The Solar System
... Neptune The farthest planet from the sun It takes 165 years to orbit the sun It makes a rotation on its once every 16.1 hours Temperature: - 364* F Moons: 13 ...
... Neptune The farthest planet from the sun It takes 165 years to orbit the sun It makes a rotation on its once every 16.1 hours Temperature: - 364* F Moons: 13 ...
Our Solar System
... one moon. The moon does not have a name. Earth’s atmosphere is 77% nitrogen and 21% oxygen. 71% of earths surface is covered in water. Earth is the only planet in which water Can exist in liquid form on its surface. It takes 365 days to orbit around the sun. When it spins it takes 23 hours and 56 mi ...
... one moon. The moon does not have a name. Earth’s atmosphere is 77% nitrogen and 21% oxygen. 71% of earths surface is covered in water. Earth is the only planet in which water Can exist in liquid form on its surface. It takes 365 days to orbit around the sun. When it spins it takes 23 hours and 56 mi ...
Chapter 15 - Department Of Computer Science
... Only the Earth and Mars have moons Only the Earth has surface water and an atmosphere that is 21% oxygen, others have no free oxygen in their atmosphere Mercury: the closest planet to the Sun, has the shortest period of revolution, is the fastmoving planet ...
... Only the Earth and Mars have moons Only the Earth has surface water and an atmosphere that is 21% oxygen, others have no free oxygen in their atmosphere Mercury: the closest planet to the Sun, has the shortest period of revolution, is the fastmoving planet ...
WebQuest: Earth, Moon, and Sun
... A. Earth is the only planet known to ___________ life. B. Earth’s ________________ are giant landmasses. C. __________________ is the highest of Earth’s mountains. D. The _____________ Ocean covers more than 1/5 of the Earth’s surface and is located between the Americas and Europe. Hurricanes often ...
... A. Earth is the only planet known to ___________ life. B. Earth’s ________________ are giant landmasses. C. __________________ is the highest of Earth’s mountains. D. The _____________ Ocean covers more than 1/5 of the Earth’s surface and is located between the Americas and Europe. Hurricanes often ...
Astronomy Unit Notes - sciencepowerpoint.com
... Most meteorites also burn up in our atmosphere. • The winter solstice is the moment when the earth is at a point in its orbit where one hemisphere is most inclined away from the sun. – Shortest day and longest night of the year (Around December 21st) – Summer solstice is when axial tilt is most incl ...
... Most meteorites also burn up in our atmosphere. • The winter solstice is the moment when the earth is at a point in its orbit where one hemisphere is most inclined away from the sun. – Shortest day and longest night of the year (Around December 21st) – Summer solstice is when axial tilt is most incl ...
A. Start with a video clip from YouTube
... luck out because some stars explode early-on in the history of the universe, and still explode today. These exploding stars can make heavier elements and they are called ________________________. Without them, we would not exist. 8. For about another ______ billion years, the universe continues to h ...
... luck out because some stars explode early-on in the history of the universe, and still explode today. These exploding stars can make heavier elements and they are called ________________________. Without them, we would not exist. 8. For about another ______ billion years, the universe continues to h ...
Solar System Astronomy
... Coriolis Effect: the tendency of matter moving across Earth’s surface to be deflected from a straight-line path. Eccentricity: the out-of-roundness of an ellipse. Eclipse: when either the Moon passes between Earth and the Sun or the Moon is in Earth’s shadow. Ellipse: a closed curve around two fixed ...
... Coriolis Effect: the tendency of matter moving across Earth’s surface to be deflected from a straight-line path. Eccentricity: the out-of-roundness of an ellipse. Eclipse: when either the Moon passes between Earth and the Sun or the Moon is in Earth’s shadow. Ellipse: a closed curve around two fixed ...
Solar System Study Guide
... Apparent motion is caused by the observer moving, whereas real motion is caused by the object moving. We could imagine that the Earth is at the center of a large sphere, called the celestial sphere; and the Sun, stars, etc. are located on the sphere and move from east to west across the sky, caused ...
