student worksheet with reading
... nebula’ – some 4.6 billion years ago. All of the parts of the solar system are considered to be of similar age. Because this nebula was spinning as it collapsed, all of its major components co-exist on a relatively flat plane (the ecliptic). The Moon and planets can always be found in a narrow band ...
... nebula’ – some 4.6 billion years ago. All of the parts of the solar system are considered to be of similar age. Because this nebula was spinning as it collapsed, all of its major components co-exist on a relatively flat plane (the ecliptic). The Moon and planets can always be found in a narrow band ...
ppt
... All planets orbit the Sun in same sense. The Sun and all planets (apart from Venus, Uranus, & Pluto) rotate in the same sense as they orbit the Sun. Inner planets are small and rocky, but outer planets are large and gaseous. There are also asteroids and comets ...
... All planets orbit the Sun in same sense. The Sun and all planets (apart from Venus, Uranus, & Pluto) rotate in the same sense as they orbit the Sun. Inner planets are small and rocky, but outer planets are large and gaseous. There are also asteroids and comets ...
Lesson 4d Models of the Solar System
... Ptolemy’s (AD 85 – 165) adaption of Aristotle’s ideas To explain the retrograde motion of some planets, he allowed each planet to move in a small circle (an epicycle) The centre of the epicycle moved on a bigger circle called a deferent. Earth is still at the centre (geocentric) ...
... Ptolemy’s (AD 85 – 165) adaption of Aristotle’s ideas To explain the retrograde motion of some planets, he allowed each planet to move in a small circle (an epicycle) The centre of the epicycle moved on a bigger circle called a deferent. Earth is still at the centre (geocentric) ...
Regents Review Questions.Unit 2.Astronomy
... Astronomers have discovered more than 400 planets outside of our solar system. The first extrasolar planet was detected in 1995 orbiting a star known as 51 Pegasi, which is similar in color and luminosity to our Sun. Astronomers can detect planets by identifying stars that move in response to the gr ...
... Astronomers have discovered more than 400 planets outside of our solar system. The first extrasolar planet was detected in 1995 orbiting a star known as 51 Pegasi, which is similar in color and luminosity to our Sun. Astronomers can detect planets by identifying stars that move in response to the gr ...
What can we learn by comparing the planets to one another?
... – Venus: Same size as Earth but much hotter – Earth: Only planet with liquid water on surface – Mars: Could have had liquid water in past – Jupiter: A gaseous giant – Saturn: Gaseous with spectacular rings – Uranus: A gas giant with a highly tilted axis – Neptune: Similar to Uranus but with normal a ...
... – Venus: Same size as Earth but much hotter – Earth: Only planet with liquid water on surface – Mars: Could have had liquid water in past – Jupiter: A gaseous giant – Saturn: Gaseous with spectacular rings – Uranus: A gas giant with a highly tilted axis – Neptune: Similar to Uranus but with normal a ...
Chapter 7 Our Planetary System
... Earth by studying in context with other worlds in the solar system. Stay focused on processes common to multiple worlds instead of individual facts specific to a particular world. ...
... Earth by studying in context with other worlds in the solar system. Stay focused on processes common to multiple worlds instead of individual facts specific to a particular world. ...
Power Functions
... their distances from the sun, and the respective number of days for one complete revolution around the sun. Use the capabilities of your GC to determine a power function model for a planet’s distance (x) versus the number of days in the planet’s orbit (y). ...
... their distances from the sun, and the respective number of days for one complete revolution around the sun. Use the capabilities of your GC to determine a power function model for a planet’s distance (x) versus the number of days in the planet’s orbit (y). ...
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 ...
Document
... Jupiter is named after the Roman king of the Gods. It would take 11 earths lined up next to each other to get from one side of Jupiter to the other, it would also take 317 earths to equal Jupiter's mass. Jupiter's red spot is a gigantic storm that has been there for over 300 years! If Jupiter had 80 ...
... Jupiter is named after the Roman king of the Gods. It would take 11 earths lined up next to each other to get from one side of Jupiter to the other, it would also take 317 earths to equal Jupiter's mass. Jupiter's red spot is a gigantic storm that has been there for over 300 years! If Jupiter had 80 ...
02 - University of New Mexico
... Earth is due to the Earth’s rotation. 7. Retrograde motion of planets is due to Earth’s motion around the Sun. ...
... Earth is due to the Earth’s rotation. 7. Retrograde motion of planets is due to Earth’s motion around the Sun. ...
Document
... Rocks on Earth ~ 4 billion years Rocks on moon ~ 4 billion years Meteorites ~ 4 billion years ...
... Rocks on Earth ~ 4 billion years Rocks on moon ~ 4 billion years Meteorites ~ 4 billion years ...
