What is the biggest planet in the solar system?
... diameters of less than 200 km, orbit at radii less than 200,000 km, and have orbital inclinations of less than half a degree. This groups includes the In 1997, the existence of the core was suggested moons of Metis, Adrastea, Amalthea, and Thebe. by gravitational measurements, indicating a mass Alon ...
... diameters of less than 200 km, orbit at radii less than 200,000 km, and have orbital inclinations of less than half a degree. This groups includes the In 1997, the existence of the core was suggested moons of Metis, Adrastea, Amalthea, and Thebe. by gravitational measurements, indicating a mass Alon ...
Solar System Formation
... • Planet travels in front of star, blocking some of stars light, which we can measure ...
... • Planet travels in front of star, blocking some of stars light, which we can measure ...
Moon and Rings - Mid
... Europa - slightly smaller than our Moon Ganymede - largest moon in Solar System, slightly larger than Mercury The closer to Jupiter, the higher the moon density (similar to behavior of terrestrial planets) => like mini “planetary” system! Intense heat of young Jupiter played role of sun. ...
... Europa - slightly smaller than our Moon Ganymede - largest moon in Solar System, slightly larger than Mercury The closer to Jupiter, the higher the moon density (similar to behavior of terrestrial planets) => like mini “planetary” system! Intense heat of young Jupiter played role of sun. ...
Homework 4: Due 11/09/2007
... B) any process by which a planet's surface evolves differently from another planet's surface C) any process by which one part of a planet's surface evolves differently from another part of the same planet's surface D) any process by which a planet evolves differently from its moons E) the process by ...
... B) any process by which a planet's surface evolves differently from another planet's surface C) any process by which one part of a planet's surface evolves differently from another part of the same planet's surface D) any process by which a planet evolves differently from its moons E) the process by ...
Jupiter - Courseweb
... (4) A system is a collection of cycles, structures, and processes that interact. Students should understand a whole in terms of its components and how these components relate to each other and to the whole. All systems have basic properties that can be described in terms of space, time, energy, and ...
... (4) A system is a collection of cycles, structures, and processes that interact. Students should understand a whole in terms of its components and how these components relate to each other and to the whole. All systems have basic properties that can be described in terms of space, time, energy, and ...
Moons of Jupiter Age of Surface
... • If density of planet & moon are the same, then RRoche = 2.5 Rplanet ...
... • If density of planet & moon are the same, then RRoche = 2.5 Rplanet ...
JUPITER AND URANUS
... because it rotates really fast. One year is 84 Earth years because it takes a long time to go around the sun. Uranus ...
... because it rotates really fast. One year is 84 Earth years because it takes a long time to go around the sun. Uranus ...
Long-period
... • discovered with 13-inch telescope using at Lowell by Clyde Tombaugh, by examining plates with a blink comparator • Orbit within Neptune’s at times (’80-99) ...
... • discovered with 13-inch telescope using at Lowell by Clyde Tombaugh, by examining plates with a blink comparator • Orbit within Neptune’s at times (’80-99) ...
Understanding Orbits
... the Sun is 76 years. But it turns out that the gravitational pull of the giant planets creates variations in that period of up to a few years (so the time between successive appearances isn't always exactly 76 years). Its next appearance should be in 2061. ...
... the Sun is 76 years. But it turns out that the gravitational pull of the giant planets creates variations in that period of up to a few years (so the time between successive appearances isn't always exactly 76 years). Its next appearance should be in 2061. ...
Understanding Orbits
... the Sun is 76 years. But it turns out that the gravitational pull of the giant planets creates variations in that period of up to a few years (so the time between successive appearances isn't always exactly 76 years). Its next appearance should be in 2061. ...
... the Sun is 76 years. But it turns out that the gravitational pull of the giant planets creates variations in that period of up to a few years (so the time between successive appearances isn't always exactly 76 years). Its next appearance should be in 2061. ...
