Planetary Science - BPS Science Weebly
... Standard: 9 - Describe lunar and solar eclipses, the observed moon phases, and tides. Relate them to the relative positions of the earth, moon, and sun. Standard: 10 - Compare and contrast properties and conditions of objects in the solar system (i.e., sun, planets, and moons) to those on Earth (i.e ...
... Standard: 9 - Describe lunar and solar eclipses, the observed moon phases, and tides. Relate them to the relative positions of the earth, moon, and sun. Standard: 10 - Compare and contrast properties and conditions of objects in the solar system (i.e., sun, planets, and moons) to those on Earth (i.e ...
Chapter 1
... Revolution – to go around in the orbit. Rotation – to spin around an axis. The Moon revolves once in about 29 days. The Moon rotates once in exactly the same time. We see only one side of the Moon. The side we don’t see is called the “dark side”. ...
... Revolution – to go around in the orbit. Rotation – to spin around an axis. The Moon revolves once in about 29 days. The Moon rotates once in exactly the same time. We see only one side of the Moon. The side we don’t see is called the “dark side”. ...
Unit Lesson Plan – Atomic Structure
... That the motion of an object in orbit is under the influence of gravitational forces How an object’s gravitational field is determined by its size and its mass How to relate the radius of the circle and the speed or rate of revolution of the particle to the magnitude of the centripetal acceler ...
... That the motion of an object in orbit is under the influence of gravitational forces How an object’s gravitational field is determined by its size and its mass How to relate the radius of the circle and the speed or rate of revolution of the particle to the magnitude of the centripetal acceler ...
the brochure
... that it can melt lead. Venus also probably once had oceans but they all boiled away into the atmosphere. ...
... that it can melt lead. Venus also probably once had oceans but they all boiled away into the atmosphere. ...
4-H or - Waushara County UW-Extension
... What does the sun do for us? What does it give us? What shape is the sun? o Round/spherical What color does it look like? o Yellow, but it is actually white How many planets are in the solar system? o 8 – Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune ...
... What does the sun do for us? What does it give us? What shape is the sun? o Round/spherical What color does it look like? o Yellow, but it is actually white How many planets are in the solar system? o 8 – Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune ...
cards for each vacation stop - Morehead Planetarium and Science
... CERES (representing the asteroid belt) — talk about a weight-loss diet 0.01 inches or 0.1 mm on our scale; too small to be included in the kit 1. Ceres is the largest object in the asteroid belt between Mars and Jupiter. Asteroids are “space rubble,” rocky remnants left over from the formation of o ...
... CERES (representing the asteroid belt) — talk about a weight-loss diet 0.01 inches or 0.1 mm on our scale; too small to be included in the kit 1. Ceres is the largest object in the asteroid belt between Mars and Jupiter. Asteroids are “space rubble,” rocky remnants left over from the formation of o ...
Notes: Sun-Earth-Moon System
... region of the solar system along its orbit. All except Mercury and Venus have at least one natural satellite, or moon. • A dwarf planet is an object that orbits the sun and has enough gravity to be spherical, but has not cleared the area of its orbit. • The solar system also includes many smaller ob ...
... region of the solar system along its orbit. All except Mercury and Venus have at least one natural satellite, or moon. • A dwarf planet is an object that orbits the sun and has enough gravity to be spherical, but has not cleared the area of its orbit. • The solar system also includes many smaller ob ...
The Solar System
... Venus is sometimes called Earth’s twin because its size and mass are similar to Earth’s. In 1962, Mariner 2 flew past Venus and sent back information about Venus’s atmosphere and rotation. The former Soviet Union landed the first probe on the surface of Venus in 1970. Venera 7, however, stopped work ...
... Venus is sometimes called Earth’s twin because its size and mass are similar to Earth’s. In 1962, Mariner 2 flew past Venus and sent back information about Venus’s atmosphere and rotation. The former Soviet Union landed the first probe on the surface of Venus in 1970. Venera 7, however, stopped work ...
