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ppt
ppt

... actually much closer to 290 K Atmospheric greenhouse effect serves to keep the temperature higher (also a very tiny heating effect due to geothermal heat) ...
Chapter 1 Periods of Western Astronomy Prehistoric Astronomy
Chapter 1 Periods of Western Astronomy Prehistoric Astronomy

... Kepler’s 3rd Law • This law implies that a planet with a larger average distance from the Sun, which is the semimajor axis distance, will take longer to circle the Sun • Third law hints at the nature of the force holding the planets in ...
Name
Name

... A) The rate that visible light from the Sun is being absorbed by the Earth’s atmosphere B) The rate that gamma rays are hitting the Earth’s atmosphere C) The rate that hydrogen is being fused into helium in the Sun D) The rate that white dwarfs are being formed in the galaxy E) The rate that stars f ...
Wilmslow Guild Lecture 2008
Wilmslow Guild Lecture 2008

... possible to establish absolute distances and the size our galaxy. Many astronomers were involved in this process, and the final shape and distribution emerged in the 1930’s. Our Galaxy has a lens-shaped spiral construction, 16,000 light years thick at the centre and 3,000 light years thick at the po ...
September - City School District of Albany
September - City School District of Albany

... - These motions explain such phenomena as the day, the year, seasons, phases of the moon, eclipses, and tides. - Gravity influences the motions of celestial objects. The force of gravity between two objects in the universe depends on their masses and the distance between them. ____1.1b 8 planets mov ...
Extrasolar planets Topics to be covered Planets and brown dwarfs
Extrasolar planets Topics to be covered Planets and brown dwarfs

... • But if we take metallicity into account: – >20% of stars with 3x the metal content of the Sun have planets – only ~3% of stars with 1/3rd of the Sun’s metallicity have planets ...
Jupiter`s Galilean Moons
Jupiter`s Galilean Moons

... amounts of ice and rock. Recent data, however, suggests a more complex core as shown here (bottom right). The surface layers of Ganymede and Callisto are shown as white to indicate that they may differ from the underlying ice/rock layers in a variety of ways including, for example, the percentage of ...
13 - Joe Griffin Media Ministries
13 - Joe Griffin Media Ministries

... this a couple of times while explaining the Carousel. The Enochian School teaches that the starry story begins with Virgo (virgin birth) and ends with Leo (Second Advent) and in between is the angelic conflict being resolved by fulfillment of the Lord’s prophecy in Genesis 3:15. It is quite possible ...
The New Astronomy and Cosmology of the Scientific Revolution
The New Astronomy and Cosmology of the Scientific Revolution

... Tycho Brahe (1546–1601) was the court astronomer to Holy Roman Emperor Rudolf II. Tycho’s impact on astronomy was considerable. He developed numerous instruments to improve the accuracy of astronomical observation, and conducted extremely meticulous empirical observations of the heavens. He discover ...
Rotation
Rotation

... determines the amount of light reflected by the Moon. C. The season of the year determines the phase of the Moon. D. The closer the Moon is to Earth, the more light the Moon ...
Day 3
Day 3

... We highlight the importance of gaseous TiO and VO opacity on the highly irradiated close-in giant planets. The dayside atmospheres of these planets naturally fall into two classes that are somewhat analogous to the M- and L-type dwarfs. Those that are warm enough to have appreciable opacity due to T ...
October 2015 - John J. McCarthy Observatory
October 2015 - John J. McCarthy Observatory

... higher quality and larger than can be produced on Earth. The most powerful medical research tool on the ISS may be its microgravity. Since 2003, the Japan Aerospace Exploration Agency, or JAXA, has been conducting protein crystallization experiments, most recently with the support of the Russian Fed ...
Introduction to Basic Stargazing Part II - Naples Free-Net
Introduction to Basic Stargazing Part II - Naples Free-Net

... astronomical unit (au) – one au is defined as the average distance from Earth to the Sun. There are two reasons for this; 1. It greatly improves computational ease of raw data. 2. It improves comprehension of relative distances. For example, the astronomical unit is measured at 92,956,000 miles. If ...
PDF file
PDF file