... Apparent motion is caused by the observer moving, whereas real motion is caused by the object moving. We could imagine that the Earth is at the center of a large sphere, called the celestial sphere; and the Sun, stars, etc. are located on the sphere and move from east to west across the sky, caused ...
1. What determines how the height of the sun in the sky at
... What determines how the height of the sun in the sky at noontime changes through the year? the tilt of Earth’s axis relative to the direction of the noontime sun the tidal cycle which in turn depends on the position of our Moon Earth’s distance from the sun—closest in summer, furthest in winter tric ...
... What determines how the height of the sun in the sky at noontime changes through the year? the tilt of Earth’s axis relative to the direction of the noontime sun the tidal cycle which in turn depends on the position of our Moon Earth’s distance from the sun—closest in summer, furthest in winter tric ...
Life Beyond Earth - University of Iowa Astrophysics
... • Water allows other molecules to dissolve, move around, and interact with each other ...
... • Water allows other molecules to dissolve, move around, and interact with each other ...
solarsystem_intermed..
... o the distances of the nine planets from the Sun in km (Col 2) o the distances relative to the Earth (e.g. Jupiter is 5.2x further than the Earth from the Sun) (Col 3) o Using a scale of 1cm = 3,000,000 km (3 million km), planetary distances have been calculated in “scaled cm” (and also in m) in the ...
... o the distances of the nine planets from the Sun in km (Col 2) o the distances relative to the Earth (e.g. Jupiter is 5.2x further than the Earth from the Sun) (Col 3) o Using a scale of 1cm = 3,000,000 km (3 million km), planetary distances have been calculated in “scaled cm” (and also in m) in the ...
Spicy Solar System Goal Model the solar system with edible
... Understanding scales See table Minimal knowledge about the Solar System ...
... Understanding scales See table Minimal knowledge about the Solar System ...
Solar System
... largest planet in the Solar System. It is a gas giant with mass one-thousandth of that of the Sun but is two and a half times the mass of all the other planets in the Solar System combined ...
... largest planet in the Solar System. It is a gas giant with mass one-thousandth of that of the Sun but is two and a half times the mass of all the other planets in the Solar System combined ...
Day-28
... (volume = 4/3 π R3) and where the planet loses the energy (surface area = 4 π R2) . The amount of energy that could be lost divided by the area of loss is proportional to R/3, where R is the radius of the planet. ...
... (volume = 4/3 π R3) and where the planet loses the energy (surface area = 4 π R2) . The amount of energy that could be lost divided by the area of loss is proportional to R/3, where R is the radius of the planet. ...
Solar System Diagnostic
... Why does the title say “Our” Solar System? _______________________________________________________________________ __________________________ Name as many planets as you can. Hint: there are eight planets in our solar system. _____________ ...
... Why does the title say “Our” Solar System? _______________________________________________________________________ __________________________ Name as many planets as you can. Hint: there are eight planets in our solar system. _____________ ...
Chapter 1-2
... Earth’s Movement - Earth rotates (spins) on its axis o Imaginary line that runs through the center of the earth from the north to the south pole o Rotation takes 24 hours (23 hours 56 minutes,4.09 seconds) = one day Causes day and night o Revolution (earth’s complete trip around the sun) takes 36 ...
... Earth’s Movement - Earth rotates (spins) on its axis o Imaginary line that runs through the center of the earth from the north to the south pole o Rotation takes 24 hours (23 hours 56 minutes,4.09 seconds) = one day Causes day and night o Revolution (earth’s complete trip around the sun) takes 36 ...
Our Solar System
... Neptune: 119% of Earth’s Pluto: 8% of Earth’s So what this all means is that a person who weighs 100 pounds on Earth would weigh 38 pounds on Mercury or Mars, 91 pounds on Venus, 254 pounds on Jupiter (!!!), 108 pounds on Saturn, 91 pounds on Uranus, 119 pounds on Neptune, or only 8 pounds on Pluto. ...
