Constructing a Solar System
... Click on the scaling tab to view the distance and diameter data for the planets. Now enter the appropriate numbers into the yellow cells on the scaling tab. The spreadsheet will automatically do the math for you. From the scaled data, how do the distances from the Sun and planet diameters ...
... Click on the scaling tab to view the distance and diameter data for the planets. Now enter the appropriate numbers into the yellow cells on the scaling tab. The spreadsheet will automatically do the math for you. From the scaled data, how do the distances from the Sun and planet diameters ...
Our Gigantic Solar System
... Using the Imperial system, Jupiter's average distance - AKA Jupiter's semi major axis - it is 483.78 million miles away from the sun. Jupiter is one planet in the solar system which justifies use of the word "gigantic". It is mostly composed of hydrogen, helium, and methane, including the very cold ...
... Using the Imperial system, Jupiter's average distance - AKA Jupiter's semi major axis - it is 483.78 million miles away from the sun. Jupiter is one planet in the solar system which justifies use of the word "gigantic". It is mostly composed of hydrogen, helium, and methane, including the very cold ...
Test#2
... 11. Suppose a planet is orbited by a number of satellites. Which of the satellites will feel the strongest tidal forces due to the planet? a) a large satellite in a close orbit, b) a large satellite in a distant orbit c) a small satellite in a close orbit, d) a small satellite in a distant orbit 12. ...
... 11. Suppose a planet is orbited by a number of satellites. Which of the satellites will feel the strongest tidal forces due to the planet? a) a large satellite in a close orbit, b) a large satellite in a distant orbit c) a small satellite in a close orbit, d) a small satellite in a distant orbit 12. ...
Module2 Unit1 Tales of the unexplained
... Jupiter is the fifth planet from the Sun and by far the largest. Jupiter is more than twice as massive as all the other planets combined (the mass of Jupiter is 318 times that of Earth).Jupiter is the fourth brightest object in the sky (after the Sun, the Moon and Venus). Saturn is the sixth planet ...
... Jupiter is the fifth planet from the Sun and by far the largest. Jupiter is more than twice as massive as all the other planets combined (the mass of Jupiter is 318 times that of Earth).Jupiter is the fourth brightest object in the sky (after the Sun, the Moon and Venus). Saturn is the sixth planet ...
Planet Earth - ThinkChemistry
... • What is the difference between stars, planets and moons? • What is the difference between The Solar System, a galaxy and The Universe? ...
... • What is the difference between stars, planets and moons? • What is the difference between The Solar System, a galaxy and The Universe? ...
Lesson 29
... temperatures 320 degrees below zero. They are the farthest from the sun. On Mercury, the temperature can reach 600 degrees; on Venus, the temperature may reach 860 degrees. Plants and animals can’t survive on these planets because of the heat or the cold. Earth is called the “Life Planet” because sc ...
... temperatures 320 degrees below zero. They are the farthest from the sun. On Mercury, the temperature can reach 600 degrees; on Venus, the temperature may reach 860 degrees. Plants and animals can’t survive on these planets because of the heat or the cold. Earth is called the “Life Planet” because sc ...
Galaxy and Beyond
... the Sun (can range from 30 - 50 Aus) Astronomical Unit (AU) - is distance b/w Earth & Sun (about 93 million miles) ...
... the Sun (can range from 30 - 50 Aus) Astronomical Unit (AU) - is distance b/w Earth & Sun (about 93 million miles) ...
powerpoint version
... • Mass about half that of Jupiter • Just 0.05 AU from star (1/20th of Earth-Sun) • Surface temperature probably about 1300 K • Confirmed by Marcy and Butler Nothing like Mercury / the solar system. How did it get there? Massive planet formed further out and dragged in by gas and dust? If so, any ter ...
... • Mass about half that of Jupiter • Just 0.05 AU from star (1/20th of Earth-Sun) • Surface temperature probably about 1300 K • Confirmed by Marcy and Butler Nothing like Mercury / the solar system. How did it get there? Massive planet formed further out and dragged in by gas and dust? If so, any ter ...
ASTR 2020, Spring 2015 Professor Jack Burns Final Exam
... planet with a mass twice that of Earth (2MEarth) orbits at a distance of 1 AU (astronomical unit) from the star. What is the orbital period of this planet? a. 1 year b. 6 months c. 2 years d. 4 years e. It cannot be determined from the information given. A: a – The orbital period of a planet depends ...
