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Study Guide #3 Answer Key
Study Guide #3 Answer Key

... believed to be, on average, about 1,000 ly (9.5×1015 km) thick.[7] It is estimated to contain at least 200 billion stars[8] and possibly up to 400 billion stars,[9] the exact figure depending on the number of very low-mass stars, which is highly uncertain. Extending beyond the stellar disk is a much ...
Read the rest of the press release
Read the rest of the press release

... Nature, the work not only improves our understanding of the evolution of our planet but also makes it possible to determine the necessary conditions for the presence of liquid water on other Earth-like planets. Like most stars, the Sun's luminosity very slowly increases during the course of its exis ...
What is the Nice model? - Lunar and Planetary Institute
What is the Nice model? - Lunar and Planetary Institute

... Belt]. At this time the giant planets are closer together than they are now. Panel 2: Planetesimals slowly leak out of Kuiper Belt and are gravitationally scattered by planets. Backreaction makes Jupiter migrate toward the Sun and makes Saturn, Uranus, and Neptune migrate away from the Sun. ...
Planet found in nearest star system to Earth » Astronautical News
Planet found in nearest star system to Earth » Astronautical News

... Alpha Centauri B is very similar to the Sun but slightly smaller and less bright. The newly discovered planet, with a mass of a little more than that of the Earth, is orbiting about six million kilometres away from the star, much closer than Mercury is to the Sun in the Solar System. The orbit of th ...
Science 09 Space Review 1. Know what a light year is
Science 09 Space Review 1. Know what a light year is

... 12. What are the phases of the moon and how do we explain it? (page 318, DO page 325 #6) 13. What are two technologies that will speed up space travel. Explain the scientific principles behind these two technologies (from the video handout). 14. How is the fact that according to Einstein, the clocks ...
WORD - hrsbstaff.ednet.ns.ca
WORD - hrsbstaff.ednet.ns.ca

... 11. A band of the celestial sphere extending on either side of the ecliptic that represents the path of the different celestial bodies (i.e. Moon, Sun, planets) and contains constellations like Gemini and Aquarius is called the a. North Celestial Pole. b. South Celestial Pole. c. Celestial Equator. ...
Review Astronomy - Cowley`s Earth Systems
Review Astronomy - Cowley`s Earth Systems

... c. The sun is a smaller, less massive star d. The sun is spinning on its axis 10. Why does the Moon only have 1/6 of the Earth’s gravity? ...
Other Solar Systems Around Other Stars
Other Solar Systems Around Other Stars

... • The signal-to-noise ratio will be too small to detect unless the planet is MASSIVE and the planet is CLOSE to the parent star, so that the parent star is reaction’ing as FAST AS POSSIBLE • That means the method is highly biased to find BIG Jupiter-like planets in orbits well inside the equivalent ...
Mars` Moons
Mars` Moons

...  The chemical composition of comets (rich in deuterium) is consistent with a cometary origin of at least some of Earth’s water and organic ...
Interstellar clouds
Interstellar clouds

... The Interstellar Medium • The interstellar medium of the milky way consists of clouds containing 90% Hydrogen, 9% Helium, and 1% dust grains. • It has an extremely low density of 1 atom per cm3, about 10 billionth the density of gas created by our best vacuums here on earth. ...
Week 8
Week 8

... Gas is eventually captured or pushed out by wind from the star, but dust and planetesimals are left around ...
Scientific Investigation - Kempsville Middle School
Scientific Investigation - Kempsville Middle School

... 48. A physical change occurs when there is a change in the physical properties, but the chemical properties remain the same. 49. A chemical reaction occurs when both the physical and chemical properties have been changed. 50. A chemical change occurs when matter interacts with matter to form a new s ...
Evolution of the Solar System and Planets Homework
Evolution of the Solar System and Planets Homework

... 80. Kepler was the first astronomer to use a telescope to accurately observe and record various objects seen in the night sky. 81. The ancient Greeks proposed an Earth-centered or Geo-centric view of the universe. 82. The Ptolemaic model of the solar system stayed in use for so long (even though we ...
pdf format
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 ...
Extra-Solar Planets
Extra-Solar Planets

