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Astro 4 Practice Test 1
Astro 4 Practice Test 1

... d. It is one of about 10 regions in space where we can observe bright stars, which all seem to cluster near each other. 3. A friend of yours from a distant country is visiting you. While going for a walk one night, you point out the North Celestial Pole. They remark that they’ve never seen either ce ...
THE DYNAMIC TRIO - Siemens Science Day
THE DYNAMIC TRIO - Siemens Science Day

... Solar System – The solar system includes the Sun and everything that orbits it. This includes eight planets and their natural satellites such as Earth’s Moon; dwarf planets such as Pluto and Ceres; asteroids; comets and meteoroids. Sun – a star made up of 92% hydrogen and 7.8% helium, which is at th ...
Title of PAPER - Department of Physics and Astronomy
Title of PAPER - Department of Physics and Astronomy

... investigation; Mercury and Earth at their current orbits and Jupiter at Mercury’s orbital radius. Mercury and the hot Jupiter were assumed to have a rotation period similar to the Earth. Each of these have a known albedo, orbital radius, planetary radius, and mass1 2 3. From this information it is p ...
Earth from Space
Earth from Space

Star Properties and Stellar Evolution
Star Properties and Stellar Evolution

... What is the size of stars? Vary from the size of Earth to 2,000 times the size of the ...
IOSR Journal of Applied Physics (IOSR-JAP)
IOSR Journal of Applied Physics (IOSR-JAP)

... star gives them the rotational axis angle. But there are some other planets that have only one star. Their rotational angle is towards the star. It also means our earth is not moving around the sun not for only the sun’s gravity but also for another star’s gravity. ...
Artifact # 2, The Solar System
Artifact # 2, The Solar System

... an introduction for your Solar System lesson by ...
Lecture - faculty
Lecture - faculty

...  Ptolemaic model failed to reproduce the observations  Also, the model is not really based on uniform circular motion  So Copernicus favors the heliocentric (Sun-centered) model  Has a natural explanation for apparent retrograde motion of ...
Chapter 27 Stars and Galaxies
Chapter 27 Stars and Galaxies

Gravitation and Orbital Motion
Gravitation and Orbital Motion

Ch13 - People @ TAMU Physics
Ch13 - People @ TAMU Physics

... and the solar system's magnetic field has doubled in strength as interstellar space appears to be applying pressure. Energetic particles originating in the solar system have declined by nearly half, while the detection of high-energy electrons from outside has increased by 100 fold. The inner edge o ...
AST 301 Fall 2007 Review for Exam 3 This exam covers only
AST 301 Fall 2007 Review for Exam 3 This exam covers only

... planets? What are “planetesimals” and how did they form? Can you name a few lines of evidence that they once did exist? Explain clearly why the terrestrial and jovian planets have such different properties in terms of the theory described in this chapter. The section on the discovery of extrasolar p ...
moon earth sun - Conrad Public Schools
moon earth sun - Conrad Public Schools

... The pull of Earth’s gravity while the moon was still molten pulled the denser parts towards Earth This makes the moon egg shaped with the pointy end towards Earth The crust is the least dense portion and it is 60km thick on the Earth side and 100km thick on the backside The gravity also pulled the h ...
Origins of the Universe
Origins of the Universe

... • Planets are mostly round due to the effects of gravity • Over time, as the nebula spins, it flattens into a disk-like shape • Planets and other objects (e.g., asteroids) form in the flat plane of the disk – hence why the orbits of planets in our solar system are largely in the same plane – all rev ...
Spring `03 final exam study guide
Spring `03 final exam study guide

... distance from the planets’ centers. The period of the satellite of planet X, though, is greater than that of the satellite of planet Y. Which planet must have the greater mass? Explain your reasoning. 16. Which planets have rings? 17. If you were classifying the planets by size only, you might make ...
Asteroids and Meteors
Asteroids and Meteors

Careful measurements reveal that the earth has a slight difference in
Careful measurements reveal that the earth has a slight difference in

... they appear to “sink” over the horizon Curved Earth ...
Universal Time
Universal Time

... • Atmosphere are H2 and He (lost by the inner planets due to higher temperature and intense solar radiation, and gravitational mass not strong enough) ...
This is the Earth! This is where you live.
This is the Earth! This is where you live.

COMMENTS ON HOMEWORK 1 In many cases the answer to a
COMMENTS ON HOMEWORK 1 In many cases the answer to a

... critical points were left unexplained or a few words preceded by a critically placed 'since' or 'because' were provided as a poor substitute for an answer. Take time to think through the explanation requested, and then write it out in your own words. Remember a neatly drawn diagram is often helpful. ...
Galileo`s telescopes Galileo (1564
Galileo`s telescopes Galileo (1564

Seasons and the Changing Sky
Seasons and the Changing Sky

... •  Rising and setting of Sun, Moon, stars as viewed from Earth → Rotating celestial sphere •  Celestial poles: the points around which the stars appear to rotate •  Celestial equator: an extension of the Earth’s equator onto the celestial sphere Circumpolar star! ...
Untitled - IES Bachiller Sabuco
Untitled - IES Bachiller Sabuco

... In Roman mythology, Saturn is the god of agriculture. Saturn is the sixth planet from the Sun, and the second largest of the nine planets. Saturn is a giant gas planet, which is made up of about 75% hydrogen and 25%helium. It's most famous planet of beautiful rings. Saturn's rings are made up more w ...
p - INAF-OAT Trieste Users site
p - INAF-OAT Trieste Users site

... For instance, network of valleys similar to those excavated by terrestrial rivers ...
the young astronomers newsletter
the young astronomers newsletter

... ever found - a chunk of space rock about 65 miles in search for extraterrestrial life. But new research diameter beyond the orbit of Mars. It had been seen indicates some such planets may not be hosting life before but then lost. This was one of the faintest because of intense heat during their form ...
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Rare Earth hypothesis



In planetary astronomy and astrobiology, the Rare Earth Hypothesis argues that the origin of life and the evolution of biological complexity such as sexually reproducing, multicellular organisms on Earth (and, subsequently, human intelligence) required an improbable combination of astrophysical and geological events and circumstances. The hypothesis argues that complex extraterrestrial life is a very improbable phenomenon and likely to be extremely rare. The term ""Rare Earth"" originates from Rare Earth: Why Complex Life Is Uncommon in the Universe (2000), a book by Peter Ward, a geologist and paleontologist, and Donald E. Brownlee, an astronomer and astrobiologist, both faculty members at the University of Washington.An alternative view point was argued by Carl Sagan and Frank Drake, among others. It holds that Earth is a typical rocky planet in a typical planetary system, located in a non-exceptional region of a common barred-spiral galaxy. Given the principle of mediocrity (also called the Copernican principle), it is probable that the universe teems with complex life. Ward and Brownlee argue to the contrary: that planets, planetary systems, and galactic regions that are as friendly to complex life as are the Earth, the Solar System, and our region of the Milky Way are very rare.
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