... planet with a mass twice that of Earth (2MEarth) orbits at a distance of 1 AU (astronomical unit) from the star. What is the orbital period of this planet? a. 1 year b. 6 months c. 2 years d. 4 years e. It cannot be determined from the information given. A: a – The orbital period of a planet depends ...
1 2 3 4 5 6 Orbital Distance (AU) Orbital Period (Years) 1 2 3 4 5 6 7
... Enter your answers using a pencil on a Scantron form. This portion of the homework investigates the relationship between how long it takes a planet to orbit a star (orbital period) and how far away that planet is from the star (orbital distance). We will start by investigating an imaginary planetary ...
... Enter your answers using a pencil on a Scantron form. This portion of the homework investigates the relationship between how long it takes a planet to orbit a star (orbital period) and how far away that planet is from the star (orbital distance). We will start by investigating an imaginary planetary ...
MS Word version
... orbit? (1 AU) Note that this satisfies Kepler’s 3rd Law --- that P2 = a3. Why aren’t any of the planets moving? (They are moving, just very slowly at this animation rate.) Kepler’s 3rd Law tells us that planets ...
... orbit? (1 AU) Note that this satisfies Kepler’s 3rd Law --- that P2 = a3. Why aren’t any of the planets moving? (They are moving, just very slowly at this animation rate.) Kepler’s 3rd Law tells us that planets ...
Lab_Solar system size scale2
... so that the amount it is stretched open is equal to the scale radius of the planet. As you measure each planet using the compass, make a circle with that measurement on a piece of construction paper to represent the planet. Some planets are too small to use the compass very well. Here is how Jupiter ...
... so that the amount it is stretched open is equal to the scale radius of the planet. As you measure each planet using the compass, make a circle with that measurement on a piece of construction paper to represent the planet. Some planets are too small to use the compass very well. Here is how Jupiter ...
Not too hot, not too cold: New Earth-like planet could
... Institution of Washington, have been studying the movement of the planet's parent star, a red dwarf called Gliese 581, for 11 years. Their observations have revealed a number of exoplanets spinning around the star. Possibility of life Recently they discovered two new alien worlds, so together with t ...
... Institution of Washington, have been studying the movement of the planet's parent star, a red dwarf called Gliese 581, for 11 years. Their observations have revealed a number of exoplanets spinning around the star. Possibility of life Recently they discovered two new alien worlds, so together with t ...
User guide 2 - Finding celestial treasures
... Positions section. (Strangely, Mercury is the planet most often closest to Earth, being the nearest about 50% of the time.) Venus is brilliant and is easy to spot when it is not near the sun. It lies either in the west after sunset or in the east before sunrise. Like our moon, it shows phases. When ...
... Positions section. (Strangely, Mercury is the planet most often closest to Earth, being the nearest about 50% of the time.) Venus is brilliant and is easy to spot when it is not near the sun. It lies either in the west after sunset or in the east before sunrise. Like our moon, it shows phases. When ...
DIY Solar System
... The Solar System consists of the Sun and eight planets, their moons, and other non-stellar objects, such as asteroids. The four smaller inner planets—Mercury, Venus, Earth and Mars, also called the terrestrial planets—are primarily composed of rock and metal. The four outer planets, called the gas g ...
... The Solar System consists of the Sun and eight planets, their moons, and other non-stellar objects, such as asteroids. The four smaller inner planets—Mercury, Venus, Earth and Mars, also called the terrestrial planets—are primarily composed of rock and metal. The four outer planets, called the gas g ...
New Scientist Magazine - Surrey, England… 19th November 2008
... Wanted: Rocky planet outside of our solar system. Must not be too hot or too cold, but just the right temperature to support life. It sounds like a simple enough wish list, but finding a planet that fulfils all of these criteria has kept astronomers busy for decades. Until recently, it meant finding ...
... Wanted: Rocky planet outside of our solar system. Must not be too hot or too cold, but just the right temperature to support life. It sounds like a simple enough wish list, but finding a planet that fulfils all of these criteria has kept astronomers busy for decades. Until recently, it meant finding ...
Take a Grand Tour of the solar system at twice the speed of light
... coming as close to the Sun as Neptune’s orbit, but going out as far as 50 times Earth’s distance from the sun, which is where we mark it in the model. Light travel time to Pluto from the Sun is nearly 7 hours. How long did it take you to traverse the distance? Onward to the stars, the nearest would ...
