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Conjunctions an Oppositions
Conjunctions an Oppositions

... Superior Planets orbit farther from the Sun than Earth. They can be in conjunction or opposition. They are in Conjunction when they are on the other side of the Sun. As far away as they can be from Earth. They are in Opposition when the Earth is between the Superior Planet and the Sun. It is then th ...
PowerPoint Presentation - Planetary Configurations
PowerPoint Presentation - Planetary Configurations

... system may bear little resemblance to its original form • This view is more in line with the “planetary migration” thought to occur even more dramatically in many extrasolar planet systems • It may be difficult to prove or disprove these models of our early solar system. The many unexplained propert ...
astronomy final exam - Physics and Astronomy
astronomy final exam - Physics and Astronomy

... How are the solar system members distributed from the sun? What are the characteristics of the outer, or Jovian, planets as compared to the inner, or terrestrial, planets? What process which was apparently common to all of the terrestrial planets in their early history? What is the Oort cloud? Where ...
The Planets in our Solar System Solar System Basics
The Planets in our Solar System Solar System Basics

... More on planet formation . . . • Temperature and distance from the Sun influenced the condensation of various substances within the evolving solar system. • Eventually, the condensing material merged to form large bodies hundreds of kilometers in diameter. ...
Presentación de PowerPoint
Presentación de PowerPoint

... It is similar to our planet in size, mass, density and volume, but it has no oceans. It has lots of volcanoes, rivers of lava and mountains. Its dense atmosphere (CO2) causes a significant greenhouse effect, which increases its surface temperature up to 480 °C; that is why there is no water in liqui ...
The Sky Above
The Sky Above

... Earths would be required to fit across the Sun's disk, and its interior could hold over 1.3 million Earths. The Sun's outer visible layer is called the photosphere and has a temperature of 6,000°C (11,000°F). ...
a ComparativePlanetology 27
a ComparativePlanetology 27

... Runaway greenhouse boiled away the oceans. This probably cannot happen on Earth, but studying Venus is what got Jim Hansen wondering what would happen here. ...
Origin of the Universe and of the Solar System
Origin of the Universe and of the Solar System

... of similar craters of impact to those of the Moon, great lava plains and numerous extended and straight escarpments, possibly originated as a result of the contraction undergone when cooling. It has a magnetic body of very little intensity. It does not count on a true atmosphere: single plans of sod ...
File - SOCIAL SCIENCE
File - SOCIAL SCIENCE

... - Celestial bodies: the objects we can see in the sky are called celestial bodies. They are luminous and nonluminous. ...
geography-vocabulary-word-list
geography-vocabulary-word-list

... Q10. Fill in the blanks:1. Our solar system is a part of________galaxy. 2. The brightest star in the saptarishi is________. 3. The word planet is derived from greek word________. 4. The planet having rings around it is _______. 5. Planets which rotate from west to east is______. 6. Nearest planet to ...
Warm Up - Cloudfront.net
Warm Up - Cloudfront.net

... The Birth of Modern Astronomy • The first great astronomer to emerge after the Middle Ages was Nicolaus Copernicus (1473-1543) • Copernicus concluded that Earth was a planet, and proposed a model of the solar system with the sun at the center • He used circles to represent the planets’ orbits • Tyc ...
Venus
Venus

... Venus • Has the most dense atmosphere than any of the terrestrial planets • Mainly consists of carbon dioxide but also some deadly acids • The carbon dioxide traps thermal energy causing a greenhouse effect-causing the temperature to be so high • Average temperature 464*C • Venus has the hottest su ...
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... Relative sizes of Sun and Moon and Distances to Each • Aristarchus ...
Lecture1
Lecture1

... • The Sun and Moon have angular diameters of ~½◦ while the planets are even smaller at a few ” or less. • Stars are too small to be resolved: their apparent size is limited by turbulence in the atmosphere to be about 1” ...
Solar System Formation, Earth, Mercury, and the Moon (Professor
Solar System Formation, Earth, Mercury, and the Moon (Professor

... near the central core). Only metal (iron, nickel) and rocks (silicates) can survive in solid form. ...
Astronomy
Astronomy

... Also a gaseous planet, with traces of methane which makes it blue-green It axis of rotation is tilted so it rotates head over heel instead of spinning like a top Does have rings Moons:13+ Day: 16 hours Year: 84 Earth Years ...
Are we Alone? The Search for Life Beyond the
Are we Alone? The Search for Life Beyond the

... Are we Alone? - The Search for Life beyond the Earth. ...
First detection of a planet that survived the red giant expansion of its
First detection of a planet that survived the red giant expansion of its

... the first planet detected around a post­red giant star and one of the oldest planets  ...
Lecture - Faculty
Lecture - Faculty

... system may bear little resemblance to its original form • This view is more in line with the “planetary migration” thought to occur even more dramatically in many extrasolar planet systems • It may be difficult to prove or disprove these models of our early solar system. The many unexplained propert ...
HOMEWORK 5 SOLUTIONS CHAPTER 9 4.A A red giant star will
HOMEWORK 5 SOLUTIONS CHAPTER 9 4.A A red giant star will

... The radius of the 0.6 solar mass white dwarf will be slightly larger than the radius of the Earth. The radius of the 1.2 solar mass star will be about half the radius of the Earth. 4.C Since the Earth would not be within the even horizon of the black hole, the Earth’s orbit will not change. Since th ...
Friends newsletter december 2011
Friends newsletter december 2011

... are still analyzing data sent back by the Galileo probe in the 1990s. In a potentially significant finding in the search for life beyond Earth, scientists studying data from NASA's Galileo probe have discovered what appears to be a body of liquid water the volume of the North American Great Lakes lo ...
Friends newsletter december 2011
Friends newsletter december 2011

... are still analyzing data sent back by the Galileo probe in the 1990s. In a potentially significant finding in the search for life beyond Earth, scientists studying data from NASA's Galileo probe have discovered what appears to be a body of liquid water the volume of the North American Great Lakes lo ...
Study Guide for Unit 4: Stars and Solar System
Study Guide for Unit 4: Stars and Solar System

... is waxing and left when it is waning. The moon does not make its own light. It is reflecting the Suns light. *Half of the moon is always lit, however during the moons orbit we see different fractions of the lit portion. *The moon has gravity the pulls slightly on the Earth. This causes ocean tides. ...
Earth, Moon, and Beyond
Earth, Moon, and Beyond

... Mother- Mars Just- Jupiter Served- Saturn Us- Uranus Nine- Neptune Pizza’s- Pluto ...
What`s In Outer Space?
What`s In Outer Space?

... minutes long. • Saturn is so dense that if a large enough ocean could be found, it would float in it. • Saturn has rings around it that make it very beautiful. ...
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Comparative planetary science

Comparative planetary science or comparative planetology is a branch of space science and planetary science in which different natural processes and systems are studied by their effects and phenomena on and between multiple bodies. The planetary processes in question include geology, hydrology, atmospheric physics, and interactions such as impact cratering, space weathering, and magnetospheric physics in the solar wind, and possibly biology, via astrobiology.Comparison of multiple bodies assists the researcher, if for no other reason than the Earth is far more accessible than any other body. Those distant bodies may then be evaluated in the context of processes already characterized on Earth. Conversely, other bodies (including extrasolar ones) may provide additional examples, edge cases, and counterexamples to earthbound processes; without a greater context, studying these phenomena in relation to Earth alone may result in low sample sizes and observational biases.
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