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Venus
Venus

... and rotates in the opposite direction to most other planets. Venus rotates so slow cause a atmospheric Venus is the second planet from the tide created by solar heating of the thick Venusian atmosphere. ...
apparent magnitude
apparent magnitude

... • A period of rotation is the length of time that an object takes to rotate once on its axis. • A period of revolution is the length of time that an object takes to revolve around the sun. • Mercury is the planet closest to the sun. • Of all the terrestrial planets, Venus has the densest atmosphere ...
Planet Earth - ThinkChemistry
Planet Earth - ThinkChemistry

... • What is the difference between stars, planets and moons? • What is the difference between The Solar System, a galaxy and The Universe? ...
Sample Exam 1
Sample Exam 1

... b. a rotational speed slower than Mercury c. dominantly composed of hydrogen d. a very dense atmosphere 17. Micrometeorites are found on the surface of the Earth, what are they called prior to impact? a. meteoroids flying through space, meteors as they cross the Earth’s atmosphere b. meteors flying ...
Document
Document

... between two large masses • The larger the mass, the larger the force of gravity and the further the masses move apart, the smaller the force of gravity ...
movement in the solar system
movement in the solar system

... among the stars. These are the planets. Planets, like the earth and moon do not make light. They get light from the sun. It has been known for more than 500 years that planets are satellites of the sun. That means that they go around the sun. ...
A tour of the solar system.
A tour of the solar system.

... Chamberlin (1900) – A star passed close to Sun, pulling away huge filaments of material. Problems: such events are extremely rare. Also material is so hot that it would dissipate into space and not accrete. ...
Chapter3 - The Science of Astronomy-ppt
Chapter3 - The Science of Astronomy-ppt

... object remains in motion unless a force acts to stop it or change its direction. • Tycho’s observations of a comet and supernova showed that the heavens could change. • The lack of noticeable stellar parallax was simply due to the fact that the stars were much farther away than anyone had previously ...
Current Study Guide - Department of Physics and Astronomy
Current Study Guide - Department of 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 ...
Astronomy Vocabulary File
Astronomy Vocabulary File

... above the planet’s North Pole Retrograde rotation—the clockwise spin of a planet or moon as seen from above the planet’s North Pole Gas giants—the large, gaseous planets of the outer solar system Satellite—a natural or artificial body that revolves around a planet Phases—the different appearances of ...
Evidence #1: Earth`s average density is higher than the Moon`s. The
Evidence #1: Earth`s average density is higher than the Moon`s. The

... the center of the cloud. Figure 2 shows these collisions. These pieces start to stick together forming larger chunks. This is similar to how individual snowflakes can come together to make a snowball. As the chunks get bigger, they attract more pieces. These smaller pieces collide with and stick to ...
NEXT MEETING THURSDAY, 18 th October 2012
NEXT MEETING THURSDAY, 18 th October 2012

... launched on November 5, 1964 was lost when the launch vehicle's nose fairing failed to jettison. On July 15, 1965 Mariner 4 became the first successful flyby of Mars and sent back 22 close-up pictures of the planet – showing craters and not canals! Subsequent Mariners went to Mars and Venus (two wer ...
Instructions for
Instructions for

... from the surface of Earth. Allow up to 5 minutes and encourage logical discussion based on current knowledge. HINTS A. The distance between the Sun and Earth is 400 times greater than the distance between the Moon and Earth. B. This galaxy cannot be our galaxy (the Milky Way) because we are able to ...
How was the Solar System Formed?
How was the Solar System Formed?

... Planets of the Solar System Standards: 1b Students know the evidence from Earth and Moon rocks indicates that the Solar System was formed from a Nebula cloud of dust and gas approximately 4.6 billion years ago (bya). 1c Students know the evidence from geological studies of Earth and other planets su ...
SOL Review - Mr. Gautier`s Biology/Earth Science
SOL Review - Mr. Gautier`s Biology/Earth Science

... 2. If an area is very karst, it probably has a lot of what? 3. If the water table goes up, what zone gets bigger? 4. Most fossils are found in this type of rock? 5. According to the Law of Superposition, the oldest rock is where? 6. Cold water rising to the surface is an example of what? 7. Ocean Cu ...
Asteroids
Asteroids

... objects with an irregular shape that orbit the Sun but are too small and numerous to be considered planets. They are known as minor planets. Asteroids range in size from Ceres, which has a diameter of about 1000 km, down to the size of pebbles. Sixteen asteroids have a diameter of 240 km or greater. ...
friends of the planetarium newsletter - june 2010
friends of the planetarium newsletter - june 2010

... South Equatorial Belt (SEB), the brown cloudy band is twice as wide as Earth and more than twenty times as long. The loss of such an enormous "stripe" can be seen with ease halfway across the solar system. "In any size telescope, or even in large binoculars, Jupiter's signature appearance has always ...
Unit Review Name
Unit Review Name

... how development in one area leads to advancement in the other. You have taken part in a number of activities that required creative solutions to a variety of problems. Many of the activities have resulted in a number of different solutions for the same problem. These solutions may have involved diff ...
Astronomy Milestone/OAS practice
Astronomy Milestone/OAS practice

... 26. A hurricane-type cloud known as the Great Red Spot can be found on which planet? A. Saturn B. Mars C. Uranus D. Jupiter 27. The atmosphere of Venus consists of thick yellow clouds formed mostly from A. helium. B. sulfur. C. hydrogen. D. carbon. 28. Which accounts for the fact that a compass can ...
chart_set_2 - Physics and Astronomy
chart_set_2 - Physics and Astronomy

... in “epicycles” that orbit the Earth. This helped to explain retrograde motion for a long time, until astronomical observations became more precise. The Ptolemaic Model. ...
Sky Science Review for Test Part A
Sky Science Review for Test Part A

... Sky Science Review for Test Science 6 S.O. 1 – Recognize that the Sun and stars emit the light by which they are seen, and that most other bodies in space, including Earth’s moon, other planets and their moons, comets and asteroids, are seen by reflected light. Bodies in space that emit (give off) l ...
Science Standards - Explore-It
Science Standards - Explore-It

... 4.2.3 Describe how human beings have made tools and machines, such as satellites to observe and do things that they could not otherwise sense or do at all, or as quickly or efficiently. 4.1.1 Recognize and describe how results of similar scientific investigations may turn out differently due to inco ...
DDS Distances #3 Speed of light = 300,000 km/s distance of a
DDS Distances #3 Speed of light = 300,000 km/s distance of a

... ...
Mercury`s Formation
Mercury`s Formation

... Candidates for where the material ended up are the Sun, Venus, and Earth The Solar Winds would most likely leave a few traces of the proto layers since the Solar Winds wouldn’t be able to make a near spherical object Chemical equilibrium condensation models for the solar nebula can’t account for a m ...
Answers
Answers

... (a) The distance between the Equator and the centre of the Earth is greater than that between the North Pole and the centre of the Earth. The greater the distance between two bodies, the smaller is the gravity between them. (b) The mass of the Earth is about 100 times that of the Moon, and the radiu ...
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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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