Inner and Outer Planets of the Solar System
... System. The high activity is believed to be caused by Jupiter and the other moons gravitational effect on Io. They squeeze and stretch the moon heating up its interior to very high temperatures. Eruptions resulting in plumes hundreds of kilometers high are then inevitable to relieve the pressure. Be ...
... System. The high activity is believed to be caused by Jupiter and the other moons gravitational effect on Io. They squeeze and stretch the moon heating up its interior to very high temperatures. Eruptions resulting in plumes hundreds of kilometers high are then inevitable to relieve the pressure. Be ...
The Solar System
... • the path of an object in space as it travels around another object • planets orbit around the sun in an elliptical (flattened circle or oval) path; proposed by Johannes Kepler Kepler’s 1st Law • due to the gravitational attraction, a planet’s (or other object’s) speed increases as it approaches ...
... • the path of an object in space as it travels around another object • planets orbit around the sun in an elliptical (flattened circle or oval) path; proposed by Johannes Kepler Kepler’s 1st Law • due to the gravitational attraction, a planet’s (or other object’s) speed increases as it approaches ...
Information and workshee - Athens
... c. Neptune b. Jupiter d. Pluto 2. Which planet takes the longest to complete one revolution (orbit) around the sun? a. Mercury c. Uranus b. Earth d. Pluto ...
... c. Neptune b. Jupiter d. Pluto 2. Which planet takes the longest to complete one revolution (orbit) around the sun? a. Mercury c. Uranus b. Earth d. Pluto ...
The Final Frontier
... On clear nights, you can often see our moon and many stars. You might even see a planet! To learn more about our solar system, study the chart below. Tips • The planet closest to the Sun is number “1.” • Questions 1–4 contain hints. ...
... On clear nights, you can often see our moon and many stars. You might even see a planet! To learn more about our solar system, study the chart below. Tips • The planet closest to the Sun is number “1.” • Questions 1–4 contain hints. ...
Astronomy word grid
... 14. Name given to the line between day and night on the Moon 17. The brightest star in the northern sky 18. The apparent backwards movement of the planets in the sky 22. A type of variable star used to measure distance 25. The name used to describe the brightness of a star 26. The name given to a ve ...
... 14. Name given to the line between day and night on the Moon 17. The brightest star in the northern sky 18. The apparent backwards movement of the planets in the sky 22. A type of variable star used to measure distance 25. The name used to describe the brightness of a star 26. The name given to a ve ...
Our Solar System
... • Neptune is a giant gas planet which is most likely made up of various “ices” and rock. Neptune has been visited by only spacecraft, voyagers on Aug. 25, 1989. • Almost everything we know about Neptune comes from this one visit. ...
... • Neptune is a giant gas planet which is most likely made up of various “ices” and rock. Neptune has been visited by only spacecraft, voyagers on Aug. 25, 1989. • Almost everything we know about Neptune comes from this one visit. ...
Planets and Other Space Rocks Notes
... • A year is 29.5 Earth years, and a day is 10.2 hours. • The temperature at the top is −178℃. • It has a tilt, so it has seasons like Earth, but they are mild. ...
... • A year is 29.5 Earth years, and a day is 10.2 hours. • The temperature at the top is −178℃. • It has a tilt, so it has seasons like Earth, but they are mild. ...
Solutions to test #1 taken on Monday
... 19. (4) What configuration of the Earth, Sun, and Moon gives rise to Neap Tides (lowest high tides)? Draw a picture if that would help. ...
... 19. (4) What configuration of the Earth, Sun, and Moon gives rise to Neap Tides (lowest high tides)? Draw a picture if that would help. ...
BABYLON and SUMERIA 3000BC
... the heavenly spheres and heavenly bodies (stars and planets). Each of the four earthly elements has its natural place. All that is earthly tends toward the center of the universe, i.e., the center of the Earth. Water tends toward a sphere surrounding the center. Air tends toward a sphere surrounding ...