The Solar System
... Venus is sometimes called Earth’s twin because its size and mass are similar to Earth’s. In 1962, Mariner 2 flew past Venus and sent back information about Venus’s atmosphere and rotation. The former Soviet Union landed the first probe on the surface of Venus in 1970. Venera 7, however, stopped work ...
... Venus is sometimes called Earth’s twin because its size and mass are similar to Earth’s. In 1962, Mariner 2 flew past Venus and sent back information about Venus’s atmosphere and rotation. The former Soviet Union landed the first probe on the surface of Venus in 1970. Venera 7, however, stopped work ...
8th Grade Science Midterm Review Put all answers on a separate
... 48. What is the Universe? A collection of all the galaxies. Universe is also considered to be all of space. 49. What is the reason for the different values of gravity on each planet in our solar system?The planets have different values of gravity based on their mass and their size. The larger the ma ...
... 48. What is the Universe? A collection of all the galaxies. Universe is also considered to be all of space. 49. What is the reason for the different values of gravity on each planet in our solar system?The planets have different values of gravity based on their mass and their size. The larger the ma ...
S-5-6-3_Pluto Graphic Organizer Why Isn`t Pluto a Planet
... Why Isn’t Pluto a Planet? Pluto was called a planet from its discovery in 1930 until it was re-classified as a "dwarf planet" in 2006. The change in status stems from the fact that, since 1993, astronomers have discovered thousands of objects similar to Pluto in size and composition, in the region o ...
... Why Isn’t Pluto a Planet? Pluto was called a planet from its discovery in 1930 until it was re-classified as a "dwarf planet" in 2006. The change in status stems from the fact that, since 1993, astronomers have discovered thousands of objects similar to Pluto in size and composition, in the region o ...
Geology Library Note#391C00.cwk (WP)
... believe the oldest rocks have been destroyed. Lunar rocks have been dated at ~4.55 billion years Meteorites give a similar age. ...
... believe the oldest rocks have been destroyed. Lunar rocks have been dated at ~4.55 billion years Meteorites give a similar age. ...
8th Grade Science Midterm Review Put all answers on a separate
... 48. What is the Universe? A collection of all the galaxies. Universe is also considered to be all of space. 49. What is the reason for the different values of gravity on each planet in our solar system?The planets have different values of gravity based on their mass and their size. The larger the ma ...
... 48. What is the Universe? A collection of all the galaxies. Universe is also considered to be all of space. 49. What is the reason for the different values of gravity on each planet in our solar system?The planets have different values of gravity based on their mass and their size. The larger the ma ...
File
... after Jupiter. It is so big that Earth could fit into it 755 times. It is believed that Saturn’s rings will one day disappear. They will either disperse (spread out) into space or get sucked into the planet by its pull of gravity. This isn't likely to happen anytime soon, more than likely occurring ...
... after Jupiter. It is so big that Earth could fit into it 755 times. It is believed that Saturn’s rings will one day disappear. They will either disperse (spread out) into space or get sucked into the planet by its pull of gravity. This isn't likely to happen anytime soon, more than likely occurring ...
The Solar System, Part I
... because of its color. 21 You can see Mars from Earth, and even without a telescope you can identify it by its reddish tint. The farther you get from the sun, the colder it is and the longer it takes to complete a revolution, or make one trip around the sun. It takes Mars 687 Earth days to revolve ar ...
... because of its color. 21 You can see Mars from Earth, and even without a telescope you can identify it by its reddish tint. The farther you get from the sun, the colder it is and the longer it takes to complete a revolution, or make one trip around the sun. It takes Mars 687 Earth days to revolve ar ...
Life on Earth - pmhsbiologyyr11
... It did NOT prove conclusively however, the origin of life but DID prove it was possible for non-living matter to produce living matter and this Chemosynthetic Origin of Life is believed by most biologists today. ...
... It did NOT prove conclusively however, the origin of life but DID prove it was possible for non-living matter to produce living matter and this Chemosynthetic Origin of Life is believed by most biologists today. ...
Planet Type Information
... loose agrgates of material that have been drawn back together by gravity after the initial object was broken up. Rich in carbon, these bodies are the most similar in composition to the star system's primary sun, and thus represent nearly pristine relics from the formation of that solar system. They ...
