Juno
... processes and conditions that governed our solar system during its formation. As our primary example of a giant planet, Jupiter can also provide critical knowledge for understanding the planetary systems being discovered around other stars. Back to Table of Contents ...
... processes and conditions that governed our solar system during its formation. As our primary example of a giant planet, Jupiter can also provide critical knowledge for understanding the planetary systems being discovered around other stars. Back to Table of Contents ...
Solar System Virtual Lab Handout
... 2. How do the distances between the orbits of the inner planets compare to the distances between the orbits of the outer planets? ...
... 2. How do the distances between the orbits of the inner planets compare to the distances between the orbits of the outer planets? ...
charts_set_6
... Icy/rocky composition Moons: Charon: radius about 590 km or 0.1 REarth . Pluto and Charon tidally locked. Nix and Hydra about 30-100 km. Origin of Pluto Now known to be just the largest known of a class of objects in the outer reaches of the Solar System. These objects are Kuiper Belt Objects. ...
... Icy/rocky composition Moons: Charon: radius about 590 km or 0.1 REarth . Pluto and Charon tidally locked. Nix and Hydra about 30-100 km. Origin of Pluto Now known to be just the largest known of a class of objects in the outer reaches of the Solar System. These objects are Kuiper Belt Objects. ...
14. 1 A Travel Guide to the Outer Planets 14.2 Jupiter 14.3 Saturn
... Jupiter and Saturn, usually called "gas giants;' are composed mostly of liquid hydrogen and might instead be called "liquid giants:' Uranus and Neptune contain water in liquid and solid form and therefore are sometimes called "ice giants:' All of the Jovian worlds have large systems of satellites an ...
... Jupiter and Saturn, usually called "gas giants;' are composed mostly of liquid hydrogen and might instead be called "liquid giants:' Uranus and Neptune contain water in liquid and solid form and therefore are sometimes called "ice giants:' All of the Jovian worlds have large systems of satellites an ...
What do you think about the origin of most of Jupiter`s moons?
... New evidence published this year • Gravity models using just the four gas giant planets is not able to produce the orbits we see today. • Early on in the solar system it is thought that this extra planet was sped up by interactions and flung out of the solar system. ...
... New evidence published this year • Gravity models using just the four gas giant planets is not able to produce the orbits we see today. • Early on in the solar system it is thought that this extra planet was sped up by interactions and flung out of the solar system. ...
Document
... 1. The brightest star visible from the northern hemisphere is the star Sirius, which is 8.7 light years from Earth in the constellation of Canis Major. It takes a spaceship 4.9 years to travel from Earth to Sirius, according to the spaceship’s on board clocks. According to Earth clocks, the trip tak ...
... 1. The brightest star visible from the northern hemisphere is the star Sirius, which is 8.7 light years from Earth in the constellation of Canis Major. It takes a spaceship 4.9 years to travel from Earth to Sirius, according to the spaceship’s on board clocks. According to Earth clocks, the trip tak ...
Moonstruck Scientists Count 63 and Rising
... Io, a moon of Jupiter, is so volcanic that it “glows in the dark,” said Paul Geissler, an astronomer at the University of Arizona in Tucson. A NASA photo caught one volcano in mid-eruption, shooting a plume of hot gas hundreds of miles into space. “Io glows green, blue, and red” said Geissler. “It l ...
... Io, a moon of Jupiter, is so volcanic that it “glows in the dark,” said Paul Geissler, an astronomer at the University of Arizona in Tucson. A NASA photo caught one volcano in mid-eruption, shooting a plume of hot gas hundreds of miles into space. “Io glows green, blue, and red” said Geissler. “It l ...
(He) particles understand where we are traveling in space
... one system to another can help us understand more about the strength of each auroral source. Investigating scientific mysteries through an interdisciplinary lens helps us see science from a whole systems approach, which in turn gives us important information about our own Earth-based systems. On bot ...
... one system to another can help us understand more about the strength of each auroral source. Investigating scientific mysteries through an interdisciplinary lens helps us see science from a whole systems approach, which in turn gives us important information about our own Earth-based systems. On bot ...
