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The Naked Eye Stars as Data Supporting Galileo`s
... FIGURE 5: Simulated field of stars of magnitudes 1 through 6 (larger circles representing brighter stars). Top left -- numbers of each magnitude in proportions found in Bright Star Catalog (i.e. real sky). Top right -numbers calculated via equation 3. Bottom left, equal numbers of each magnitude. B ...
... FIGURE 5: Simulated field of stars of magnitudes 1 through 6 (larger circles representing brighter stars). Top left -- numbers of each magnitude in proportions found in Bright Star Catalog (i.e. real sky). Top right -numbers calculated via equation 3. Bottom left, equal numbers of each magnitude. B ...
Astronomy 201 Review 3 Explain why the jovian planets are so
... Explain why the jovian planets are so much different from the terrestrial planets and why Jupiter has the most mass, followed by Saturn, and so forth. Compare the atmospheres of the jovian planets including defining characteristics, weather patterns, and structure. Compare the in ...
... Explain why the jovian planets are so much different from the terrestrial planets and why Jupiter has the most mass, followed by Saturn, and so forth. Compare the atmospheres of the jovian planets including defining characteristics, weather patterns, and structure. Compare the in ...
Jupiter and Saturn
... 5. What is the evidence that Europa has an ocean beneath its surface? 6. What is unusual about the magnetic fields of Ganymede and Callisto? 7. How is it possible for Saturn’s moon Titan to have an atmosphere? 8. Why do some of Jupiter’s moons orbit in the “wrong” direction? 9. What kinds of geologi ...
... 5. What is the evidence that Europa has an ocean beneath its surface? 6. What is unusual about the magnetic fields of Ganymede and Callisto? 7. How is it possible for Saturn’s moon Titan to have an atmosphere? 8. Why do some of Jupiter’s moons orbit in the “wrong” direction? 9. What kinds of geologi ...
Jupiter and Saturn
... 5. What is the evidence that Europa has an ocean beneath its surface? 6. What is unusual about the magnetic fields of Ganymede and Callisto? 7. How is it possible for Saturn’s moon Titan to have an atmosphere? 8. Why do some of Jupiter’s moons orbit in the “wrong” direction? 9. What kinds of geologi ...
... 5. What is the evidence that Europa has an ocean beneath its surface? 6. What is unusual about the magnetic fields of Ganymede and Callisto? 7. How is it possible for Saturn’s moon Titan to have an atmosphere? 8. Why do some of Jupiter’s moons orbit in the “wrong” direction? 9. What kinds of geologi ...
Chapter 9 Lecture Notes
... 5. What is the evidence that Europa has an ocean beneath its surface? 6. What is unusual about the magnetic fields of Ganymede and Callisto? 7. How is it possible for Saturn’s moon Titan to have an atmosphere? 8. Why do some of Jupiter’s moons orbit in the “wrong” direction? 9. What kinds of geologi ...
... 5. What is the evidence that Europa has an ocean beneath its surface? 6. What is unusual about the magnetic fields of Ganymede and Callisto? 7. How is it possible for Saturn’s moon Titan to have an atmosphere? 8. Why do some of Jupiter’s moons orbit in the “wrong” direction? 9. What kinds of geologi ...
Jupiter`s and Saturn`s Moons
... 5. What is the evidence that Europa has an ocean beneath its surface? 6. What is unusual about the magnetic fields of Ganymede and Callisto? 7. How is it possible for Saturn’s moon Titan to have an atmosphere? 8. Why do some of Jupiter’s moons orbit in the “wrong” direction? 9. What kinds of geologi ...
... 5. What is the evidence that Europa has an ocean beneath its surface? 6. What is unusual about the magnetic fields of Ganymede and Callisto? 7. How is it possible for Saturn’s moon Titan to have an atmosphere? 8. Why do some of Jupiter’s moons orbit in the “wrong” direction? 9. What kinds of geologi ...
Document
... Peculiarities of the Earth – Moon system Earth is the only telluric planet with a genuine satellite Among all solar system satellites, our Moon is unique because: • its orbit does not coincide with the planet’s equatorial plane • its large size compared to the planet Moreover, the Moon was closer to ...
... Peculiarities of the Earth – Moon system Earth is the only telluric planet with a genuine satellite Among all solar system satellites, our Moon is unique because: • its orbit does not coincide with the planet’s equatorial plane • its large size compared to the planet Moreover, the Moon was closer to ...
The Milky Way - Department of Physics
... Jupiter’s ring: dark and reddish; only discovered by Voyager 1 spacecraft. Composed of microscopic particles of rocky material ...
... Jupiter’s ring: dark and reddish; only discovered by Voyager 1 spacecraft. Composed of microscopic particles of rocky material ...
Do extrasolar planets go bang
... planet in the sunward direction, and the magnetotail has been observed to stretch anti-sunward as far as the orbit of Saturn, some 750 million km downstream. No wonder the jovian aurorae, powered by its magnetosphere, are so much brighter than their feebly flickering terrestrial counterparts. There ...
