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class slides for Chapter 4
class slides for Chapter 4

... dimming of the parent star’s luminosity. ...
The Search for Another Earth
The Search for Another Earth

... it is quite rational to speculate that some of those planets orbiting other stars might be habitable. The search for planets outside the solar system, termed as extrasolar planets or exoplanets, started during the nineteenth century. But the necessary technology to detect even a large planet similar ...
Earth Science Exams and Keys 2014 Season
Earth Science Exams and Keys 2014 Season

... 60. Which statement best describes how are galaxies distributed in space? A) the galaxies lie on sheets and chains surrounding empty space B) the galaxies are distributed uniformly in space C) there are a few large clusters of galaxies with nothing in between D) there are many clusters of galaxies n ...
Our Place in a Vast Universe
Our Place in a Vast Universe

... rest and that it was the earth that revolved around the sun. (This reference makes Aristarchus the first person to propose the heliocentric theory, that the sun is at the center of the solar system.) In order to avoid observable changes in angles between the directions to the stars as the earth move ...
Earth Science Spring Break Packet 2016
Earth Science Spring Break Packet 2016

... C. supplies the oxygen living organisms require to carry on respiration. D. traps heat close to Earth's surface to maintain temperatures necessary for life. ...
Star Classification and its Connection to Exoplanets.
Star Classification and its Connection to Exoplanets.

... the pie, so the viewer can see the result: G classified (sun-like) stars have the majority of the exoplanets, at 38%. The second pie chart uses data from the percentage of stars that have planets, so at around 6.6% of a total of around 18%, G stars make up about 37%, again the dominant planet host. ...
Astronomy - Core Knowledge Foundation
Astronomy - Core Knowledge Foundation

... (Sadler, 1987). At this early grade level, students are  help to reinforce and extend learning about the  not expected to explain the seasons or the cause of  nature of light and the sun.  the phases of the moon Instead, they will be focusing  on the development of key terms and language that  Misco ...
Mission 1 - NC State University
Mission 1 - NC State University

... in the sky are much further away from us than the Sun. Their long distance away from us is the reason they look like tiny points of light in the night sky. We measure the distance of stars from Earth in light years. A light year is the distance that light travels in one year. Since light travels at ...
Pluto_Ceres_ASP
Pluto_Ceres_ASP

... that Ceres is a planet by the above scientific definition. For historical reasons, one may choose to distinguish Ceres from the classical planets by referring to it as a “dwarf planet.” ...
StarFlight - Center for the Presentation of Science
StarFlight - Center for the Presentation of Science

... subjects: (1) the Solar System, and (2) common constellations. The form of the evaluation was an open-ended discussion where we asked people to draw the Solar System and any constellations they could remember, and then explain what they drew. We collected 10 interviews during one afternoon at the Mu ...
4-eclipses-and-tides
4-eclipses-and-tides

... 26. Base your answer to the following question on the passage below. A Newly Discovered Planet Scientists studying a Sun-like star named Ogle-Tr-3 discovered a planet that is, on the average, 3.5 million kilometers away from the star’s surface. The planet was discovered as a result of observing a c ...
Lecture 6
Lecture 6

... • Study orbital preriods  get masses - planets around Sun  Sun’s mass - Jupiter’s moons around Jupiter  Jupiter’s mass • Also used for stars (more on this later) - two nearby stars orbiting each other  their masses - an exoplanet orbiting a star will cause the star to wobble a bit  can give mas ...
American Scientist
American Scientist

... Solar System, is not really needed to form exoplanetary systems populated by close-in super Earths—Earthlike exoplanets somewhat larger than our Earth, which seem to be an omnipresent breed. Our Solar System appears not to be the dominant outcome of planet formation and it may be exerting a provinci ...
FREE Sample Here
FREE Sample Here

... Figure 0.9 is also an important one. Make sure students understand that it shows the apparent path of the Sun on the celestial sphere. Use models of Earth and the Sun (or just two spheres) to help explain how Earth’s tilt changes the position of the Sun in the sky as Earth orbits the Sun. Emphasize ...
4-eclipses-and-tides
4-eclipses-and-tides

... 26. Base your answer to the following question on the passage below. A Newly Discovered Planet Scientists studying a Sun-like star named Ogle-Tr-3 discovered a planet that is, on the average, 3.5 million kilometers away from the star’s surface. The planet was discovered as a result of observing a c ...
Time From the Perspective of a Particle Physicist
Time From the Perspective of a Particle Physicist

... • Study orbital preriods  get masses - planets around Sun  Sun’s mass - Jupiter’s moons around Jupiter  Jupiter’s mass • Also used for stars (more on this later) - two nearby stars orbiting each other  their masses - an exoplanet orbiting a star will cause the star to wobble a bit  can give mas ...
University of Arizona Department of Astronomy
University of Arizona Department of Astronomy

... gravity somewhere in space that pulls a bunch of little space particles together and they all collide somewhere in the middle of all this gravity and wham bam. .” Early work comprising part of Janelle Bailey’s PhD dissertation ...
July 2008 - Warren Astronomical Society
July 2008 - Warren Astronomical Society

... the WASP is e-mailed to each member and/or is available online at warrenastronomicalsociety.org. Requests by other Astronomy clubs to receive the WASP, and all other correspondence should be addressed to the Publications Director, Larry Phipps, at [email protected]. Articles for inclusion in the WA ...
Earth Moon Sun System PPT
Earth Moon Sun System PPT

... -Solar Day: relative to the Sun, when the Sun returns to its original position in the sky (when a position on Earth realigns with the Sun – 24 hours -Sidereal Day: relative to distant stars, when a star other than the Sun returns to its original position in the night sky (when a position on Earth re ...
Project Icarus: Astronomical Considerations Relating to the Choice
Project Icarus: Astronomical Considerations Relating to the Choice

... (1)Science to be conducted on route, e.g. of the local interstellar medium (LISM), and physical and astrophysical studies which could make use of the Icarus vehicle as an observing platform; (2)Astrophysical studies of the target star itself, or stars if a multiple system is selected; (3)Planetary s ...
Earth Moon Sun System PPT
Earth Moon Sun System PPT

... -Solar Day: relative to the Sun, when the Sun returns to its original position in the sky (when a position on Earth realigns with the Sun – 24 hours -Sidereal Day: relative to distant stars, when a star other than the Sun returns to its original position in the night sky (when a position on Earth re ...
ph709-14
ph709-14

... Analysis of Hubble Space Telescope data indicated that planets were only beginning to form around Beta Pictoris, a very young star at between 20 million and 100 million years old. Most dust grains in the disk are not agglomerating to form larger bodies; instead, they are eroding and being moved away ...
Sun - Cobb Learning
Sun - Cobb Learning

... 14. The precession of Earth's rotational axis causes the location of the a. north celestial pole and south celestial pole to change. b. vernal equinox and autumnal equinox to change. c. summer solstice and winter solstice to change. d. Both a and b above. e. All of the above. ...
i. relative age of rock strata or events
i. relative age of rock strata or events

... ANOTHER DEAD SMART GUY (with a really neat name): TYCHO BRAHE *RECORDED EXTENSIVE OBSERVATIONS OF C.B. OVER 20 YRS. *HAD A METAL NOSE ...
1 Lecture 8: Uranus and Neptune
1 Lecture 8: Uranus and Neptune

... – low amount of high level clouds means that weather patterns cannot readily be seen as they are blocked out how high atmospheric haze – high winds 200 km/h to 500 km/h do form bands like Jupiter, but are buried deeper in the atmosphere – Hubble Space Telescope discovered small dark spot indicating ...
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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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