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Sample exam 2
Sample exam 2

... 12. The rotational rate of Venus is really hard to determine, because Venus’s surface features cannot be seen under its thick opaque atmosphere. But it was known long before any spacecraft came anywhere near it! In fact, radar (radio waves) beamed from Earth at Venus and the Doppler shift were used ...
Dead Earth – Lesson 4 – Life on other worlds
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... • The Earth’s magnetic field also protects us from harmful particles and radiation from the Sun ...
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Astronomy Notes
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... There are two major motions of the earth…. • Rotation - the spinning of the earth on its axis resulting in daily changes such as the rising and setting of the sun and moon. • Revolution - the movement of the earth in its orbit around the sun resulting in yearly changes such as the changing ...
ASTR0 100 HW #4 – SOLUTIONS – 2 points each
ASTR0 100 HW #4 – SOLUTIONS – 2 points each

... 27. The fact that we have not yet discovered an Earth-mass planet tells us that such planets must be very rare. This should be considered surprising rather than reasonable. The lack of lower-mass planets discovered thus far is because lower-mass planets are harder to detect, and our current technolo ...
Who Wants To Be A Millionaire?
Who Wants To Be A Millionaire?

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Who Wants To Be A Millionaire?

... C north and sets in the south D south and sets in the north A ...
Planets of the Solar System – Scavenger Hunt KEY Saturn, Uranus
Planets of the Solar System – Scavenger Hunt KEY Saturn, Uranus

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... THE EARTH WITHIN A SOLAR SYSTEM What is the Solar System? Our solar system is the Sun and the planets that orbit, or spin, around it. The Sun is really a star that is only about 93,000,000 miles from us. Until 2006 we had nine known planets, Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Nept ...
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... A Mars-sized object crashes into Earth creating debris that ends up in orbit around the Earth, eventually coalescing through accretion to form the Moon. 4.6 Ga As the solar disk cools down, orbiting material collides and clumps to form larger objects (accretion). Continued accretion led to larger bo ...
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Solar nebula theory

... The Sun’s outer core will expand and the Sun will become a Red Giant. Theory #1: The Earth will get engulfed by the Sun and exist no more. Theory #2: When the Sun first begins to shrink, gravitational attraction between the Earth and Sun will become less. Some scientists think the Earth may move awa ...
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More evidence for ninth planet roaming solar system`s

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Life Cycles of Stars

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TC`s planet project

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Integrative Studies 410 Our Place in the Universe

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Ch. 26 The Sun and the Solar System

... – Followed the motion of planets, and the Moon throughout its orbit and not just at particular times. He had the most precise records from before the invention of the telescope Johannes Kepler: Tycho’s assistant. Discovered that planet’s orbits were elliptical rather than circular ...
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... sun and it is the closest planet to Earth. •It is named after the Roman Goddess of love and beauty. •The diameter of Venus is about 7,520 miles (about 400 miles smaller than that of Earth). •It takes 224 days for Venus to orbit around the sun. •Has mountains that are higher than Earth. ...
Chapter 25 Teacher Notes
Chapter 25 Teacher Notes

... •Most like Earth of all of the planets •“red planet” because of high iron content on its surface •Last volcanic activity about 100 million years ago •Olympus Mon is largest volcano in solar system. If on Earth, its base would cover the space between Cleveland and Washington D.C. Mars •Very thin atmo ...
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Task 1: The Solar System Task 2: Orbits of the

... scrap piece of paper before drawing them on your poster. 1 Draw a diagram showing the Sun, Mercury, Venus, Earth, the Moon, and Mars and the orbit for each planet and the Moon. 2 Add an arrow to show which way the planets orbit the Sun. 3 Label the planet with the longest year and the planet with th ...
Aims You are going to create a poster about space. First work
Aims You are going to create a poster about space. First work

... scrap piece of paper before drawing them on your poster. 1 Draw a diagram showing the Sun, Mercury, Venus, Earth, the Moon, and Mars and the orbit for each planet and the Moon. 2 Add an arrow to show which way the planets orbit the Sun. 3 Label the planet with the longest year and the planet with th ...
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Formation and evolution of the Solar System



The formation of the Solar System began 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center, forming the Sun, while the rest flattened into a protoplanetary disk out of which the planets, moons, asteroids, and other small Solar System bodies formed.This widely accepted model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.The Solar System has evolved considerably since its initial formation. Many moons have formed from circling discs of gas and dust around their parent planets, while other moons are thought to have formed independently and later been captured by their planets. Still others, such as the Moon, may be the result of giant collisions. Collisions between bodies have occurred continually up to the present day and have been central to the evolution of the Solar System. The positions of the planets often shifted due to gravitational interactions. This planetary migration is now thought to have been responsible for much of the Solar System's early evolution.In roughly 5 billion years, the Sun will cool and expand outward many times its current diameter (becoming a red giant), before casting off its outer layers as a planetary nebula and leaving behind a stellar remnant known as a white dwarf. In the far distant future, the gravity of passing stars will gradually reduce the Sun's retinue of planets. Some planets will be destroyed, others ejected into interstellar space. Ultimately, over the course of tens of billions of years, it is likely that the Sun will be left with none of the original bodies in orbit around it.
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