The most important questions to study for the exam
... • Hydrogen gas throughout most of its interior, surrounding a small rocky core. • Rock throughout most of the interior, with an atmosphere of hydrogen containing dense clouds. • Hydrogen in liquid form throughout most of the interior, surrounding a small rocky core. 7. One significant physical chara ...
... • Hydrogen gas throughout most of its interior, surrounding a small rocky core. • Rock throughout most of the interior, with an atmosphere of hydrogen containing dense clouds. • Hydrogen in liquid form throughout most of the interior, surrounding a small rocky core. 7. One significant physical chara ...
Comets - Cloudfront.net
... Comets that orbit with a period of less than 200 years are called short period comets. They originate from the Kuiper belt Each time a comet nears the Sun it loses mass. Gradually it evaporates leaving only dust and rock… a meteor shower ...
... Comets that orbit with a period of less than 200 years are called short period comets. They originate from the Kuiper belt Each time a comet nears the Sun it loses mass. Gradually it evaporates leaving only dust and rock… a meteor shower ...
Facilitator Information - Lunar and Planetary Institute
... once every 10 hours and orbits the Sun once every 12 years. This makes its atmosphere tumultuous. The atmosphere is divided into distinct bands. Wind speeds are high - up to 400 kilometers per hour (250 miles per hour)! Lightening on Jupiter is frequent. The Giant Red Spot is a massive storm system, ...
... once every 10 hours and orbits the Sun once every 12 years. This makes its atmosphere tumultuous. The atmosphere is divided into distinct bands. Wind speeds are high - up to 400 kilometers per hour (250 miles per hour)! Lightening on Jupiter is frequent. The Giant Red Spot is a massive storm system, ...
Comets - Cloudfront.net
... Comets that orbit with a period of less than 200 years are called short period comets. Each time a comet nears the Sun it loses mass. Gradually it evaporates leaving only dust and rock… a meteor shower ...
... Comets that orbit with a period of less than 200 years are called short period comets. Each time a comet nears the Sun it loses mass. Gradually it evaporates leaving only dust and rock… a meteor shower ...
A Brief History of Planetary Science
... rings composed of small particles Ring properties different for each planet ...
... rings composed of small particles Ring properties different for each planet ...
Day_31
... • Mainly light elements (hydrogen/helium). • Jupiter’s composition like that of the Sun (71% H, 27% He). • Biggest difference is the amount of massive elements. • Saturn has somewhat more than Jupiter. • Uranus/Neptune have larger fraction of massive elements. ...
... • Mainly light elements (hydrogen/helium). • Jupiter’s composition like that of the Sun (71% H, 27% He). • Biggest difference is the amount of massive elements. • Saturn has somewhat more than Jupiter. • Uranus/Neptune have larger fraction of massive elements. ...
Universal gravitation
... 7. Use the graphing capabilities of your TI calculator to plot T 2 vs. R3 (T2 should be plotted along the vertical axis) and to determine the equation of the line. Write the equation in slope-intercept form below. 8. How does the T2/R3 ratios for Jupiter (as shown in the last column of the data tabl ...
... 7. Use the graphing capabilities of your TI calculator to plot T 2 vs. R3 (T2 should be plotted along the vertical axis) and to determine the equation of the line. Write the equation in slope-intercept form below. 8. How does the T2/R3 ratios for Jupiter (as shown in the last column of the data tabl ...
Jupiter
... obtained by the Yerkes Observatory in the late nineteenth century show an elongated red spot, occupying the same range of latitudes but with twice the longitudinal extension. Sometimes, it is a strong red color, and really quite remarkable, and sometimes pales into insignificance. Historically, init ...
... obtained by the Yerkes Observatory in the late nineteenth century show an elongated red spot, occupying the same range of latitudes but with twice the longitudinal extension. Sometimes, it is a strong red color, and really quite remarkable, and sometimes pales into insignificance. Historically, init ...
Jupiter - Mrs Foos, Room 10
... temperature on Jupiter is about –148ºC (–234ºF). Its atmosphere consists mainly of hydrogen and helium. How Big Is Jupiter? Known as the king of the planets, Jupiter is the largest planet in the Solar System. It is 142,984 kilometers (88,846 mi.) across. Jupiter is so large that 1,300 Earths could f ...
