Geology 305 with Terry J. Boroughs: The Solar System and the
... B. geologic processes we observe today have operated similarly in the past C. early Earth was covered by a uniform magma ocean ...
... B. geologic processes we observe today have operated similarly in the past C. early Earth was covered by a uniform magma ocean ...
Evolution of the Solar System and Planets Homework
... was not the correct model of the solar system) because it was able to predict the approximate position of the major objects (Moon, etc.) in the night-time sky. 83. The Universe is approximately 14 Billion years old. 84. The current theory on the origin of the solar system states that the major plane ...
... was not the correct model of the solar system) because it was able to predict the approximate position of the major objects (Moon, etc.) in the night-time sky. 83. The Universe is approximately 14 Billion years old. 84. The current theory on the origin of the solar system states that the major plane ...
ppt
... Neptune was discovered in 1846. Is it easy to see and identify Uranus and Neptune as planets? Why or why not? How are they identified as planets? ...
... Neptune was discovered in 1846. Is it easy to see and identify Uranus and Neptune as planets? Why or why not? How are they identified as planets? ...
Planets - Digitalis Education
... will help you find your directions: Polaris, the north star. Allow a student to point out the Big Dipper with a light pointer, then show how to use the 'pointer stars' to find Polaris. Review the other directions and display the cardinal points. B) One difference between stars and planets is that st ...
... will help you find your directions: Polaris, the north star. Allow a student to point out the Big Dipper with a light pointer, then show how to use the 'pointer stars' to find Polaris. Review the other directions and display the cardinal points. B) One difference between stars and planets is that st ...
Comets, Meteors, and Asteroids
... Very few comets enter inner solar system; most stay far from Sun. Kuiper belt: In orderly orbits from 30–100 AU in disk of solar system Oort cloud: In random orbits extending to about 50,000 AU ...
... Very few comets enter inner solar system; most stay far from Sun. Kuiper belt: In orderly orbits from 30–100 AU in disk of solar system Oort cloud: In random orbits extending to about 50,000 AU ...
Project Pan-STARRS and the Outer Solar System - UCLA
... Jupiter maintains a large population of Trojans (bodies sharing Jupiter’s orbit but circulating ± 60 deg. from the planet in longitude at the L4 and L5 Lagrangian points). More than 1600 are known as of May 2003 but the total population is far larger. When measured down to diameters D ∼1 km, the num ...
... Jupiter maintains a large population of Trojans (bodies sharing Jupiter’s orbit but circulating ± 60 deg. from the planet in longitude at the L4 and L5 Lagrangian points). More than 1600 are known as of May 2003 but the total population is far larger. When measured down to diameters D ∼1 km, the num ...
Sec 28.4 - Highland High School
... Since its discovery by Clyde Tombaugh in 1930, Pluto has been an unusual planet. It is not a terrestrial or gas planet; it is made of rock and ice. ...
... Since its discovery by Clyde Tombaugh in 1930, Pluto has been an unusual planet. It is not a terrestrial or gas planet; it is made of rock and ice. ...
Document
... The planets, in order from closest to farthest from the sun: Mercury These five were known Venus and Earth observed by Mars ancient Jupiter cultures Saturn Uranus Neptune dwarf planets: Pluto, Eris ...
... The planets, in order from closest to farthest from the sun: Mercury These five were known Venus and Earth observed by Mars ancient Jupiter cultures Saturn Uranus Neptune dwarf planets: Pluto, Eris ...
The Dwarf Planets
... While we can't see most of the objects in the Kuiper belt well enough to determine whether they are round or not, we can estimate how big an object has to be before it becomes round and therefore how many objects in the Kuiper belt are likely round. In the asteroid belt Ceres, with a diameter of 900 ...
... While we can't see most of the objects in the Kuiper belt well enough to determine whether they are round or not, we can estimate how big an object has to be before it becomes round and therefore how many objects in the Kuiper belt are likely round. In the asteroid belt Ceres, with a diameter of 900 ...
models of the solar system
... 6. Fit & tape them into the “aphelion” side of the ellipse. B. Conclusion Questions: 1. These 2 pie slices are equal in area even though they are different shapes (FAT slice and skinny slice). This means that the closer the planet is to the sun the (greater or smaller) the distance it must travel in ...
... 6. Fit & tape them into the “aphelion” side of the ellipse. B. Conclusion Questions: 1. These 2 pie slices are equal in area even though they are different shapes (FAT slice and skinny slice). This means that the closer the planet is to the sun the (greater or smaller) the distance it must travel in ...
Student Activity: Comparing the Sizes of Planets and Their
... Students should know the order of the planets before starting this activity. If necessary, teach them a mnemonic, such as My Velvet Elephant Munches... In this activity the Sun is placed at one end of the field and the planets are arranged linearly. Discuss with students that this is not an accurate ...
... Students should know the order of the planets before starting this activity. If necessary, teach them a mnemonic, such as My Velvet Elephant Munches... In this activity the Sun is placed at one end of the field and the planets are arranged linearly. Discuss with students that this is not an accurate ...
docx - STAO
... Students should know the order of the planets before starting this activity. If necessary, teach them a mnemonic, such as My Velvet Elephant Munches... In this activity the Sun is placed at one end of the field and the planets are arranged linearly. Discuss with students that this is not an accurate ...
... Students should know the order of the planets before starting this activity. If necessary, teach them a mnemonic, such as My Velvet Elephant Munches... In this activity the Sun is placed at one end of the field and the planets are arranged linearly. Discuss with students that this is not an accurate ...
File
... Comparing the Terrestrial and Jovian Planets Terrestrial planets are the first 4 planets. Their surfaces are solid and they are referred to as the “rocky” planets. Jovian planets are the outer 4 planets. Their surfaces are gas and often have frozen cores and are referred to as the “gas giants.” The ...