... planet in the sunward direction, and the magnetotail has been observed to stretch anti-sunward as far as the orbit of Saturn, some 750 million km downstream. No wonder the jovian aurorae, powered by its magnetosphere, are so much brighter than their feebly flickering terrestrial counterparts. There ...
1. Differential Rotation
... • Janus and Epimethius, have the same orbit, one slightly closer to Saturn than the other; every 4 Earth years they switch places ...
... • Janus and Epimethius, have the same orbit, one slightly closer to Saturn than the other; every 4 Earth years they switch places ...
The Case for the Investigation of the Magnetic Fields and Plasma
... – Juno mission would map high latitude regions of Jovian magnetic field and magnetosphere from Jupiter. Fully endorsed. ...
... – Juno mission would map high latitude regions of Jovian magnetic field and magnetosphere from Jupiter. Fully endorsed. ...
Jupiter and Saturn
... 63 moons have now been found orbiting Jupiter, but most are very small The four largest are the Galilean moons, so called because they were first observed by Galileo: ...
... 63 moons have now been found orbiting Jupiter, but most are very small The four largest are the Galilean moons, so called because they were first observed by Galileo: ...
Questions 1-9
... skyscrapers as the Chrysler Building in New York City and related structures such as the Paramount Theater in Oakland, 5) California The word “zigzag” alludes to the geometric and stylized ornamentation of zigzags, angular patterns, abstracted plant and animal motifs, sunbursts, astrological imagery ...
... skyscrapers as the Chrysler Building in New York City and related structures such as the Paramount Theater in Oakland, 5) California The word “zigzag” alludes to the geometric and stylized ornamentation of zigzags, angular patterns, abstracted plant and animal motifs, sunbursts, astrological imagery ...
Lecture 12
... A. at opposition and it is midnight at your location on Earth. B. at opposition and it is sunset or sunrise at your location on Earth. C. at conjunction and it is midnight at your location on Earth. D. at conjunction and it is sunset or sunrise at your location on Earth. E. at opposition and it is j ...
... A. at opposition and it is midnight at your location on Earth. B. at opposition and it is sunset or sunrise at your location on Earth. C. at conjunction and it is midnight at your location on Earth. D. at conjunction and it is sunset or sunrise at your location on Earth. E. at opposition and it is j ...
The Main Point Overview
... • Inner Galilean moon. • Most volcanically-active world in the solar system! • Interior melted by tides from Jupiter. I ' A Io's Amazing i L Landforms! df ...
... • Inner Galilean moon. • Most volcanically-active world in the solar system! • Interior melted by tides from Jupiter. I ' A Io's Amazing i L Landforms! df ...
OAT Asteroids:Comets
... • “Minor planets”, ranging in size from several hundred km to boulders (most less than 10 km) • Orbits are fairly circular, most between Mars and Jupiter; some orbits in resonance with Jupiter; some Earth-crossing ...
... • “Minor planets”, ranging in size from several hundred km to boulders (most less than 10 km) • Orbits are fairly circular, most between Mars and Jupiter; some orbits in resonance with Jupiter; some Earth-crossing ...
Chapter 18 Folder
... 2. universe 3. galaxy 4. crater 5. solar system 6. satellite 7. space probe p. 167 1. late 2009 2. middle 2012; late 2015 3. Yes, the second full moon would have occurred at the very end of the month. 4. They are referring to something that rarely or seldom happens. ...
... 2. universe 3. galaxy 4. crater 5. solar system 6. satellite 7. space probe p. 167 1. late 2009 2. middle 2012; late 2015 3. Yes, the second full moon would have occurred at the very end of the month. 4. They are referring to something that rarely or seldom happens. ...
Jupiter
... The result of such model building is the set of mass-radius curves on the next slide. Points J, S, U, and N on this plot indicate the observed data for the planets Jupiter, Saturn, Uranus, and Neptune. The point J, representing Jupiter, lies very close to the mass-radius relations for cold planets ...
... The result of such model building is the set of mass-radius curves on the next slide. Points J, S, U, and N on this plot indicate the observed data for the planets Jupiter, Saturn, Uranus, and Neptune. The point J, representing Jupiter, lies very close to the mass-radius relations for cold planets ...
Three basic types of asteroids
... nucleus of comet Tempel 1 on, July 4. Before, during and after the demise of this 820-pound impactor, a "flyby" spacecraft will be watching the 4-mile wide comet nucleus from nearby, collecting pictures and data of the event. The impactor's impact with comet Tempel 1 is expected to form a football-f ...
... nucleus of comet Tempel 1 on, July 4. Before, during and after the demise of this 820-pound impactor, a "flyby" spacecraft will be watching the 4-mile wide comet nucleus from nearby, collecting pictures and data of the event. The impactor's impact with comet Tempel 1 is expected to form a football-f ...
Fun Fact: Venus rotates backward compared with mist other planets
... The Sun The sun is in the center of the solar system. It is also, the biggest object in the solar system. The sun is one of the many, many stars in the universe. ...
... The Sun The sun is in the center of the solar system. It is also, the biggest object in the solar system. The sun is one of the many, many stars in the universe. ...
