How is the universe both predictable and unpredictable at the same
... next closest star to us is ______________ light years away. - The light you see from some stars was really given off millions of years ago. B. Astronomical Units - Measures distance between objects in the solar system. - Is the average distance between Earth and the Sun…. about 150 million kilometer ...
... next closest star to us is ______________ light years away. - The light you see from some stars was really given off millions of years ago. B. Astronomical Units - Measures distance between objects in the solar system. - Is the average distance between Earth and the Sun…. about 150 million kilometer ...
8.1 Touring the Night Sky Pg. 308 #1
... 4. Terrestrial planets are the 4 planets closest to the Sun. They have rocky surfaces similar to Earth’s. The next four planets are known as gas giants. They are called that because they are mostly made up of gases and liquids. 5. The difference between stars and planets are; stars are massive colle ...
... 4. Terrestrial planets are the 4 planets closest to the Sun. They have rocky surfaces similar to Earth’s. The next four planets are known as gas giants. They are called that because they are mostly made up of gases and liquids. 5. The difference between stars and planets are; stars are massive colle ...
Lesson #5: Ch 3, Section 3, The Inner Planets
... They have great insight into the solar system and I feel that this project will allow them to dive deeper into the solar system and showcase their skills in two ways instead of a typical exam style assessment. My planning was solid for this and I plan on having a solid discussion and explanation of ...
... They have great insight into the solar system and I feel that this project will allow them to dive deeper into the solar system and showcase their skills in two ways instead of a typical exam style assessment. My planning was solid for this and I plan on having a solid discussion and explanation of ...
Who am I? - Denton ISD
... • Natural or artificial bodies that revolve around more massive bodies such as planets. • Mercury and Venus have no natural satellites called moons. ...
... • Natural or artificial bodies that revolve around more massive bodies such as planets. • Mercury and Venus have no natural satellites called moons. ...
Questions for this book (Word format)
... It took astronomers many years to realise that some of the “fuzzy patches” or “nebulae” in the night sky are actually galaxies like the Milky Way. One reason for this was that only some of the objects catalogued as “nebulae” are actually galaxies. List at least three types of nebula which are not ex ...
... It took astronomers many years to realise that some of the “fuzzy patches” or “nebulae” in the night sky are actually galaxies like the Milky Way. One reason for this was that only some of the objects catalogued as “nebulae” are actually galaxies. List at least three types of nebula which are not ex ...
Earth Science Library wk 1.cwk (WP)
... a. If the predictions are borne out it strengthens our belief in the hypothesis. b. If predictions are not borne out the hypothesis needs to be abandoned or modified. Back to the drawing ...
... a. If the predictions are borne out it strengthens our belief in the hypothesis. b. If predictions are not borne out the hypothesis needs to be abandoned or modified. Back to the drawing ...
Geology 305 with Terry J. Boroughs: The Solar System and the
... D. formation resulting from a collision between the Earth and a Mars- sized body E. none of these 74. The Moon’s composition is: A. Roughly identical to the Earth’s composition B. Completely different than the Earth’s composition C. Similar to but not completely identical nor completely different th ...
... D. formation resulting from a collision between the Earth and a Mars- sized body E. none of these 74. The Moon’s composition is: A. Roughly identical to the Earth’s composition B. Completely different than the Earth’s composition C. Similar to but not completely identical nor completely different th ...
Your Title Here
... •Students will be able to name the eight planets in order from the closest to the sun to the farthest away. •Students will be able to tell at least two facts about each planet. ...
... •Students will be able to name the eight planets in order from the closest to the sun to the farthest away. •Students will be able to tell at least two facts about each planet. ...
FOSS Planetary Science Glossary 1 FOSS Planetary
... Planetary system: A star and the planets, moons, and other objects and materials that orbit that star. Plate tectonics: A theory supported by evidence that Earth’s crust and upper mantle are composed of several thin, relatively rigid plates that move relative to one another, causing earthquakes and ...
... Planetary system: A star and the planets, moons, and other objects and materials that orbit that star. Plate tectonics: A theory supported by evidence that Earth’s crust and upper mantle are composed of several thin, relatively rigid plates that move relative to one another, causing earthquakes and ...
