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PHYSICS 1500 - ASTRONOMY TOTAL
PHYSICS 1500 - ASTRONOMY TOTAL

... The overwhelming majority of exoplanets known today have been discovered by the Radial Velocity and Transit techniques. Which of the following types of planets would you expect to be discovered most readily using these techniques? (a) hot planets in orbits which graze the stellar surface (b) large p ...
Astronomy - SparkNotes
Astronomy - SparkNotes

... surface features of a planet. • When the heat is gone, the planet can no longer evolve from the inside, and it is considered dead. Atmosphere: The balance between the force of gravity on a planet and its average surface temperature determines the amount and composition of its atmosphere. • If the av ...
Space
Space

... times wider than the Earth. The solar system can be divided into two planetary groups: the Earth like (terrestrial) planets and the outer or Jovian planets. Terrestrial planets: smaller, rockier, closer to the Sun. Jovian planets: large and gaseous, located greater distances from the Sun with small ...
Actual Earth Motions
Actual Earth Motions

... “ rotation of the sun 2 rotation of the Earth 0 revolution of the Earth “ revolution of the sun ...
Measuring the Distance to Stars Using Parallax
Measuring the Distance to Stars Using Parallax

... Notice from the pictures that astronomers measure the star’s position against background stars, first in December and again in June when the Earth is opposite from where it was 6 months ago. Now notice that the Earth in December to the star and back to the Earth in June makes an angle. It is this an ...
Final Study Guide
Final Study Guide

... 22. Discuss the process of differentiation, and how we can know about the interior of the earth. 23. What is meant by the “runaway greenhouse effect” that makes Venus so hot? How does it work? 24. Describe Uranus in terms of size, composition, appearance, rotation rate, atmosphere, and magnetic fiel ...
UNIT 2 - Orange Public Schools
UNIT 2 - Orange Public Schools

... categorizing, representing, and interpreting the natural and designed world. Who, what, when, where, why, and how questions form the basis for young learners’ investigations during sensory explorations, experimentation, and focused inquiry Fundamental scientific concepts and principles and the links ...
Astronomy - Dalriada at dalriada.org.uk
Astronomy - Dalriada at dalriada.org.uk

... The remaining eight planets divide into two groups, the inner planets: Mercury; Venus; Earth; Mars, and the outer planets: Jupiter; Saturn; Uranus; Neptune. Extracting from [18]: The inner planets and outer planets are characterized by different features. The 4 inner planets are called terrestrial p ...
THE DEFINITION OF PLANET: A DYNAMICIST`S POINT OF VIEW
THE DEFINITION OF PLANET: A DYNAMICIST`S POINT OF VIEW

... ready to give a ”dynamical” definition of planet, applicable to our solar system as well as to extrasolar planetary systems. A non deuterium burning celestial body is a planet if the following three conditions are all met for most of its existence: 1. it moves about the Sun (alternatively, a star) a ...
Comets and the Solar System Practical Astronomy: 16 September
Comets and the Solar System Practical Astronomy: 16 September

... Comets and the Solar System Practical Astronomy: 16 September 2014 ...
Comets and the Solar System Practical Astronomy: 16 September
Comets and the Solar System Practical Astronomy: 16 September

... Comets and the Solar System Practical Astronomy: 16 September 2014 ...
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File 3rd quarter review

...  The direct (perpendicular) rays of the sun hit the tropic of ____________.  Sun rise is _______ of east, and sunset is ________ of the west. 58. Winter solstice is on ________.  The _______ hemisphere is tilted towards the sun.  The direct (perpendicular) rays of the sun hit the Tropic of _____ ...
Habitability
Habitability

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Habitability
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... – Several stars in our galaxy with planets the size of Jupiter within terrestrial zone from their sun – Mass of star • Larger mass, greater luminosity, shorter life • Most abundant stars in galaxy are least luminous and longest-lived (M-dwarfs) ...
RealOccult - Montgomery College
RealOccult - Montgomery College

... profile very accurately so that when solar eclipses happen and the last part of the photosphere appears in deep lunar valleys, forming Baily's Beads. The timing of these Baily's beads can be used to tell whether the sun is getting larger or smaller over time, by comparing Baily's beads timing from s ...
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Naked-eye astronomy

... Last thought on coordinates • The Equatorial System of Coordinates is what most astronomers use when specifying the location of an object on the Celestial Sphere • Right Ascension (measured eastwards from the Vernal Equinox) goes from 0h to 24h • Declination (measured north or south from the celes ...
Part II: Ideas in Conflict.
Part II: Ideas in Conflict.

... a spherical shell which rotate around the earth.  An alternate model, which works just as well, is for the earth to rotate inside the shell of stars.  In order to explain the motion of all the other celestial bodies, more spherical shells must be added to this model. ...
Don`t Panic, But the Sun Will (Far) Outlive Earth (Op-Ed)
Don`t Panic, But the Sun Will (Far) Outlive Earth (Op-Ed)

... This 10% increase in the sun’s brightness, triggering the evaporation of our oceans, will occur over the next billion years or so. Predictions of exactly how rapidly this process will unfold depend on who you talk to. Most models suggest that as the oceans evaporate, more and more water will be pres ...
Chapter 1: Introduction to Earth Science Indiana State Standards 1
Chapter 1: Introduction to Earth Science Indiana State Standards 1

... Indiana State Standards Understand that both weather and climate involve the transfer of matter and energy throughout the atmosphere and hydrosphere, driven by solar energy and gravity. (ES.4.3, ES.4.4, ES.4.5, ES.4.6) SCI.ES.4.1 2010 Examine the origins, structure, composition, and function of Eart ...
Study Guide 2 - Otterbein University
Study Guide 2 - Otterbein University

... Short Answer Questions [3 points each] (Please use the back side of the computer sheet to record your answers) 7. Explain Kepler’s second law in your own words. (Merely restating it won’t garner any points.) 8. Why do the planets have (almost) circular orbits around the Sun, even though the gravita ...
conjunction and opposition
conjunction and opposition

... Greatest elongation is the best time to view these inner planets as they will be seen at their furthest angular distance from the Sun, well away from a line of sight with the Sun. ...
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SC.4.E.5.4,5.1, 5.2, 5.3 Earth & Space

... Answer: The stars appear to move because of Earth’s rotation. Constellations or patterns of stars also change with the seasons because Earth is orbiting around the sun. 3. Why do constellations change with the seasons? Answer: The constellations have been in the same positions for thousands of years ...
What causes eclipses?
What causes eclipses?

... –  Like the Sun and Moon, planets usually drift eastward relative to the stars from night to night, but sometimes, for a few weeks or few months, a planet turns westward in its apparent retrograde motion. •  Why did the ancient Greeks reject the real explanation for planetary motion? –  Most Greeks ...
section 4 powerpoint
section 4 powerpoint

... The importance of Kepler’s 3rd Law is that, as shown by Newton, the constant of proportionality for a3 = P2 contains two constants, π (pi) and G (the gravitational constant), plus the sum of the masses of the two coorbiting bodies. If one can determine orbital periods P and semi-major axes a, then ...
Thinking About Gravity
Thinking About Gravity

... Gravity: Everything has its own gravity. Everything exerts a pulling force on everything else. However, only large things have enough gravity to successfully pull other objects towards them. The force of gravity depends on how much mass you have. The larger the object is, the more gravity it has (Th ...
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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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