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Heliocentric model
Heliocentric model

... can make are their positions relative to the Earth and the Sun – the planetary configuration – Inferior conjunction – between us and the Sun (a transit occurs when it is silhouetted against the Sun’s bright ...
Document
Document

... celestial object—what fraction of the sky that object seems to cover • The angular diameter (or angular size) of the Moon is ½° or the Moon subtends an angle of ½°. ...
Asteroids, Comets and Meteorites What is an Asteroid? Asteroids
Asteroids, Comets and Meteorites What is an Asteroid? Asteroids

... material from which we are condensed created solids in its expanding atmosphere › these included minerals, metals, hydrocarbons, icy aggregates › when our Solar system was formed, the processes that led to the concentrations of elements we now find at different distances from the Sun were complex, r ...
Milankovitch Cycles and Glaciation
Milankovitch Cycles and Glaciation

... The episodic nature of the Earth's glacial and interglacial periods within the present Ice Age (the last couple of million years) have been caused primarily by cyclical changes in the Earth's circumnavigation of the Sun. Variations in the Earth's eccentricity, axial tilt, and precession comprise the ...
Science 09 Space Review 1. Know what a light year is
Science 09 Space Review 1. Know what a light year is

... assignment). Which planets move faster? Why do some planets move faster than others? Which planets are hot, which planets are cold? (pg 328-340) Do page 432 #20 16. Write down possible fusion equations for fusion reactions that occur during the life cycle of stars. Massive stars burn a succession of ...
astronomy history time machine
astronomy history time machine

... clues suggesting that Earth is not the center of the universe the scientific revolution that dethroned Earth from its location at the center of the universe Copernicus’s argument that the planets orbit the Sun why the direction of motion of the planets on the celestial sphere sometimes appears to ch ...
Grade 9 Applied
Grade 9 Applied

... _____ 8. How many electrons can the first shell of a Bohr-Rutherford diagram hold? a) 2 b) 4 c) 6 d) 8 _____ 9. How many electrons can the second shell of a Bohr-Rutherford diagram ...
1 Dr. Steve Hawley Volume 35 Number 04 APRIL 2009
1 Dr. Steve Hawley Volume 35 Number 04 APRIL 2009

... who coined the term. Uncertainty aside, all of the panel members spoke eagerly of NASA's Kepler space telescope, which launched on March 7. That mission is designed to search for signs of smaller, rocky planets like Earth among over 100,000 stars. "Let me be bold and say that perhaps planetary scien ...
Astronomy Curriculum
Astronomy Curriculum

... Astronomy is an observational science that deals with the origin, evolution, and interactions of our universe, galaxies, our solar system, and the various objects found therein. Astronomy is a high level elective, with elements of physics and mathematics, intended for those students who wish to furt ...
Scaling the SEM reading
Scaling the SEM reading

... approximately 4.5 billion years ago. The debris from that collision was thrown out into space, and that debris eventually joined together to form the Moon. The newly formed Moon traveled at just the right speed so that it remained within the control of Earth’s gravitational field. Now the Moon is Ea ...
Issue 122 - Aug 2014
Issue 122 - Aug 2014

... When you think about gravitation here on Earth, you very likely think about how constant it is, at 9.8 m/s2 (32 ft/s2). Only, that's not quite right. Depending on how thick the Earth's crust is, whether you're slightly closer to or farther from the Earth's center, or what the density of the material ...
Astronomy DR Packet
Astronomy DR Packet

... Chapter 2, Section 1: Planet Earth Earth’s Gravity 1. ______________ and _____________ orbit each other. This Earth-Moon system orbits the ___________ in a regular path. 2. Earth’s gravity pulls the Moon toward _____________________. Without gravity, the Moon would continue moving in a ____________ ...
Stars - Red, Blue, Old, New pt.3
Stars - Red, Blue, Old, New pt.3

... Jupiter • To about 15-20 times the mass of Jupiter ...
Exoplanets
Exoplanets

... mass to the mass of the Sun (10-3) • The Sun’s wobble due to Jupiter is only 13 m/s • The speed of light is 3x108 m/s • For the Doppler effect: / = v/c • So, we have to detect changes in wavelength  of spectral lines of less than one part in 107 to measure this! • Massive, close-in gas giants ar ...
PHYSICS 110: PHYSICS OF EVERYDAY PHENOMENA
PHYSICS 110: PHYSICS OF EVERYDAY PHENOMENA

... The student will be assessed through class discussion, home work, quizzes, exams, and observatory observations to: (The student will be able to do are noted in this font.) --- identify specific constellations to locate portions of our night sky (look into a clear night sky and in few minutes determi ...
1. The Sun has a surface temperature of about 6000 K.
1. The Sun has a surface temperature of about 6000 K.