... data matched with Copernicus’s theory. • Realized that the orbits cannot be perfect circles. The orbits were elliptical. • Discovered 3 mathematical laws of planetary motion. ...
Atmospheric biomarkers on terrestrial exoplanets Abstract Introduction
Atmospheric biomarkers on terrestrial exoplanets Abstract Introduction

... have been detected around 107 main sequence stars1 . As the detection of a planet requires observations made over a time comparable to its period, most of them have a short period. The radial velocity method has recently been used successfully to reveal outer planets at the same orbital distance as ...
The James Webb Space Telescope: A Vision for the Future
The James Webb Space Telescope: A Vision for the Future

... The universe began 13.8 billion years ago as an expanding fireball. But how did stars and galaxies arise from this raw fury? Webb’s vision will be able to witness the flicker of the first galaxies popping into existence in the early universe. Continued, page 6… ...
Jupiter - Mrs Foos, Room 10
Jupiter - Mrs Foos, Room 10

... Jupiter, the fifth planet in our Solar System, is about 778 million kilometers (484 million miles) from the Sun. The average temperature on Jupiter is about –148ºC (–234ºF). Its atmosphere consists mainly of hydrogen and helium. How Big Is Jupiter? Known as the king of the planets, Jupiter is the la ...
About Uranus - COSTA VERDE production
About Uranus - COSTA VERDE production

... It mainly consists of 83% hydrogen (H), 15 % helium (He) and 1.9 % Methane (CH4) and is an ice giant, which is a subspecies of the gas giants, as it is mostly composed of ice and rock as well as gases. ...
Lesson 7
Lesson 7

... sun, or feed around the sun. None of those choices make sense. The Earth does circle around the sun. In Number three, did you remember to write in a complete statement? I hope so! “Why is Earth called the Life Planet?” (Response: Scientists believe Earth is the only planet where plants, animals, and ...
The Planets - Guild of Students
The Planets - Guild of Students

... Venus is sometimes regarded as Earth's sister planet. In some ways they are very similar. Venus is only slightly smaller than Earth (95% of Earth's diameter, 80% of Earth's mass). Both have few craters indicating relatively young surfaces. Their densities and chemical compositions are similar. Since ...
Universe and Stars Project Final Due Date
Universe and Stars Project Final Due Date

... 1. Describe how the Universe was formed and provide at least 3 pieces of evidence of the Big Bang. ( LT A) Make sure you include what red shift and steady state means. http://www.schoolsobservatory.org.uk/astro/cosmos/bb_evid 2. Describe scientific explanations and conditions that explain and contri ...
Earth - Mrs. Christov`s Physical Geography Class
Earth - Mrs. Christov`s Physical Geography Class

... HUMAN- ENVIRONMENT INTERACTION: the effects of human activities on the environment, as well as the impacts of environmental processes on humans, have become topics of increasing concern. ...
3 Biology and Geology 3. Secondary Education
3 Biology and Geology 3. Secondary Education

... Earth: the fish, the algae, etc., which live in the hydrosphere; the birds, the insects, etc., in the atmosphere; and the mammals, reptiles, spiders, plants, etc., which are on and in the crust of the geosphere. Biology and Geology 3. Secondary Education ...
Working with the Illinois Learning Standards: A Constructivist
Working with the Illinois Learning Standards: A Constructivist

... • use a globe and a light bulb to simulate the earth and sun; illustrate day and night, and rotation and revolution • using a light bulb as the sun, have children spin in place to simulate rotation; students should watch for “rising” and “setting” of the sun as they rotate • chart the position of th ...
Partial Solar Eclipse Watch Party
Partial Solar Eclipse Watch Party

... a partial solar eclipse. We had telescopes and cameras set up to safely view the Sun. Solar glasses were available for purchase in the ticket booth. News stations from across the Metroplex joined the public and Planetarium staff to watch this rare event. Among the news stations covering the event we ...
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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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