... • Method 1 – Use the fact that the Sun and Planet corotate around their common centre of gravity. – So the star will be moving around a small ellipse whose size depends on the mass and distance of the planet. – Precise measurements of the doppler shift in the spectral lines of the star can show up t ...
AST 207 Test 2 26 October 2011
AST 207 Test 2 26 October 2011

... b. (2 pts.) Why does the helium in the core of the sun not fuse at the present time? (1 pt.) When that helium does fuse eventually, what will the helium become? The core of the sun is too cool to fuse helium. When it does fuse helium, the result will be carbon. c. (3 pts.) When the solar system was ...
sorption feature centered near 0.7 µm and attributed → Fe 3+
sorption feature centered near 0.7 µm and attributed → Fe 3+

... Introduction: The structural traits of our Solar System, including physical distribution of objects out through the Kuiper Belt, are not yet fully understood. Unifying these diverse characteristics has been the subject of multiple dynamical studies of the Solar System. The recent “Nice model” [1,2,3 ...
UT 3.4 - Homeschool Academy
UT 3.4 - Homeschool Academy

... gravitational force than the terrestrial planets. This prevents their gases from escaping, so they have thick atmospheres. All of the giants have many moons and are surrounded by a set of rings. A ring is a thin disk of small particles of ice and rock. Jupiter is the largest and most massive planet. ...
Kepler`s Laws and Galileo 8/31/2016
Kepler`s Laws and Galileo 8/31/2016

... • Wrote book on Copernican vs Ptolemaic models in 1632, nominally with Church’s permission. But it offended Church. Dialogue Concerning the Two Chief World Systems. In Italian. Character in book Simplicio defended Church’s position  spent last 10 years of his life in house arrest. Catholic church s ...
Lecture 19: Planet Formation I. Clues from the Solar System
Lecture 19: Planet Formation I. Clues from the Solar System

... acceleration. Considering that the pressure is much smaller than gravity, one finds that the gas rotates ~0.5% slower than the keplerian speed. ...
Earth and Space Science - science
Earth and Space Science - science

... • Dark Matter: Scientists noted while observing the Andromeda galaxy that the stars orbit the centre of the gravity much faster than predicted by the galaxy’s mass. 90% of the galaxy’s mass comes from something that emits no light. ...
α Centauri: a double star - University of Canterbury
α Centauri: a double star - University of Canterbury

... Wiegert & Holman found stable orbits inside 2.34 AU, but unstable 3 to 70 AU from each star, provided i = 0° (coplanar with binary orbit). ...
Lesson #5: Constellations - Center for Learning in Action
Lesson #5: Constellations - Center for Learning in Action

... Cover the outside of the tube with the colored paper of your choice and then decorate it with stickers and other art materials provided. Using the black construction paper cut out a circle with a 6-8 inch diameter. Students may need help with this step. In the center of the black circle, draw the po ...
Scale of the Universe in space, time, and motion
Scale of the Universe in space, time, and motion

... Universe on the entire range of length scales from sub-nuclear to cosmological. • Knowing the typical size and time scales of a ...
The Sky and the Motions of the Earth
The Sky and the Motions of the Earth

... once (west-to-east) on its axis. This causes us to face different directions and see different stars. The stars’ daily (diurnal) motion reflects the earth’s spin. ...
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History of Solar System formation and evolution hypotheses



Ideas concerning the origin and fate of the world date from the earliest known writings; however, for almost all of that time, there was no attempt to link such theories to the existence of a ""Solar System"", simply because almost no one knew or believed that the Solar System, in the sense we now understand it, existed. The first step towards a theory of Solar System formation was the general acceptance of heliocentrism, the model which placed the Sun at the centre of the system and the Earth in orbit around it. This conception had been gestating for thousands of years, but was only widely accepted by the end of the 17th century. The first recorded use of the term ""Solar System"" dates from 1704.
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