... The inner planets are made of rocks and metals. The outer planets also have ices and gasses. Only rocks and metals were solids near the Sun, so the planetesimals were made of rocks and metals. Out farther, ices could freeze onto the dust grains, so they got included in the planetesimals. In addition ...
The Reflector - Peterborough Astronomical Association
The Reflector - Peterborough Astronomical Association

... What probably happened was that he and his friend were looking at Arcturus at high power through the telescope. Because it wasn’t motorized, and the Earth continues rotating, stars move across the field of view, and out of sight. One of my guests at the observatory that night That was what (in his m ...
November 2015 Eyepiece - Amateur Astronomers Association of
November 2015 Eyepiece - Amateur Astronomers Association of

... Venus – Earth’s nearest neighbor is the brightest object in the night sky, after the Moon. Also known by the misnomers “Evening Star” or “Morning Star,” the planet will shine at about -4.0 magnitude, and you can see it in the early morning towards the east. Venus is named for the Roman goddess of lo ...
Common Misconceptions in Astronomy and History
Common Misconceptions in Astronomy and History

... is unable to stop, or consume, the material completely, due to its size, a piece of it will reach the Earth's surface, where it is known as a Meteorite. Meteorites most likely originate from the asteroid belt as rock or ice-rock fragments formed through the collisions of asteroids and comets. Meteo ...
Integrated Science - Syllabus
Integrated Science - Syllabus

... Identify common uses and harmful effects for different EM waves Compare & contrast constructive and destructive waves ...
Life in the galactic danger zone
Life in the galactic danger zone

... factors implicit within them better. “This type of work depends upon numerous observational studies of supernovae, exoplanet searches, protoplanetary discs and the morphology of the Galaxy,” says Gowanlock. “Advanced models of the chemical evolution of the Galaxy and dynamical simulations of planet ...
on his death bed. Retrograde Motion The heliocentric
on his death bed. Retrograde Motion The heliocentric

... *He finally completed the Rudolphine Tables which allowed for accurate prediction of planetary position. *Kepler's accuracy was from 10 to 100 times better than previous tables. ...
RP 4E1 Earth in the Universe - NC Science Wiki
RP 4E1 Earth in the Universe - NC Science Wiki

... What are the predictable patterns caused by Earth’s movement in the solar system? The solar system consists of the sun and a collection of objects of varying sizes and conditions— including planets and their moons—that are held in orbit around the sun by its gravitational pull on them. This system a ...
Big Bang
Big Bang

... • Asteroids - small, solid objects in the Solar System • Comets - small bodies in the Solar System that (at least occasionally) exhibit a coma (or atmosphere) and/or a tail • Meteorites - small extraterrestrial body that reaches the Earth's surface ...
Sparta High School
Sparta High School

... 5.1 Science Practices All students will understand that science is both a body of knowledge and an evidence-based, model-building enterprise that continually extends, refines, and revises knowledge. The four Science Practices strands encompass the knowledge and reasoning skills that students must ac ...
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Astrobiology



Astrobiology is the study of the origin, evolution, distribution, and future of life in the universe: extraterrestrial life and life on Earth. This interdisciplinary field encompasses the search for habitable environments in our Solar System and habitable planets outside our Solar System, the search for evidence of prebiotic chemistry, laboratory and field research into the origins and early evolution of life on Earth, and studies of the potential for life to adapt to challenges on Earth and in outer space. Astrobiology addresses the question of whether life exists beyond Earth, and how humans can detect it if it does. (The term exobiology is similar but more specific—it covers the search for life beyond Earth, and the effects of extraterrestrial environments on living things.)Astrobiology makes use of physics, chemistry, astronomy, biology, molecular biology, ecology, planetary science, geography, and geology to investigate the possibility of life on other worlds and help recognize biospheres that might be different from the biosphere on Earth. The origin and early evolution of life is an inseparable part of the discipline of astrobiology. Astrobiology concerns itself with interpretation of existing scientific data; given more detailed and reliable data from other parts of the universe, the roots of astrobiology itself—physics, chemistry and biology—may have their theoretical bases challenged. Although speculation is entertained to give context, astrobiology concerns itself primarily with hypotheses that fit firmly into existing scientific theories.The chemistry of life may have begun shortly after the Big Bang, 13.8 billion years ago, during a habitable epoch when the Universe was only 10–17 million years old. According to the panspermia hypothesis, microscopic life—distributed by meteoroids, asteroids and other small Solar System bodies—may exist throughout the universe. According to research published in August 2015, very large galaxies may be more favorable to the creation and development of habitable planets than smaller galaxies, like the Milky Way galaxy. Nonetheless, Earth is the only place in the universe known to harbor life. Estimates of habitable zones around other stars, along with the discovery of hundreds of extrasolar planets and new insights into the extreme habitats here on Earth, suggest that there may be many more habitable places in the universe than considered possible until very recently.Current studies on the planet Mars by the Curiosity and Opportunity rovers are now searching for evidence of ancient life as well as plains related to ancient rivers or lakes that may have been habitable. The search for evidence of habitability, taphonomy (related to fossils), and organic molecules on the planet Mars is now a primary NASA objective on Mars.
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