... the heavenly spheres and heavenly bodies (stars and planets). Each of the four earthly elements has its natural place. All that is earthly tends toward the center of the universe, i.e., the center of the Earth. Water tends toward a sphere surrounding the center. Air tends toward a sphere surrounding ...
Our Solar System
... Mercury: 38% of Earth’s Venus: 91% of Earth’s Earth: 100% of Earth’s Mars: 38% of Earth’s Jupiter: 254% of Earth’s Saturn: 108% of Earth’s Uranus: 91% of Earth’s Neptune: 119% of Earth’s Pluto: 8% of Earth’s So what this all means is that a person who weighs 100 pounds on Earth would weigh 38 pounds ...
... Mercury: 38% of Earth’s Venus: 91% of Earth’s Earth: 100% of Earth’s Mars: 38% of Earth’s Jupiter: 254% of Earth’s Saturn: 108% of Earth’s Uranus: 91% of Earth’s Neptune: 119% of Earth’s Pluto: 8% of Earth’s So what this all means is that a person who weighs 100 pounds on Earth would weigh 38 pounds ...
Chapter 13 Lesson 3 Notes
... The planets are divided into four ___________________ planets and four ___________________ planets. The planets are separated by a huge ___________________ ___________________ between Mars and ___________________. The asteroid ___________________ is a ring shaped area where many small, rocky bodies ...
... The planets are divided into four ___________________ planets and four ___________________ planets. The planets are separated by a huge ___________________ ___________________ between Mars and ___________________. The asteroid ___________________ is a ring shaped area where many small, rocky bodies ...
The Solar System - uheledsciencemethods
... • Fifth planet from the sun and the largest planet in the Solar System • Considered a gas giant planet • Mostly made out of hydrogen and a little bit of helium • Has a giant storm known as the Great Red Spot ...
... • Fifth planet from the sun and the largest planet in the Solar System • Considered a gas giant planet • Mostly made out of hydrogen and a little bit of helium • Has a giant storm known as the Great Red Spot ...
1 - WordPress.com
... Science 9 Questions: Chapter 11.2 The Sun and Its Planetary System P382-395 29. Explain why the frozen debris found in the Oort cloud, more than 50 000 AU away from the Sun, is still considered part of the solar system. ...
... Science 9 Questions: Chapter 11.2 The Sun and Its Planetary System P382-395 29. Explain why the frozen debris found in the Oort cloud, more than 50 000 AU away from the Sun, is still considered part of the solar system. ...
AST101 Lecture 16 Extra Solar Planets
... •1“ (arcsec) = 1/3600 degree As seen from α Centauri (4.3 LY): •Earth is 0.75 arcsec from Sol •Jupiter is 4 arcsec from Sol Can we see this? Yes, but it takes special techniques, and is not easy. ...
... •1“ (arcsec) = 1/3600 degree As seen from α Centauri (4.3 LY): •Earth is 0.75 arcsec from Sol •Jupiter is 4 arcsec from Sol Can we see this? Yes, but it takes special techniques, and is not easy. ...
Chapter 7
... they are made of countless small chunks of ice and rock, each orbiting like a tiny moon. Artist’s conception ...
... they are made of countless small chunks of ice and rock, each orbiting like a tiny moon. Artist’s conception ...
Formation of the solar system
... planets - presumably mostly Fe, Si, O and other "heavier" elements. 3) The asteroids are between Mars and Jupiter - a large (˜2000) group of minor planets. The largest of Ceres (760 km diameter). These are thought to be the source of metoerites 4) The outer planets - Jupiter, Saturn, Uranus, Neptune ...
... planets - presumably mostly Fe, Si, O and other "heavier" elements. 3) The asteroids are between Mars and Jupiter - a large (˜2000) group of minor planets. The largest of Ceres (760 km diameter). These are thought to be the source of metoerites 4) The outer planets - Jupiter, Saturn, Uranus, Neptune ...
Heliocentric Model –The sun is the center of the solar system
... the Sun, planets, and stars orbited a stationary Earth. Copernicus suggested that the Sun was the center of the solar system. Kepler demonstrated that each planet orbited the Sun in an elliptical pattern. ...
