Chapter 24 Vocabulary link - Flushing Community Schools
... Some planets’ moons storms that reveal may be one of these that was pulled from an active and rapidly the belt. Their sizes changing atmosphere, range from very tiny it has 11 moons, and pinkish Triton is the to 940 km in largest. diameter. ...
... Some planets’ moons storms that reveal may be one of these that was pulled from an active and rapidly the belt. Their sizes changing atmosphere, range from very tiny it has 11 moons, and pinkish Triton is the to 940 km in largest. diameter. ...
Vagabonds of the Solar System
... that we see today • Combining all the asteroids would produce an object of only 1500 km in diameter ...
... that we see today • Combining all the asteroids would produce an object of only 1500 km in diameter ...
exercise 3
... Nine major planets are currently known. They are commonly divided into two groups: the inner planets (Mercury, Venus, Earth, and Mars) and the outer planets (Jupiter, Saturn, Uranus, and Neptune). The inner planets are small and are composed primarily of rock and iron. The outer planets are much lar ...
... Nine major planets are currently known. They are commonly divided into two groups: the inner planets (Mercury, Venus, Earth, and Mars) and the outer planets (Jupiter, Saturn, Uranus, and Neptune). The inner planets are small and are composed primarily of rock and iron. The outer planets are much lar ...
Solar System Diagnostic
... school to jot down your thoughts on the following questions. Even if you only know a little about something but it may not make full sense please jot it down. This paper will not be graded, but I will read it to better understand your knowledge coming into this topic. It will help me to know which a ...
... school to jot down your thoughts on the following questions. Even if you only know a little about something but it may not make full sense please jot it down. This paper will not be graded, but I will read it to better understand your knowledge coming into this topic. It will help me to know which a ...
Chapter 29 Our Solar System
... is the planet most similar to Earth in physical properties, such as diameter, mass, and density. ...
... is the planet most similar to Earth in physical properties, such as diameter, mass, and density. ...
NAME ______ PERIOD ______ DATE_________ OGT Practice
... NAME _____________ PERIOD _______ DATE_________ OGT Practice QUIZ #8 ...
... NAME _____________ PERIOD _______ DATE_________ OGT Practice QUIZ #8 ...
Why is Pluto no longer a planet
... smaller than Pluto, or in Eris’s case, larger. If Pluto remained as a planet many other subjects would have to be declared planets as well, including Ceres. The only eight planets that meet these requirements are the ones from Mercury to Neptune. In July 2005 a group of astronomers have discovered a ...
... smaller than Pluto, or in Eris’s case, larger. If Pluto remained as a planet many other subjects would have to be declared planets as well, including Ceres. The only eight planets that meet these requirements are the ones from Mercury to Neptune. In July 2005 a group of astronomers have discovered a ...
Motions of the Planets
... Mercury and Venus are colloquially referred to as morning or evening “stars”. Both planets appear at dusk or dawn, when they can be easily seen against the dim sky. During the day, Venus is visible, if you know exactly where to look. ...
... Mercury and Venus are colloquially referred to as morning or evening “stars”. Both planets appear at dusk or dawn, when they can be easily seen against the dim sky. During the day, Venus is visible, if you know exactly where to look. ...
Astronomy Review (Cope) 64KB Jun 09 2013 08:13:01 PM
... 18. Starting with the speed of light being 3.00 x 10 meters per second (or 300,000 km per second), calculate how far light will travel in one (365 day) year. Stars ...
... 18. Starting with the speed of light being 3.00 x 10 meters per second (or 300,000 km per second), calculate how far light will travel in one (365 day) year. Stars ...
8thGrCh4.3-4.5Outline
... Scientists classify small objects in the solar system based on their _______________, _______________, _______________________, and _______________. The major categories include _________________, _____________, ___________________, and ___________________. Areas of the Solar System: Most of the sma ...
... Scientists classify small objects in the solar system based on their _______________, _______________, _______________________, and _______________. The major categories include _________________, _____________, ___________________, and ___________________. Areas of the Solar System: Most of the sma ...
Lauren Stinson
... • 4 more moons were found in late 2000 and 9 more were discovered recently with a total of 31 moons ...
... • 4 more moons were found in late 2000 and 9 more were discovered recently with a total of 31 moons ...
pdf format
... • Be influenced by gravity of planets • impact the planet: e.g. Comet Shoemaker-Levy hit Jupiter in 1994; perhaps comets were source of water on Earth. • be speeded up & ejected to outer solar system or even from solar system • be perturbed into an orbit with a shorter period – each time it approach ...