Life on Billions of Planets
... themselves are so dim. With so many M-dwarfs right around the cosmic corner, however, and with so many relatively small planets orbiting in their habitable zones, the job will be orders of magnitude easier. That's the good news. But there are a few caveats as well. For one thing, it's not guaranteed ...
... themselves are so dim. With so many M-dwarfs right around the cosmic corner, however, and with so many relatively small planets orbiting in their habitable zones, the job will be orders of magnitude easier. That's the good news. But there are a few caveats as well. For one thing, it's not guaranteed ...
Planet - Tasker Milward Physics Website
... together to make Helium. Lots of energy is released in the process as heat and light. ...
... together to make Helium. Lots of energy is released in the process as heat and light. ...
NAME - wths
... 19) What three reasons are given as to the difference between the Jovian planets and the terrestrial planets? ...
... 19) What three reasons are given as to the difference between the Jovian planets and the terrestrial planets? ...
Quiz #1 - UCLA - Earth, Planetary, and Space Sciences
... 1. List the planets in the Solar System (8 points + 2 points if you get them in order from closest to furthest from the Sun.) ...
... 1. List the planets in the Solar System (8 points + 2 points if you get them in order from closest to furthest from the Sun.) ...
Spaceship Earth
... the center of the Milky Way galaxy once every 2.3x108 years. Speed ~ 8x105 km/hr. • The Milky Way is moving toward the Andromeda galaxy, speed ~ 3x105 km/hr • The Milky Way (along with the local group) partakes in the expansion of the universe. ...
... the center of the Milky Way galaxy once every 2.3x108 years. Speed ~ 8x105 km/hr. • The Milky Way is moving toward the Andromeda galaxy, speed ~ 3x105 km/hr • The Milky Way (along with the local group) partakes in the expansion of the universe. ...
History of Astronomy
... Explained apparent motion of stars and sun using Earth’s rotation and orbit Explained why Mercury and Venus are always seen near the Sun Invented idea of Astronomical Unit (A.U.) – Distance of Earth from the Sun (About 93 million ...
... Explained apparent motion of stars and sun using Earth’s rotation and orbit Explained why Mercury and Venus are always seen near the Sun Invented idea of Astronomical Unit (A.U.) – Distance of Earth from the Sun (About 93 million ...
PPT
... A few words about the Sun. The Sun is a large sphere of gas (mostly H, He – hydrogen and helium). The Sun shines because it is hot (T = 5,800 K). The Sun remains hot because it is powered by fusion of hydrogen to helium (H-bomb). ...
... A few words about the Sun. The Sun is a large sphere of gas (mostly H, He – hydrogen and helium). The Sun shines because it is hot (T = 5,800 K). The Sun remains hot because it is powered by fusion of hydrogen to helium (H-bomb). ...
ASTRONOMY 161
... A few words about the Sun. The Sun is a large sphere of gas (mostly H, He – hydrogen and helium). The Sun shines because it is hot (T = 5,800 K). The Sun remains hot because it is powered by fusion of hydrogen to helium (H-bomb). ...
... A few words about the Sun. The Sun is a large sphere of gas (mostly H, He – hydrogen and helium). The Sun shines because it is hot (T = 5,800 K). The Sun remains hot because it is powered by fusion of hydrogen to helium (H-bomb). ...
Solar System Quiz
... ____ 14. The two inner planets most alike in size, mass, and density are a. Mercury and Venus. c. Venus and Earth. b. Earth and Mars. d. Mars and Mercury. ____ 15. Many comets in the Kuiper belt are the result of a. meteor showers. c. collisions between large objects. b. inertia. d. Saturn’s gravita ...
... ____ 14. The two inner planets most alike in size, mass, and density are a. Mercury and Venus. c. Venus and Earth. b. Earth and Mars. d. Mars and Mercury. ____ 15. Many comets in the Kuiper belt are the result of a. meteor showers. c. collisions between large objects. b. inertia. d. Saturn’s gravita ...
Planet Characteristics - Red Hook Central Schools
... carbon dioxide. Mars has two small moons. ...
... carbon dioxide. Mars has two small moons. ...
Orrery
An orrery is a mechanical model of the solar system that illustrates or predicts the relative positions and motions of the planets and moons, usually according to the heliocentric model. It may also represent the relative sizes of these bodies; but since accurate scaling is often not practical due to the actual large ratio differences, a subdued approximation may be used instead. Though the Greeks had working planetaria, the first orrery that was a planetarium of the modern era was produced in 1704, and one was presented to Charles Boyle, 4th Earl of Orrery — whence came the name. They are typically driven by a clockwork mechanism with a globe representing the Sun at the centre, and with a planet at the end of each of the arms.