... the Sun, planets, and stars orbited a stationary Earth. Copernicus suggested that the Sun was the center of the solar system. Kepler demonstrated that each planet orbited the Sun in an elliptical pattern. ...
ss - PAMS-Doyle
... Diameter= 120,000 km Period of revolution= 29.46 years Period of rotation= 10.5 hours ...
... Diameter= 120,000 km Period of revolution= 29.46 years Period of rotation= 10.5 hours ...
Ch 27 Study Guide
... a. Neptune c. Uranus b. Jupiter d. Saturn ____ 30. The early atmosphere developed when many volcanic eruptions released large amounts of gases in a process called a. lava flow. c. combustion. b. outgassing. d. ozone. ____ 31. Which of the following planets has seasons like Earth’s because its axis t ...
... a. Neptune c. Uranus b. Jupiter d. Saturn ____ 30. The early atmosphere developed when many volcanic eruptions released large amounts of gases in a process called a. lava flow. c. combustion. b. outgassing. d. ozone. ____ 31. Which of the following planets has seasons like Earth’s because its axis t ...
Solar System - wikithurston
... If you moved to Mercury you would way a lot less. If you wayed 70 pounds on Earth you would way 27 pounds on Mercury. It takes Mars 686.98 days to orbit the Sun. Mars excites because its mild temperament is more like the Earth’s than any of the other planets. ...
... If you moved to Mercury you would way a lot less. If you wayed 70 pounds on Earth you would way 27 pounds on Mercury. It takes Mars 686.98 days to orbit the Sun. Mars excites because its mild temperament is more like the Earth’s than any of the other planets. ...
Planets - WordPress.com
... 9. It was discovered by accident while looking for a “Planet X” believed to cause wobbles in the orbits of Uranus and Neptune (It is too small to be Planet X, which may still be out there.). 10. It was discovered in 1930. ...
... 9. It was discovered by accident while looking for a “Planet X” believed to cause wobbles in the orbits of Uranus and Neptune (It is too small to be Planet X, which may still be out there.). 10. It was discovered in 1930. ...
20081 Study Guide_77-120
... 2. No. The scale is too large to show the relative sizes of all the planets. 3. The inner planets are closer together than the outer planets. 4. Most models do not accurately represent both the relative size of and the relative distance between the sun and all of the planets. ...
... 2. No. The scale is too large to show the relative sizes of all the planets. 3. The inner planets are closer together than the outer planets. 4. Most models do not accurately represent both the relative size of and the relative distance between the sun and all of the planets. ...
Definition of planet
The definition of planet, since the word was coined by the ancient Greeks, has included within its scope a wide range of celestial bodies. Greek astronomers employed the term asteres planetai (ἀστέρες πλανῆται), ""wandering stars"", for star-like objects which apparently moved over the sky. Over the millennia, the term has included a variety of different objects, from the Sun and the Moon to satellites and asteroids.By the end of the 19th century the word planet, though it had yet to be defined, had become a working term applied only to a small set of objects in the Solar System. After 1992, however, astronomers began to discover many additional objects beyond the orbit of Neptune, as well as hundreds of objects orbiting other stars. These discoveries not only increased the number of potential planets, but also expanded their variety and peculiarity. Some were nearly large enough to be stars, while others were smaller than Earth's moon. These discoveries challenged long-perceived notions of what a planet could be.The issue of a clear definition for planet came to a head in 2005 with the discovery of the trans-Neptunian object Eris, a body more massive than the smallest then-accepted planet, Pluto. In its 2006 response, the International Astronomical Union (IAU), recognised by astronomers as the world body responsible for resolving issues of nomenclature, released its decision on the matter. This definition, which applies only to the Solar System, states that a planet is a body that orbits the Sun, is massive enough for its own gravity to make it round, and has ""cleared its neighbourhood"" of smaller objects around its orbit. Under this new definition, Pluto and the other trans-Neptunian objects do not qualify as planets. The IAU's decision has not resolved all controversies, and while many scientists have accepted the definition, some in the astronomical community have rejected it outright.