... • Be influenced by gravity of planets • impact the planet: e.g. Comet Shoemaker-Levy hit Jupiter in 1994; perhaps comets were source of water on Earth. • be speeded up & ejected to outer solar system or even from solar system • be perturbed into an orbit with a shorter period – each time it approach ...
Some SOLAR SYSTEM notes
... accumulated to form the Sun. But because dust is denser than gas, some of the dust settled to the mid-plane of the disc. These dust particles stuck together to make clumps, then clumps stuck together to make rocks, then rocks collided to make planets. In the case of the `gas giant' planets, Jupiter, ...
... accumulated to form the Sun. But because dust is denser than gas, some of the dust settled to the mid-plane of the disc. These dust particles stuck together to make clumps, then clumps stuck together to make rocks, then rocks collided to make planets. In the case of the `gas giant' planets, Jupiter, ...
Section 1: Planetary Motion Rotation – the spinning of a body on its
... When part of the ocean is directly facing the moon, the water there bulges toward the moon. Tidal Range – is the difference between levels of ocean water at high and low tide Spring Tides – are tides with the largest daily tidal range: occur during new and full moons Neap Tides – are tides with the ...
... When part of the ocean is directly facing the moon, the water there bulges toward the moon. Tidal Range – is the difference between levels of ocean water at high and low tide Spring Tides – are tides with the largest daily tidal range: occur during new and full moons Neap Tides – are tides with the ...
Chapter 6 Study Guide
... 11. What type of energy powers the sun? _________________________________________ 12. Who discovered gravity? _____________________________________________ 13. What is the difference between mass and weight? ___________________________________ _______________________________________________________ ...
... 11. What type of energy powers the sun? _________________________________________ 12. Who discovered gravity? _____________________________________________ 13. What is the difference between mass and weight? ___________________________________ _______________________________________________________ ...
inner planets
... The Earth needs one year to make one complete orbit around the Sun. 3. How long does Uranus need to orbit the Sun? Uranus needs 83.7 years to orbit around the Sun. 4. How long does the Earth need to complete one rotation? The Earth needs one day to complete one rotation. 5. How long does it take for ...
... The Earth needs one year to make one complete orbit around the Sun. 3. How long does Uranus need to orbit the Sun? Uranus needs 83.7 years to orbit around the Sun. 4. How long does the Earth need to complete one rotation? The Earth needs one day to complete one rotation. 5. How long does it take for ...
Planetary Science Vocabulary #2 1. Asteroids Objects made of rock
... Planetary Science Vocabulary #2 1. Asteroids ...
... Planetary Science Vocabulary #2 1. Asteroids ...
File
... Minor Members of the Solar System Today you will learn: 1. What other objects, besides the planets, orbit around the sun. ...
... Minor Members of the Solar System Today you will learn: 1. What other objects, besides the planets, orbit around the sun. ...
Exploring Space What’s Out There?
... travels around a star • Orbit = the path that a celestial object takes around another object • Solar system = the sun and all the celestial objects that travel around it ...
... travels around a star • Orbit = the path that a celestial object takes around another object • Solar system = the sun and all the celestial objects that travel around it ...
Study Guide Our Solar System Student Note: The upcoming test on
... Dwarf planets orbit the sun and have enough gravity to pull themselves into spheres but they have other objects in the areas of their orbits. There are five known dwarf planets, including Pluto. Except Cere, all dwarf planets orbit beyond Neptune. ...
... Dwarf planets orbit the sun and have enough gravity to pull themselves into spheres but they have other objects in the areas of their orbits. There are five known dwarf planets, including Pluto. Except Cere, all dwarf planets orbit beyond Neptune. ...
Chapter 21
... • Moon is small, low mass so it rapidly cooled off. • Low escape velocity • No atmosphere, so unprotected against meteorite impacts. • Must have formed in a molten state -“sea of lava” • Heavy rocks sunk to bottom; lighter rocks at the surface • No magnetic field means small core with little metalli ...
... • Moon is small, low mass so it rapidly cooled off. • Low escape velocity • No atmosphere, so unprotected against meteorite impacts. • Must have formed in a molten state -“sea of lava” • Heavy rocks sunk to bottom; lighter rocks at the surface • No magnetic field means small core with little metalli ...
Solar System
... At 2.77 AU, Ceres is the largest body in the asteroid belt, and the only one of them cataloged in 2006 as a dwarf planet. planet. Discovered in 1801 by Giuseppe Piazzi was considered a planet until 1850 when others find many similar objects. ...
... At 2.77 AU, Ceres is the largest body in the asteroid belt, and the only one of them cataloged in 2006 as a dwarf planet. planet. Discovered in 1801 by Giuseppe Piazzi was considered a planet until 1850 when others find many similar objects. ...
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.