Students make a distance-scale solar system model with toilet paper.
... planets in our solar system. Voyager II, traveling at nearly 50,000 mph took 12 years to reach the planet Neptune. We can make a scale model of the distances between the planets using almost anything as our reference. In doing so, we may be able to determine a variety of ways to classify the planets ...
... planets in our solar system. Voyager II, traveling at nearly 50,000 mph took 12 years to reach the planet Neptune. We can make a scale model of the distances between the planets using almost anything as our reference. In doing so, we may be able to determine a variety of ways to classify the planets ...
CHAPTER 1 Planets of the Solar System
... Since the time of Copernicus, Kepler, and Galileo, we have learned a lot more about our solar system. Astronomers have discovered two more planets (Uranus and Neptune), five dwarf planets (Ceres, Pluto, Makemake, Haumea, and Eris), more than 150 moons, and many, many asteroids and other small object ...
... Since the time of Copernicus, Kepler, and Galileo, we have learned a lot more about our solar system. Astronomers have discovered two more planets (Uranus and Neptune), five dwarf planets (Ceres, Pluto, Makemake, Haumea, and Eris), more than 150 moons, and many, many asteroids and other small object ...
Planets and Moons - Fraser Heights Chess Club
... light, they travel MUCH slower. The Apollo missions took 4 days to reach the Moon - at the speed of light it would have taken 2 seconds!! These rockets were travelling roughly 200,000 times slower than light. At this speed it would take 125 YEARS to get to Pluto! ...
... light, they travel MUCH slower. The Apollo missions took 4 days to reach the Moon - at the speed of light it would have taken 2 seconds!! These rockets were travelling roughly 200,000 times slower than light. At this speed it would take 125 YEARS to get to Pluto! ...
CHAPTER 1 Planets of the Solar System
... Since the time of Copernicus, Kepler, and Galileo, we have learned a lot more about our solar system. Astronomers have discovered two more planets (Uranus and Neptune), five dwarf planets (Ceres, Pluto, Makemake, Haumea, and Eris), more than 150 moons, and many, many asteroids and other small object ...
... Since the time of Copernicus, Kepler, and Galileo, we have learned a lot more about our solar system. Astronomers have discovered two more planets (Uranus and Neptune), five dwarf planets (Ceres, Pluto, Makemake, Haumea, and Eris), more than 150 moons, and many, many asteroids and other small object ...
Unit 2 Study Guide - Grant County Schools
... Planets are in constant motion. The two motions that all planets do is rotate and revolve. A rotation is one spin of a planet on its axis. As the planet spins half of the planet is facing the sun and the other half is facing away. The lit side is day and the dark side is night. The spinning of the p ...
... Planets are in constant motion. The two motions that all planets do is rotate and revolve. A rotation is one spin of a planet on its axis. As the planet spins half of the planet is facing the sun and the other half is facing away. The lit side is day and the dark side is night. The spinning of the p ...
Unit 2 Study Guide (word)
... Planets are in constant motion. The two motions that all planets do is rotate and revolve. A rotation is one spin of a planet on its axis. As the planet spins half of the planet is facing the sun and the other half is facing away. The lit side is day and the dark side is night. The spinning of the p ...
... Planets are in constant motion. The two motions that all planets do is rotate and revolve. A rotation is one spin of a planet on its axis. As the planet spins half of the planet is facing the sun and the other half is facing away. The lit side is day and the dark side is night. The spinning of the p ...
Testing
... Which of these facts is NOT explained by the nebular theory? • There are two main types of planets: terrestrial and jovian. • Planets orbit in the same direction and plane. • Asteroids and comets exist. • There are four terrestrial and four jovian planets. ...
... Which of these facts is NOT explained by the nebular theory? • There are two main types of planets: terrestrial and jovian. • Planets orbit in the same direction and plane. • Asteroids and comets exist. • There are four terrestrial and four jovian planets. ...
Our Place in Space
... Group 4: Astronomers finally learned that Earth is one of at least eight other planets that travel around the Sun. Group 5: The Sun is a star at the center of the Solar System. It isn’t the biggest or the brightest star in our galaxy, but it is the star closest to Earth. Group 1: It is the largest b ...