2010_03_09 LP18 & 19 Jupiter Saturn Uranus
... made of? How do we know that compounds are in an atmosphere, and not their components? Is/was there life on the giant planets or their moons? What makes the colors? Do the colors/stripes change over time? RINGS?!?!?!??!?!?!?! Temperature? ...
... made of? How do we know that compounds are in an atmosphere, and not their components? Is/was there life on the giant planets or their moons? What makes the colors? Do the colors/stripes change over time? RINGS?!?!?!??!?!?!?! Temperature? ...
The Outer Solar System Chapter 7:
... Radius: ~ 16 % smaller than Jupiter Av. density: 0.69 g/cm3 → Would float in water! ...
... Radius: ~ 16 % smaller than Jupiter Av. density: 0.69 g/cm3 → Would float in water! ...
File
... Since our book was published, some exciting discoveries have been made in the region that lies outside of the orbit of Neptune. The region is called the Kuiper Belt and is the home to many dwarf planets, including Pluto and Eris, which was only discovered in 2005. Eris is bigger than Pluto! In 2006, ...
... Since our book was published, some exciting discoveries have been made in the region that lies outside of the orbit of Neptune. The region is called the Kuiper Belt and is the home to many dwarf planets, including Pluto and Eris, which was only discovered in 2005. Eris is bigger than Pluto! In 2006, ...
Earth Science
... hydrogen and helium (liquid core, gaseous atmosphere). Has over 60 moons including four large moons. The Great Red Spot, a huge atmospheric storm that has lasted for at least 300 years. ...
... hydrogen and helium (liquid core, gaseous atmosphere). Has over 60 moons including four large moons. The Great Red Spot, a huge atmospheric storm that has lasted for at least 300 years. ...
Stratigraphy and composition of lava flows in Mare Nubium
... Soon after the planets formed there was a lot of leftover debris from the planet building process – things like comets and asteroids. With its powerful gravity, Jupiter sucked up many of them and also kicked lots of them out of the Solar System that could have hit Earth. Because of this, Jupiter is ...
... Soon after the planets formed there was a lot of leftover debris from the planet building process – things like comets and asteroids. With its powerful gravity, Jupiter sucked up many of them and also kicked lots of them out of the Solar System that could have hit Earth. Because of this, Jupiter is ...
August 2016
... sea of salty water lies under Ganymede’s curst. The same seems to be true of Europa and Callisto. Also Galileo’s infared spectrometer showed traces of salt on Ganymede’s surface consistent with brine making its way to the surface by means of eruptions. It’s been suggested that Ganymede’s seas are la ...
... sea of salty water lies under Ganymede’s curst. The same seems to be true of Europa and Callisto. Also Galileo’s infared spectrometer showed traces of salt on Ganymede’s surface consistent with brine making its way to the surface by means of eruptions. It’s been suggested that Ganymede’s seas are la ...
Sample Final - Lawrence University
... Why are mountains and volcanoes on Mars so much taller on Mars than on the Earth? (a) Mars lacks plate tectonics and has a lower surface gravity than the Earth. (b) The atmospheric pressure on Mars is much lower than on the Earth. (c) The surface of mars is composed of low-density ices. (d) Gigantic ...
... Why are mountains and volcanoes on Mars so much taller on Mars than on the Earth? (a) Mars lacks plate tectonics and has a lower surface gravity than the Earth. (b) The atmospheric pressure on Mars is much lower than on the Earth. (c) The surface of mars is composed of low-density ices. (d) Gigantic ...
Physics 110 - Lawrence University
... Why are mountains and volcanoes on Mars so much taller on Mars than on the Earth? (a) Mars lacks plate tectonics and has a lower surface gravity than the Earth. (b) The atmospheric pressure on Mars is much lower than on the Earth. (c) The surface of mars is composed of low-density ices. (d) Gigantic ...
... Why are mountains and volcanoes on Mars so much taller on Mars than on the Earth? (a) Mars lacks plate tectonics and has a lower surface gravity than the Earth. (b) The atmospheric pressure on Mars is much lower than on the Earth. (c) The surface of mars is composed of low-density ices. (d) Gigantic ...