... temperature on Jupiter is about –148ºC (–234ºF). Its atmosphere consists mainly of hydrogen and helium. How Big Is Jupiter? Known as the king of the planets, Jupiter is the largest planet in the Solar System. It is 142,984 kilometers (88,846 mi.) across. Jupiter is so large that 1,300 Earths could f ...
Astronomy Name ______KEY Solar System Objects Quiz Study
... 4. What evidence is there for the solar nebula theory? At least 3 pieces of evidence All planets orbit counter clockwise (CCW); All planets orbit on the ecliptic plane; Axis of rotation (for most planets) is perpendicular to ecliptic 2. Vocabulary 1. Planet spherical; orbit a star; cleared its own o ...
... 4. What evidence is there for the solar nebula theory? At least 3 pieces of evidence All planets orbit counter clockwise (CCW); All planets orbit on the ecliptic plane; Axis of rotation (for most planets) is perpendicular to ecliptic 2. Vocabulary 1. Planet spherical; orbit a star; cleared its own o ...
Asteroids Comets Meteor Showers
... Two types of comets • Long-period comets (P>200 years) – Very elliptical orbits, random inclinations to ecliptic, equally likely to be prograde or retrograde – Many have periods of millions of years. Then orbit sizes are >104 AU. ...
... Two types of comets • Long-period comets (P>200 years) – Very elliptical orbits, random inclinations to ecliptic, equally likely to be prograde or retrograde – Many have periods of millions of years. Then orbit sizes are >104 AU. ...
Asteroid - Hoover12
... Comets contain information about the outer solar system Most of them visit the inner part only once, a few are regular guests One of the most famous comets is Halley’s comet. It was discovered by Edmund Halley in 1682. Its orbital period is 76 years. The last appearance in ...
... Comets contain information about the outer solar system Most of them visit the inner part only once, a few are regular guests One of the most famous comets is Halley’s comet. It was discovered by Edmund Halley in 1682. Its orbital period is 76 years. The last appearance in ...
Outer or Jovian Planets - Academic Computer Center
... sidereal rate, that is at the same rate that the stars appeared to move across the sky so it had to be coming from something in space and not something on the ground. • Further observations showed that the bursts were actually drifting slightly, (could it be a planet?). • Only Jupiter was overhead a ...
... sidereal rate, that is at the same rate that the stars appeared to move across the sky so it had to be coming from something in space and not something on the ground. • Further observations showed that the bursts were actually drifting slightly, (could it be a planet?). • Only Jupiter was overhead a ...
Comet Shoemaker–Levy 9
Comet Shoemaker–Levy 9 (formally designated D/1993 F2) was a comet that broke apart and collided with Jupiter in July 1994, providing the first direct observation of an extraterrestrial collision of Solar System objects. This generated a large amount of coverage in the popular media, and the comet was closely observed by astronomers worldwide. The collision provided new information about Jupiter and highlighted its role in reducing space debris in the inner Solar System.The comet was discovered by astronomers Carolyn and Eugene M. Shoemaker and David Levy. Shoemaker–Levy 9, at the time captured by and orbiting Jupiter, was located on the night of March 24, 1993, in a photograph taken with the 40 cm (16 in) Schmidt telescope at the Palomar Observatory in California. It was the first comet observed to be orbiting a planet, and had probably been captured by the planet around 20 – 30 years earlier.Calculations showed that its unusual fragmented form was due to a previous closer approach to Jupiter in July 1992. At that time, the orbit of Shoemaker–Levy 9 passed within Jupiter's Roche limit, and Jupiter's tidal forces had acted to pull apart the comet. The comet was later observed as a series of fragments ranging up to 2 km (1.2 mi) in diameter. These fragments collided with Jupiter's southern hemisphere between July 16 and July 22, 1994, at a speed of approximately 60 km/s (37 mi/s) or 216,000 km/h (134,000 mph). The prominent scars from the impacts were more easily visible than the Great Red Spot and persisted for many months.