... Group 4: Astronomers finally learned that Earth is one of at least eight other planets that travel around the Sun. Group 5: The Sun is a star at the center of the Solar System. It isn’t the biggest or the brightest star in our galaxy, but it is the star closest to Earth. Group 1: It is the largest b ...
Contact: Sharon Worthy
... and farthest from the sun, it’s never been visited by one of our space probes. Although it does have one moon, some people still think it should be considered a big asteroid instead of a planet! Since it was discovered in 1930, scientists have learned that Pluto has an odd elliptical orbit, which at ...
... and farthest from the sun, it’s never been visited by one of our space probes. Although it does have one moon, some people still think it should be considered a big asteroid instead of a planet! Since it was discovered in 1930, scientists have learned that Pluto has an odd elliptical orbit, which at ...
Document
... Cratering on planets and satellites is the result of impacts from interplanetary debris • When an asteroid, comet, or meteoroid collides with the surface of a terrestrial planet or satellite, the result is an impact crater • Geologic activity renews the surface and erases craters, so a terrestrial ...
... Cratering on planets and satellites is the result of impacts from interplanetary debris • When an asteroid, comet, or meteoroid collides with the surface of a terrestrial planet or satellite, the result is an impact crater • Geologic activity renews the surface and erases craters, so a terrestrial ...
The Milky Way
... The solar wind, a flow of plasma from the Sun, creates a bubble in the interstellar medium known as the heliosphere, which extends out to the edge of the scattered disc. The hypothetical Oort cloud, which acts as the source for long-period comets, may also exist at a distance roughly a thousand time ...
... The solar wind, a flow of plasma from the Sun, creates a bubble in the interstellar medium known as the heliosphere, which extends out to the edge of the scattered disc. The hypothetical Oort cloud, which acts as the source for long-period comets, may also exist at a distance roughly a thousand time ...
No Slide Title
... radius a and albedo A orbiting the Sun at a distance of r A.U. from it. Albedo = fraction of incident light reflected. The radiance at the Sun’s surface is σT4 where T = 5779 K. The surface area of the Sun is 4πR2, so the total emergent radiant flux from the Sun is = 4πRσT4. At a distance r from ...
... radius a and albedo A orbiting the Sun at a distance of r A.U. from it. Albedo = fraction of incident light reflected. The radiance at the Sun’s surface is σT4 where T = 5779 K. The surface area of the Sun is 4πR2, so the total emergent radiant flux from the Sun is = 4πRσT4. At a distance r from ...
Merit - NZQA
... hydrogen fuel. To fuse He → C their core had to collapse and their outer layers expanded outwards. This means red giants have a large surface area but a low temperature range of ...
... hydrogen fuel. To fuse He → C their core had to collapse and their outer layers expanded outwards. This means red giants have a large surface area but a low temperature range of ...
Late Heavy Bombardment
The Late Heavy Bombardment (abbreviated LHB and also known as the lunar cataclysm) is a hypothetical event thought to have occurred approximately 4.1 to 3.8 billion years (Ga) ago, corresponding to the Neohadean and Eoarchean eras on Earth. During this interval, a disproportionately large number of asteroids apparently collided with the early terrestrial planets in the inner Solar System, including Mercury, Venus, Earth, and Mars. The LHB happened after the Earth and other rocky planets had formed and accreted most of their mass, but still quite early in Earth's history.Evidence for the LHB derives from lunar samples brought back by the Apollo astronauts. Isotopic dating of Moon rocks implies that most impact melts occurred in a rather narrow interval of time. Several hypotheses are now offered to explain the apparent spike in the flux of impactors (i.e. asteroids and comets) in the inner Solar System, but no consensus yet exists. The Nice model is popular among planetary scientists; it postulates that the gas giant planets underwent orbital migration and scattered objects in the asteroid and/or Kuiper belts into eccentric orbits, and thereby into the path of the terrestrial planets. Other researchers argue that the lunar sample data do not require a cataclysmic cratering event near 3.9 Ga, and that the apparent clustering of impact melt ages near this time is an artifact of sampling materials retrieved from a single large impact basin. They also note that the rate of impact cratering could be significantly different between the outer and inner zones of the Solar System.