... Comparing the Terrestrial and Jovian Planets Terrestrial planets are the first 4 planets. Their surfaces are solid and they are referred to as the “rocky” planets. Jovian planets are the outer 4 planets. Their surfaces are gas and often have frozen cores and are referred to as the “gas giants.” The ...
Patterns in the Solar System
... Comparing the Terrestrial and Jovian Planets Terrestrial planets are the first 4 planets. Their surfaces are solid and they are referred to as the “rocky” planets. Jovian planets are the outer 4 planets. Their surfaces are gas and often have frozen cores and are referred to as the “gas giants.” The ...
... Comparing the Terrestrial and Jovian Planets Terrestrial planets are the first 4 planets. Their surfaces are solid and they are referred to as the “rocky” planets. Jovian planets are the outer 4 planets. Their surfaces are gas and often have frozen cores and are referred to as the “gas giants.” The ...
Introduction
... simultaneous thorium-argon lamp observation (see, e.g., Konacki et al. 2003c) and an Iodine absorption cell (see, e.g., Cumming, Marcy, & Butler 1999 and references therein). While the Iodine cell is placed into the path of the star signal, before entering the spectrograph (and thus reducing the sig ...
... simultaneous thorium-argon lamp observation (see, e.g., Konacki et al. 2003c) and an Iodine absorption cell (see, e.g., Cumming, Marcy, & Butler 1999 and references therein). While the Iodine cell is placed into the path of the star signal, before entering the spectrograph (and thus reducing the sig ...
Mercury
... One of Mercury's largest features is called the Caloris Basin. It is about 1300 km across! It was probably created by a very large crash early in the history of the solar system. You can see Mercury with a pair of binoculars or even the naked eye. Because it is always very near the Sun, Mercury may ...
... One of Mercury's largest features is called the Caloris Basin. It is about 1300 km across! It was probably created by a very large crash early in the history of the solar system. You can see Mercury with a pair of binoculars or even the naked eye. Because it is always very near the Sun, Mercury may ...
\(309239\) 2007 RW10: a large temporary quasi
... around 0◦ we have the quasi-satellite state, this is a specific configuration of a 1:1 mean motion resonance, one in which the body librates around the mean longitude of its associated planet; the minor planet orbits the Sun in an approximate ellipse with the same (mean) period as the planet. When v ...
... around 0◦ we have the quasi-satellite state, this is a specific configuration of a 1:1 mean motion resonance, one in which the body librates around the mean longitude of its associated planet; the minor planet orbits the Sun in an approximate ellipse with the same (mean) period as the planet. When v ...
Solutions
... Suppose someone claimed to make the discoveries described below. (These are not real discoveries.) Decide whether each discovery should be considered reasonable or surprising. Explain clearly; not all these have definitive answers, so your explanation is more important than your chosen answer. 19. A ...
... Suppose someone claimed to make the discoveries described below. (These are not real discoveries.) Decide whether each discovery should be considered reasonable or surprising. Explain clearly; not all these have definitive answers, so your explanation is more important than your chosen answer. 19. A ...
Comparative Planetology I: Our Solar System Chapter Seven
... from the same cloud of interstellar gas and dust The composition of this cloud was shaped by cosmic processes, including nuclear reactions that took place within stars that died long ...
... from the same cloud of interstellar gas and dust The composition of this cloud was shaped by cosmic processes, including nuclear reactions that took place within stars that died long ...
Powerpoint Presentation (large file)
... from the same cloud of interstellar gas and dust • The composition of this cloud was shaped by cosmic processes, including nuclear reactions that took place within stars that died long ...
... from the same cloud of interstellar gas and dust • The composition of this cloud was shaped by cosmic processes, including nuclear reactions that took place within stars that died long ...
Constructing the Solar System: A Smashing Success!
... Asteroids are bodies that formed in the early Solar System, and are likely to represent planetesimals that survived the period of planet building and are still in orbit around the Sun today. Most asteroids are found in orbits between Mars and Jupiter (although some are on Earth-crossing orbits, and ...
... Asteroids are bodies that formed in the early Solar System, and are likely to represent planetesimals that survived the period of planet building and are still in orbit around the Sun today. Most asteroids are found in orbits between Mars and Jupiter (although some are on Earth-crossing orbits, and ...
ECCENTRICITY PRACTICE
... of revolution? A) Gravitational pull would decrease and period of revolution would increase. B) Gravitational pull would decrease and period of revolution would decrease. C) Gravitational pull would increase and period of revolution would increase. D) Gravitational pull would increase and period of ...
... of revolution? A) Gravitational pull would decrease and period of revolution would increase. B) Gravitational pull would decrease and period of revolution would decrease. C) Gravitational pull would increase and period of revolution would increase. D) Gravitational pull would increase and period of ...
Neptune
... • Orbiting the Sun: 164.79 years to orbit the sun • On its own axis: it takes 16Earth hours to rotate on its own axis ...
... • Orbiting the Sun: 164.79 years to orbit the sun • On its own axis: it takes 16Earth hours to rotate on its own axis ...
The Outer Planets - Amazon Web Services
... and helium. Because they are so massive, the gas giants exert a much stronger gravitational force than the terrestrial planets. Gravity keeps the giant planets' gases from escaping, so they have thick atmospheres. Despite the name "gas giant," much of the hydrogen and helium is actually in liquid fo ...
... and helium. Because they are so massive, the gas giants exert a much stronger gravitational force than the terrestrial planets. Gravity keeps the giant planets' gases from escaping, so they have thick atmospheres. Despite the name "gas giant," much of the hydrogen and helium is actually in liquid fo ...