... loose agrgates of material that have been drawn back together by gravity after the initial object was broken up. Rich in carbon, these bodies are the most similar in composition to the star system's primary sun, and thus represent nearly pristine relics from the formation of that solar system. They ...
8 Grade/Comp.Sci.III adv Course Code: 2002110
... scientists must use to design an investigation by exploring ways scientists have collected data about stars Identify properties that are common to all hydrogenburning stars (fusion and chemical composition) and properties that may differ (temperature, brightness, and distance from Earth, age, and si ...
... scientists must use to design an investigation by exploring ways scientists have collected data about stars Identify properties that are common to all hydrogenburning stars (fusion and chemical composition) and properties that may differ (temperature, brightness, and distance from Earth, age, and si ...
Astronomy Club
... particles there did not combine to form the planets. Due to large distance from the Sun it should be very cold and like central part of the comets it should be consisting of dust and gases. This flat belt is called 'Couiper Belt'. Couiper assumed that all small period comets emerge from this belt. I ...
... particles there did not combine to form the planets. Due to large distance from the Sun it should be very cold and like central part of the comets it should be consisting of dust and gases. This flat belt is called 'Couiper Belt'. Couiper assumed that all small period comets emerge from this belt. I ...
Missions To Planets In Our
... have suggested that such pits formed by the collapse of subsurface magma chambers. If this suggestion is correct, the pits are evidence of volcanic processes Now, after third flyby, we have a nearly total coverage of Mercury's surface with the exception of the polar-regions at latitudes above 60° N ...
... have suggested that such pits formed by the collapse of subsurface magma chambers. If this suggestion is correct, the pits are evidence of volcanic processes Now, after third flyby, we have a nearly total coverage of Mercury's surface with the exception of the polar-regions at latitudes above 60° N ...
Characteristics Cards KEY
... Size/Mass: 56,900 X 1022 kg Terrestrial or Gas Giant: Gas giant Atmosphere: Thick atmosphere of hydrogen and helium; methane and ammonia also present Physical Properties: Atmosphere of methane and helium, no solid surface, first planet discovered to have rings. The sky gradually turns into liquid un ...
... Size/Mass: 56,900 X 1022 kg Terrestrial or Gas Giant: Gas giant Atmosphere: Thick atmosphere of hydrogen and helium; methane and ammonia also present Physical Properties: Atmosphere of methane and helium, no solid surface, first planet discovered to have rings. The sky gradually turns into liquid un ...
Lecture 14: The Giant Planets, their Moons, and their Rings
... Liquid metallic hydrogen? • Liquid hydrogen: if you poured it into a cup, it would assume the shape of the cup, but would not spread out throughout the entire volume (as would a gas). • Metallic hydrogen: will conduct electricity. • Fact that this layer can flow and can conduct electricity means ...
... Liquid metallic hydrogen? • Liquid hydrogen: if you poured it into a cup, it would assume the shape of the cup, but would not spread out throughout the entire volume (as would a gas). • Metallic hydrogen: will conduct electricity. • Fact that this layer can flow and can conduct electricity means ...
GEOL1010 Hour Exam 1 Sample
... against further observations. Finally the surviving hypothesis becomes the theory that explains the original and subsequent observations. In the case of the origin and age of the Earth, the observations are the many rocks of different radiometric ages and stratigraphic positions. The hypothesis is t ...
... against further observations. Finally the surviving hypothesis becomes the theory that explains the original and subsequent observations. In the case of the origin and age of the Earth, the observations are the many rocks of different radiometric ages and stratigraphic positions. The hypothesis is t ...
Magnetic fields
... Neptune has one moon of interest, Triton. By this distance from the sun, most objects are very cold. Triton is the coldest known body in the solar system at an average temperature of 35 K. Temperatures this cold create some very odd effects. Triton is volcanically active. However, the volcanoes are ...
... Neptune has one moon of interest, Triton. By this distance from the sun, most objects are very cold. Triton is the coldest known body in the solar system at an average temperature of 35 K. Temperatures this cold create some very odd effects. Triton is volcanically active. However, the volcanoes are ...
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.