PlanetTour
... Size: Bigger than our moon and smaller than earth Density: like Mercury, Venus, Earth (~4 times density of water) Atmosphere: Thin, CO2, some greenhouse warming Giant volcanoes due to small gravity Large rift valley Water Flowed at one time May be locked under the surface. Recent indications of perm ...
... Size: Bigger than our moon and smaller than earth Density: like Mercury, Venus, Earth (~4 times density of water) Atmosphere: Thin, CO2, some greenhouse warming Giant volcanoes due to small gravity Large rift valley Water Flowed at one time May be locked under the surface. Recent indications of perm ...
Document
... parallel to the ecliptic plane, instead of perpendicular. • Component perpendicular to the ecliptic points the opposite direction of revolution: retrograde rotation. • The orbital plane of Uranus’s moons is similarly tilted: thus one can’t explain the odd tilt of the planet by invoking one big impac ...
... parallel to the ecliptic plane, instead of perpendicular. • Component perpendicular to the ecliptic points the opposite direction of revolution: retrograde rotation. • The orbital plane of Uranus’s moons is similarly tilted: thus one can’t explain the odd tilt of the planet by invoking one big impac ...
Vagabond MOONS - UMd Astronomy
... finds over the next 6 years. By now, these have pushed the number of known moons in the solar system to 140. ...
... finds over the next 6 years. By now, these have pushed the number of known moons in the solar system to 140. ...
Jovian Planets - Valhalla High School
... 1781 by Sir William Herschel While small relative to Jupiter/Saturn, Uranus is 4x larger in diameter than Earth and has 15x the mass At its far distance, Uranus is difficult to study from Earth, but even close up images from Voyager reveal a rather featureless object Uranus’s Atmosphere Atmo ...
... 1781 by Sir William Herschel While small relative to Jupiter/Saturn, Uranus is 4x larger in diameter than Earth and has 15x the mass At its far distance, Uranus is difficult to study from Earth, but even close up images from Voyager reveal a rather featureless object Uranus’s Atmosphere Atmo ...
Exploration of Io
The exploration of Io, Jupiter's third-largest moon, began with its discovery in 1610 and continues today with Earth-based observations and visits by spacecraft to the Jupiter system. Italian astronomer Galileo Galilei was the first to record an observation of Io on January 8, 1610, though Simon Marius may have also observed Io at around the same time. During the 17th century, observations of Io and the other Galilean satellites helped with the measurement of longitude by map makers and surveyors, with validation of Kepler's Third Law of planetary motion, and with measurement of the speed of light. Based on ephemerides produced by astronomer Giovanni Cassini and others, Pierre-Simon Laplace created a mathematical theory to explain the resonant orbits of three of Jupiter's moons, Io, Europa, and Ganymede. This resonance was later found to have a profound effect on the geologies of these moons. Improved telescope technology in the late 19th and 20th centuries allowed astronomers to resolve large-scale surface features on Io as well as to estimate its diameter and mass.The advent of unmanned spaceflight in the 1950s and 1960s provided an opportunity to observe Io up-close. In the 1960s the moon's effect on Jupiter's magnetic field was discovered. The flybys of the two Pioneer probes, Pioneer 10 and 11 in 1973 and 1974, provided the first accurate measurement of Io's mass and size. Data from the Pioneers also revealed an intense belt of radiation near Io and suggested the presence of an atmosphere. In 1979, the two Voyager spacecraft flew through the Jupiter system. Voyager 1, during its encounter in March 1979, observed active volcanism on Io for the first time and mapped its surface in great detail, particularly the side that faces Jupiter. The Voyagers observed the Io plasma torus and Io's sulfur dioxide (SO2) atmosphere for the first time. NASA launched the Galileo spacecraft in 1989, which entered Jupiter's orbit in December 1995. Galileo allowed detailed study of both the planet and its satellites, including six flybys of Io between late 1999 and early 2002 that provided high-resolution images and spectra of Io's surface, confirming the presence of high-temperature silicate volcanism on Io. Distant observations by Galileo allowed planetary scientists to study changes on the surface that resulted from the moon's active volcanism.Following Galileo and a distant encounter by the Pluto-bound New Horizons spacecraft in 2007, NASA and the European Space Agency (ESA) made plans to return to the Jupiter system and Io. In 2009, NASA approved a plan to send an orbiter to Europa called the Jupiter Europa Orbiter as part of a joint program with ESA called the Europa/Jupiter System Mission. The ESA component of the project was the Jupiter Ganymede Orbiter. However, the EJSM mission collaboration was cancelled. ESA is continuing with its initiative under the name Jupiter Icy Moon Explorer (JUICE) to explore Ganymede, Europa, and Callisto, without plans to investigate Io at all. The proposed NASA Discovery mission Io Volcano Observer, currently going through a competitive process to be selected, would explore Io as its primary mission. In the meantime, Io continues to be observed by the Hubble Space Telescope as well as by Earth-based astronomers using improved telescopes such as Keck and the European Southern Observatory, that use new technologies such as adaptive optics.