... Neptune: 119% of Earth’s Pluto: 8% of Earth’s So what this all means is that a person who weighs 100 pounds on Earth would weigh 38 pounds on Mercury or Mars, 91 pounds on Venus, 254 pounds on Jupiter (!!!), 108 pounds on Saturn, 91 pounds on Uranus, 119 pounds on Neptune, or only 8 pounds on Pluto. ...
Building Our Solar System Profile - Grade91P
... - located between Mars and Jupiter - rocky remains from formation of our solar system 4.6 bil. Years ago - rocks of various sizes: a few feet to several miles in diameter -Ceres: largest asteroid 950 km wide -Jupiter and Mars can absorb these asteroids or fling them into orbits of other planets ...
... - located between Mars and Jupiter - rocky remains from formation of our solar system 4.6 bil. Years ago - rocks of various sizes: a few feet to several miles in diameter -Ceres: largest asteroid 950 km wide -Jupiter and Mars can absorb these asteroids or fling them into orbits of other planets ...
Solar System Diagram
... Mercury and Pluto have seven planets between them. There is just one planet between Uranus and Pluto. During the 16th century only six planets had been discovered: Earth, Mars, Mercury, Jupiter, Saturn, and Venus. These are the six planets closest to the Sun. Uranus is between Saturn and Neptune. Th ...
... Mercury and Pluto have seven planets between them. There is just one planet between Uranus and Pluto. During the 16th century only six planets had been discovered: Earth, Mars, Mercury, Jupiter, Saturn, and Venus. These are the six planets closest to the Sun. Uranus is between Saturn and Neptune. Th ...
Today`s Powerpoint - Physics and Astronomy
... Aristotle vs. Aristarchus (3rd century B.C.): Aristotle: Sun, Moon, Planets and Stars rotate around fixed Earth. Aristarchus: Used geometry of eclipses to show Sun bigger than Earth (and Moon smaller), so guessed that Earth orbits the Sun. Also guessed Earth spins on its axis once a day => apparent ...
... Aristotle vs. Aristarchus (3rd century B.C.): Aristotle: Sun, Moon, Planets and Stars rotate around fixed Earth. Aristarchus: Used geometry of eclipses to show Sun bigger than Earth (and Moon smaller), so guessed that Earth orbits the Sun. Also guessed Earth spins on its axis once a day => apparent ...
Jupiter • The largest planet in the solar system
... The largest planet in the solar system. Stripes and swirls are cold, windy clouds of ammonia and water. Great Red Spot is a giant storm bigger than Earth that has raged for hundreds of years. Surrounded by 53 confirmed moons, as well as 14 provisional ones. Has three rings, but they are ve ...
... The largest planet in the solar system. Stripes and swirls are cold, windy clouds of ammonia and water. Great Red Spot is a giant storm bigger than Earth that has raged for hundreds of years. Surrounded by 53 confirmed moons, as well as 14 provisional ones. Has three rings, but they are ve ...
Earth's rotation
Earth's rotation is the rotation of the planet Earth around its own axis. The Earth rotates from the west towards east. As viewed from North Star or polestar Polaris, the Earth turns counter-clockwise.The North Pole, also known as the Geographic North Pole or Terrestrial North Pole, is the point in the Northern Hemisphere where the Earth's axis of rotation meets its surface. This point is distinct from the Earth's North Magnetic Pole. The South Pole is the other point where the Earth's axis of rotation intersects its surface, in Antarctica.The Earth rotates once in about 24 hours with respect to the sun and once every 23 hours 56 minutes and 4 seconds with respect to the stars (see below). Earth's rotation is slowing slightly with time; thus, a day was shorter in the past. This is due to the tidal effects the Moon has on Earth's rotation. Atomic clocks show that a modern-day is longer by about 1.7 milliseconds than a century ago, slowly increasing the rate at which UTC is adjusted by leap seconds.