Lecture 08a: Galilean moons - Sierra College Astronomy Home Page
... The closest Galilean satellite to Jupiter; Extreme tidal forces; 200× the heat per gram, compared to radioactivity on Earth); The most volcanically active place in the Solar System; Typical temperatures are 90-130K; Constant volcanic eruptions, local temperatures reaching 2000ºC (3600ºF); ...
... The closest Galilean satellite to Jupiter; Extreme tidal forces; 200× the heat per gram, compared to radioactivity on Earth); The most volcanically active place in the Solar System; Typical temperatures are 90-130K; Constant volcanic eruptions, local temperatures reaching 2000ºC (3600ºF); ...
Study Guide for Midterm 2 Midterm 1 Exam procedures
... There are also a few more general ideas that you should understand, including the following ...
... There are also a few more general ideas that you should understand, including the following ...
12 6 4 10 14 8 2 16 Saturn Neptune Jupiter Uranus
... Slide your thumb and your forefinger behind 2 of the planets and press together so they bend round and touch. ...
... Slide your thumb and your forefinger behind 2 of the planets and press together so they bend round and touch. ...
How the Universe Works: Extreme Planets Name State whether the
... 16. The larger the gas giants got the more _________________ they have. 17. Jupiter and Saturn have over _______ moons each. They formed from the massive amounts of gas and dust that the planets were able to collect because of their gravity. 18. All gas giants have rings. True or false? 19. What is ...
... 16. The larger the gas giants got the more _________________ they have. 17. Jupiter and Saturn have over _______ moons each. They formed from the massive amounts of gas and dust that the planets were able to collect because of their gravity. 18. All gas giants have rings. True or false? 19. What is ...
The Solar System
... The Moons There are 162 moons in our solar system and they are still looking today Jupiter has the most moons The dwarf planet has its moon slightly smaller then the plant Our is also called Luna ...
... The Moons There are 162 moons in our solar system and they are still looking today Jupiter has the most moons The dwarf planet has its moon slightly smaller then the plant Our is also called Luna ...
Homework 4 (due Tuesday, May 3, 2016)
... have had free-flowing water and a denser atmosphere as recently as a few million years ago. It is possible that life evolved then. Future Mars missions will look for it. (C) Viking experiments gave us only negative or ambiguous results. Also, the period when surface water and a denser atmosphere may ...
... have had free-flowing water and a denser atmosphere as recently as a few million years ago. It is possible that life evolved then. Future Mars missions will look for it. (C) Viking experiments gave us only negative or ambiguous results. Also, the period when surface water and a denser atmosphere may ...
Homework 4 AST 301, Spring 2015 PLEASE ANSWER THIS
... have had free-flowing water and a denser atmosphere as recently as a few million years ago. It is possible that life evolved then. Future Mars missions will look for it. (C) Viking experiments gave us only negative or ambiguous results. Also, the period when surface water and a denser atmosphere may ...
... have had free-flowing water and a denser atmosphere as recently as a few million years ago. It is possible that life evolved then. Future Mars missions will look for it. (C) Viking experiments gave us only negative or ambiguous results. Also, the period when surface water and a denser atmosphere may ...
The Outer Planets
... last for 100s of years (GRS) Largest planet Over 60 moons, most in our solar system ...
... last for 100s of years (GRS) Largest planet Over 60 moons, most in our solar system ...
Midterm 2 Wednesday (Feb 29)
... • On top of rock/ice core with 10-15 x mass of Earth. • Lots of weather on Jupiter • Ammonia (NH3) clouds. • Strong winds at different latitudes. (differential rotation) • Cyclonic storms • Great Red Spot – 2 x size of Earth – 400 yrs so far ...
... • On top of rock/ice core with 10-15 x mass of Earth. • Lots of weather on Jupiter • Ammonia (NH3) clouds. • Strong winds at different latitudes. (differential rotation) • Cyclonic storms • Great Red Spot – 2 x size of Earth – 400 yrs so far ...
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.