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Lecture 2+3 - University of Texas Astronomy Home Page
Lecture 2+3 - University of Texas Astronomy Home Page

... - Nuclear fusion occurs in core where temp and pressure are very high. - The energy released is transported from core to the cooler surface (called photosphere) where it is released as light and heat. This is the ‘surface’ where visible yellow light from the Sun comes from. ...
New Corroboration of Meier`s Information Regarding Other Planets
New Corroboration of Meier`s Information Regarding Other Planets

... period of 3,600 years. Unfortunately, I am unable to describe the planet Vulcan/Volkano any better than I can the two outer planets -- Transpluto and UNI -- because I have never been given any descriptions about them. I was informed, however, that Vulcan/Volkano, the planet closest to the sun, previ ...
Integrative Studies 410 Our Place in the Universe
Integrative Studies 410 Our Place in the Universe

... • Cloud contracts/warms, begins radiating; almost all radiated energy escapes • Cloud becomes dense  opaque to radiation  radiated energy trapped  core heats up ...
Chapter 24 Test:Stars/Galaxies
Chapter 24 Test:Stars/Galaxies

... The positions of the constellations appear to change throughout the year because _____. (a) the sun revolves around the galaxy, (b) Earth revolves around the sun, (c) the constellations revolve around Earth, (d) Earth revolves around the stars. ...
01D)EA~1
01D)EA~1

... and sometimes fall back relative to one another (this is called retrograde motion) but this is due to their different speeds and positions in our Solar System. ...
Stars - Images
Stars - Images

... Ways of tracking where the constellations are located during the different seasons of the year. Remember as the earth revolves around the sun, it also rotates causing the stars to “shift” in the ...
astr100_finalexam
astr100_finalexam

... D) clouds in its atmosphere reflect sunlight back into space [13] Which of the following is NOT explained by the Solar Nebula theory? A) common rotation of most of the planets B) the number of moons each planet has C) common age of Solar System objects D) different composition of inner and outer pl ...
Level 1 Solar system, Planets, Sun, Asteroid belt, Kuipler belt and
Level 1 Solar system, Planets, Sun, Asteroid belt, Kuipler belt and

... 3. Like Earth, Mars has seasons, polar ice caps, volcanoes, canyons and weather, but its atmosphere is too thin for liquid water to exist for long on the surface. 4. There are signs of ancient floods on Mars, but evidence for water now exists mainly in icy soil and thin clouds. ...
Where to Look: Habitable Zones
Where to Look: Habitable Zones

... “The receipt of a message from an advanced civilization will show that there are advanced civilizations, that there are methods of avoiding the self-destruction that seems so real a danger of our present technological adolescence. Finding a solution to a problem is helped enormously by the certain k ...
Before Humankind - Salem State University
Before Humankind - Salem State University

... for billions of years. When hydrogen atoms in their core fuse together under pressure and heat, they become helium atoms. This process is called fusion. After billions of years stars cool and collapse and become supernova. Debris from their collapse heats up again and a cloud of hot hydrogen and hel ...
The Origin of the Solar System and Other Planetary Systems
The Origin of the Solar System and Other Planetary Systems

... figure but are numerous. Stars with composition like our Sun are much more likely to have planets, showing that the “dusty disk” theory of solar system formation is plausible. Some of these “planets” may actually be brown dwarfs (i.e. a large body not quite large enough to be a star), but probably n ...
pdf version
pdf version

... that the young solar system must have been filled very early with colliding planetary embryos known as ‘‘planetesimals’’. In Chapter 3, we have attempted to describe in a simplified fashion the chronology of the evolution of the solar system, starting with the birth of its parent star, our Sun, and en ...
Lecture9_2014_v2 - UCO/Lick Observatory
Lecture9_2014_v2 - UCO/Lick Observatory

... replenished by collisions of rocky bodies. ...
Mountain Skies March 7 2016
Mountain Skies March 7 2016

... Mercury in the evening sky, Jupiter is rising right about sunset. Look for it low in the east as the sun sets in the west. Until a waxing crescent moon enters the evening sky later this week, Jupiter is the brightest object in the evening sky. In fact, tonight Jupiter is at opposition which means it ...
February 18
February 18

... • As a planet moves around its orbit, it sweeps out equal areas in equal times. • This means that the planet travels faster when it is nearer the Sun and slower when it is farther from the Sun ...
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... no beginning and will continue forever. Although the universe is expanding, it maintains its average density – steady-state – through the continuous creation of new matter. Most cosmologists now reject the theory because it cannot explain background radiation or the observation that the appearance o ...
Notes: Astronomy and Groups of Stars
Notes: Astronomy and Groups of Stars

