moon will clear a gap in the rings, two moons will confine material into a very narrow ring in between them. Resona ...
Exploration of Jupiter
The exploration of Jupiter has been conducted via close observations by automated spacecraft. It began with the arrival of Pioneer 10 into the Jovian system in 1973, and, as of 2014, has continued with seven further spacecraft missions. All of these missions were undertaken by the National Aeronautics and Space Administration (NASA), and all but one have been flybys that take detailed observations without the probe landing or entering orbit. These probes make Jupiter the most visited of the Solar System's outer planets as all missions to the outer Solar System have used Jupiter flybys to reduce fuel requirements and travel time. Plans for more missions to the Jovian system are under development, none of which are scheduled to arrive at the planet before 2016. Sending a craft to Jupiter entails many technical difficulties, especially due to the probes' large fuel requirements and the effects of the planet's harsh radiation environment.The first spacecraft to visit Jupiter was Pioneer 10 in 1973, followed a year later by Pioneer 11. Aside from taking the first close-up pictures of the planet, the probes discovered its magnetosphere and its largely fluid interior. The Voyager 1 and Voyager 2 probes visited the planet in 1979, and studied its moons and the ring system, discovering the volcanic activity of Io and the presence of water ice on the surface of Europa. Ulysses further studied Jupiter's magnetosphere in 1992 and then again in 2000. The Cassini probe approached the planet in 2000 and took very detailed images of its atmosphere. The New Horizons spacecraft passed by Jupiter in 2007 and made improved measurements of its and its satellites' parameters.The Galileo spacecraft is the only one to have entered orbit around Jupiter, arriving in 1995 and studying the planet until 2003. During this period Galileo gathered a large amount of information about the Jovian system, making close approaches to all of the four large Galilean moons and finding evidence for thin atmospheres on three of them, as well as the possibility of liquid water beneath their surfaces. It also discovered a magnetic field around Ganymede. As it approached Jupiter, it also witnessed the impact of Comet Shoemaker–Levy 9. In December 1995, it sent an atmospheric probe into the Jovian atmosphere, so far the only craft to do so.Future probes planned by NASA include the Juno spacecraft, launched in 2011, which will enter a polar orbit around Jupiter to determine whether it has a rocky core. The European Space Agency selected the L1-class JUICE mission in 2012 as part of its Cosmic Vision programme to explore three of Jupiter's Galilean moons, with a possible Ganymede lander provided by Roscosmos. JUICE is proposed to be launched in 2022. Some NASA administrators have even speculated as to the possibility of human exploration of Jupiter, but such missions are not considered feasible with current technology; such as radiation protection.