... coming as close to the Sun as Neptune’s orbit, but going out as far as 50 times Earth’s distance from the sun, which is where we mark it in the model. Light travel time to Pluto from the Sun is nearly 7 hours. How long did it take you to traverse the distance? Onward to the stars, the nearest would ...
Presentación de PowerPoint
... more matter than all the other planets put together, and its volume is one thousand times the volume of Earth. It has many satellites, and four of them (Io, Callisto, Europa and Ganymede) were discovered by Galilei in 1610. Its thick atmosphere is complex, and it is made up of hydrogen (90%) and hel ...
... more matter than all the other planets put together, and its volume is one thousand times the volume of Earth. It has many satellites, and four of them (Io, Callisto, Europa and Ganymede) were discovered by Galilei in 1610. Its thick atmosphere is complex, and it is made up of hydrogen (90%) and hel ...
Document
... ecliptic. Therefore, the Sun and Earth both lie exactly on the plane of the ecliptic, and equivalently the Sun is seen by definition to lie exactly on the ecliptic as viewed from the Earth. The other planets of the solar system lie approximately but not exactly on the ecliptic: their orbits lie on p ...
... ecliptic. Therefore, the Sun and Earth both lie exactly on the plane of the ecliptic, and equivalently the Sun is seen by definition to lie exactly on the ecliptic as viewed from the Earth. The other planets of the solar system lie approximately but not exactly on the ecliptic: their orbits lie on p ...
ppt
... •The energy for this activity may have been provided by tidal heating – occurred when Triton was captured by Neptune’s gravity into a retrograde orbit ...
... •The energy for this activity may have been provided by tidal heating – occurred when Triton was captured by Neptune’s gravity into a retrograde orbit ...
Lesson 6 Slides
... planet to orbit the Sun increases rapidly with the radius of its orbit. Thus, we find that Mercury, the innermost planet, takes only 88 days to orbit the Sun but the outermost planet (Pluto) requires 248 years to do the same. ...
... planet to orbit the Sun increases rapidly with the radius of its orbit. Thus, we find that Mercury, the innermost planet, takes only 88 days to orbit the Sun but the outermost planet (Pluto) requires 248 years to do the same. ...
Section 23.3 The Outer Planets
... Instead of being generally perpendicular to the plane of its orbit like the other planets, Uranus’s axis of rotation lies nearly parallel with the plane of its orbit. ...
... Instead of being generally perpendicular to the plane of its orbit like the other planets, Uranus’s axis of rotation lies nearly parallel with the plane of its orbit. ...
Planets beyond Neptune
Following the discovery of the planet Neptune in 1846, there was considerable speculation that another planet might exist beyond its orbit. The search began in the mid-19th century and culminated at the start of the 20th with Percival Lowell's quest for Planet X. Lowell proposed the Planet X hypothesis to explain apparent discrepancies in the orbits of the giant planets, particularly Uranus and Neptune, speculating that the gravity of a large unseen ninth planet could have perturbed Uranus enough to account for the irregularities.Clyde Tombaugh's discovery of Pluto in 1930 appeared to validate Lowell's hypothesis, and Pluto was officially named the ninth planet. In 1978, Pluto was conclusively determined to be too small for its gravity to affect the giant planets, resulting in a brief search for a tenth planet. The search was largely abandoned in the early 1990s, when a study of measurements made by the Voyager 2 spacecraft found that the irregularities observed in Uranus's orbit were due to a slight overestimation of Neptune's mass. After 1992, the discovery of numerous small icy objects with similar or even wider orbits than Pluto led to a debate over whether Pluto should remain a planet, or whether it and its neighbours should, like the asteroids, be given their own separate classification. Although a number of the larger members of this group were initially described as planets, in 2006 the International Astronomical Union reclassified Pluto and its largest neighbours as dwarf planets, leaving Neptune the farthest known planet in the Solar System.Today, the astronomical community widely agrees that Planet X, as originally envisioned, does not exist, but the concept of Planet X has been revived by a number of astronomers to explain other anomalies observed in the outer Solar System. In popular culture, and even among some astronomers, Planet X has become a stand-in term for any undiscovered planet in the outer Solar System, regardless of its relationship to Lowell's hypothesis. Other trans-Neptunian planets have also been suggested, based on different evidence. As of March 2014, observations with the WISE telescope have ruled out the possibility of a Saturn-sized object out to 10,000 AU, and a Jupiter-sized or larger object out to 26,000 AU.