... The core of stars is very hot. The temperatures observed are of the outer layer of the star. ...
Part 2 Answer Key
Part 2 Answer Key

... Star Clusters are multiple star systems bound together by the force of gravity. Star Clusters can be divided into two main groups. One group is called Globular Clusters. They contain many stars and gravity holds them tightly together. They swarm just outside the galaxy and form a halo or bulge. We k ...
Origin of the Solar System – Notes Rings encircle Jupiter, Saturn
Origin of the Solar System – Notes Rings encircle Jupiter, Saturn

... and ice, are called comets. When a comet comes close enough to the Sun, the Sun’s radiation vaporizes some of the comet’s ices, producing long flowing tails of gas and dust particles. Some comets appear to originate from locations far beyond the Kuiper belt. The source of these is thought to be a sw ...
The Future of Life on Earth Over the Next Few Billion Years
The Future of Life on Earth Over the Next Few Billion Years

... We will eventually find planets that are like the Earth, but much older ...
Intro To The Solar System
Intro To The Solar System

... Earth has diameter 0.3 mm. Sun: ~ size of a small plum. Mercury, Venus, Earth, Mars: ~ size of a grain of salt. Jupiter: ~ size of an apple seed. Saturn: ~ slightly smaller than Jupiter’s “apple seed”. ...
Solar System PPT
Solar System PPT

... Way, which is among billions of galaxies that make up the universe ...
the universe
the universe

... The Universe Scientists have gathered a lot of evidence and information about the universe. They have used their observations to develop a theory called the Big Bang. The theory states that about 13,700 million years ago all the matter in the universe was concentrated into a single incredibly tiny p ...
Fulltext PDF - Indian Academy of Sciences
Fulltext PDF - Indian Academy of Sciences

... them the music of the spheres 13, attributing specific notes to the various planets. He said that there was no audible sound there but that “the movements of the planets are modulated according to harmonic proportions.” By his painstaking analysis of the data on the orbit of Mars, which had been col ...
the universe
the universe

... The Universe (source: www.bbc.co.uk/bitesize/gcse/science /) Scientists have gathered a lot of evidence and information about the universe. They have used their observations to develop a theory called the Big Bang. The theory states that about 13,700 million years ago all the matter in the universe ...
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Planetary habitability



Planetary habitability is the measure of a planet's or a natural satellite's potential to develop and sustain life. Life may develop directly on a planet or satellite or be transferred to it from another body, a theoretical process known as panspermia. As the existence of life beyond Earth is unknown, planetary habitability is largely an extrapolation of conditions on Earth and the characteristics of the Sun and Solar System which appear favourable to life's flourishing—in particular those factors that have sustained complex, multicellular organisms and not just simpler, unicellular creatures. Research and theory in this regard is a component of planetary science and the emerging discipline of astrobiology.An absolute requirement for life is an energy source, and the notion of planetary habitability implies that many other geophysical, geochemical, and astrophysical criteria must be met before an astronomical body can support life. In its astrobiology roadmap, NASA has defined the principal habitability criteria as ""extended regions of liquid water, conditions favourable for the assembly of complex organic molecules, and energy sources to sustain metabolism.""In determining the habitability potential of a body, studies focus on its bulk composition, orbital properties, atmosphere, and potential chemical interactions. Stellar characteristics of importance include mass and luminosity, stable variability, and high metallicity. Rocky, terrestrial-type planets and moons with the potential for Earth-like chemistry are a primary focus of astrobiological research, although more speculative habitability theories occasionally examine alternative biochemistries and other types of astronomical bodies.The idea that planets beyond Earth might host life is an ancient one, though historically it was framed by philosophy as much as physical science. The late 20th century saw two breakthroughs in the field. The observation and robotic spacecraft exploration of other planets and moons within the Solar System has provided critical information on defining habitability criteria and allowed for substantial geophysical comparisons between the Earth and other bodies. The discovery of extrasolar planets, beginning in the early 1990s and accelerating thereafter, has provided further information for the study of possible extraterrestrial life. These findings confirm that the Sun is not unique among stars in hosting planets and expands the habitability research horizon beyond the Solar System.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. 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. On 4 November 2013, astronomers reported, based on Kepler space mission data, that there could be as many as 40 billion Earth-sized planets orbiting in the habitable zones of Sun-like stars and red dwarfs within the Milky Way. 11 billion of these estimated planets may be orbiting Sun-like stars. The nearest such planet may be 12 light-years away, according to the scientists.
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