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Primordial planets, comets and moons foster life in the cosmos
Primordial planets, comets and moons foster life in the cosmos

... would be extremely rare and confined to local star systems. For HGD cosmology (Fig. 2 bottom), the 1013 -1016 s interval has many stars and warm planets, and is the optimum time period for life to appear and for its first seeds to be widely scattered on cosmic scales. Plasma-protogalaxies form near ...
Animated Science Space Revision
Animated Science Space Revision

... Some asteroids have orbits that pass close to Earth and some even hit it. About 65 million years ago, an asteroid landed in Mexico. We think it caused the climate to change. This meant that dinosaurs could not survive. The four outer planets are sometimes called the gas giants. They are made mainly ...
update : Feb.27,2014
update : Feb.27,2014

... Need to be in the right kind of solar system with a Jupiter size planet at the right distance to remove much of debris from system to reduce impacts on earth not close enough to significantly affect Earth’s orbit ...
SOLAR SYSTEM OVERVIEW - Ms. Ferebee`s Webpage
SOLAR SYSTEM OVERVIEW - Ms. Ferebee`s Webpage

... The inner planets: Mercury, Venus, Earth, and Mars. Mercury is closest to the Sun and Mars is the most distant of these rocky planets. Earth is the only place in the solar system or the universe known to have life. This is because Earth has liquid water, oxygen and a protective atmosphere. ...
Opposition of Saturn - Hong Kong Observatory
Opposition of Saturn - Hong Kong Observatory

... Figure 1      Relative positions of a superior planet, the Earth and the Sun during opposition and conjunction of the superior planet.  Opposition of Saturn  Saturn is the second largest planet in the Solar System and the sixth planet away from the Sun. Saturn is characterized by the Saturn ring, wh ...
The MAS Winter Schedule February 21st: Membership Meeting at
The MAS Winter Schedule February 21st: Membership Meeting at

... to melt iron (2,700°F); the night side is much to obtain measurements of the planet over three “cooler”—at 900°F it would “only” melt lead. nearly consecutive orbits with Wide Field Camera Because heat is so poorly distributed through its 3. They also acquired data from three primary atmosphere, fie ...
Solar System Lesson Organizer
Solar System Lesson Organizer

... Prior to listening to a read aloud, students will identify what they know and have learned that may be related to the specific story or topic to be read aloud. Students will retell key details. Prior to listening to a read aloud, students will identify what they know and have learned that may be rel ...
Abstract - The University of Akron
Abstract - The University of Akron

... system. In 1969, two new space probes, named Pioneer 10 and 11, were designed and built to travel through the asteroid belt toward Jupiter and Saturn and onward. Both the spacecraft and their trajectories were designed to eventually escape the solar system and become the first man-made objects inten ...
1 Exoplanets 2 Types of Exoplanets
1 Exoplanets 2 Types of Exoplanets

... Exoplanets are a hot topic in astronomy right now. As of January, 2015, there are over 1500 confirmed exoplanet discoveries with more than 3000 candidates still waiting to be confirmed. These exoplanets and exoplanet systems are of extreme interest to astronomers as they provide insights into planet ...
View PDF - Sara Seager
View PDF - Sara Seager

... atmospheres orbiting main-sequence stars [see (10) or sizes, orbits, and host star type. The diversity extends to new kinds of planets, which are very and references therein]. This article reviews upcommon yet have no solar system counterparts. Even with the requirement that a planet’s surface dates ...
Detecting the glint of starlight on the oceans of distant planets
Detecting the glint of starlight on the oceans of distant planets

... terms of Eq. (6). The model light curves (thick black line—0% clouds, dashed line—50% clouds) are smoothed fits to the results of 72 diurnally-averaged, whole-disk integrations of reflected light. Here, the orbit is viewed edge-on and the disk-centered latitude is the Tropic of Cancer. Earth geograp ...
Chapter 3: Galileo, Newton, and Einstein
Chapter 3: Galileo, Newton, and Einstein

... shape every point of which is the same total distance from two fixed points (the foci). Eccentricity is the distance between the foci and its center divided by half the longest distance across (semi-major axis). ...
Revolutions of Earth
Revolutions of Earth

... Although Copernicus’ model was simpler –it didn’t need epicycles and deferents - it still did not perfectly describe the motion of the planets. Johannes Kepler solved the problem a short time later when he determined that the planets moved around the Sun in ellipses (ovals), not circles ( Figure 1.2 ...
timeline
timeline

... 3000 BCE - Babylonian astrologer-astronomers begin making methodical observations of the skies 2000 BCE - Babylonians develop a zodiac 1300 BCE - Chinese use of firework-rockets becomes widespread 1000 BCE - Babylonians record sun/moon/planetary movements Egyptians use sun-clock 600-400 BCE - Pythag ...
A Triple Conjunction
A Triple Conjunction

... Any pair of superior planets (that is, planets outside the Earth’s orbit) can give rise to a triple conjunction whereby, instead of a single pass, the planets meet and separate three times over a period of a few months. The more exterior a pair of planets are, the more frequent are triple conjunctio ...
Grade 5 ELA Life on a New Planet
Grade 5 ELA Life on a New Planet

... which share some of the traits of Earth and Mars. However, in our own solar system no signs of life have yet been found. With the extreme size and scope of the universe, that is likely to change. It may also change sooner than we think. According to astronomers, or scientists who study space, it is ...
Planet Jupiter - Rocky View Schools
Planet Jupiter - Rocky View Schools

... atmosphere of clouds. One discovery that these probes made was the detection of Jupiter’s thin and delicate ring structure, which is not visible from the Earth. The probes also detected many new satellites, and along with recent discoveries we now know of 52 moons in orbit around Jupiter, the most o ...
Is our solar system unique?
Is our solar system unique?

... show us that stars and disks are all very different from each other. And, they gave us the surprising observation of outflows. Simulations also agree with theory, but they can’t model everything at once, and there are some problems (things take too long, for one) ...
How did the Solar System form?
How did the Solar System form?

... •  If there’s ice around (> 5 AU from the star, where it’s cold) the cores are bigger. If big enough, they’ll suck gas out of the disk and form giant planets •  Moons form via collision or capture or in mini disks ...
Lecture 7 Gravity and satellites
Lecture 7 Gravity and satellites

... gravitational field strength at that location, the motion of the object could be considered as free falling. A person during free falling would experience apparent weightlessness (a = g and N = 0) Motion of the planets A satellite is an object that is in a stable orbit around a more massive central ...
Secular Increase of the Astronomical Unit: a Possible Explanation in
Secular Increase of the Astronomical Unit: a Possible Explanation in

... existence of dAU=dt has not been confirmed robustly in terms of an independent analysis of observations by other ephemeris groups, it is important not only to perform theoretical studies, but also to re-analyze the data and to obtain a more accurate value of dAU=dt by adding new observations, e.g., ...
Astronomy - Learn Earth Science
Astronomy - Learn Earth Science

... If an object is moving toward you, the waves get scrunched together and get (longer, shorter). If an object is moving away from you, the waves appear to spread out and get (longer, shorter). ...
Revolutions of Earth
Revolutions of Earth

... Although Copernicus’ model was simpler – it didn’t need epicycles and deferents - it still did not perfectly describe the motion of the planets. Johannes Kepler solved the problem a short time later when he determined that the planets moved around the Sun in ellipses (ovals), not circles (Figure 1.2 ...
Stellar Astronomy Sample Questions for Exam 3
Stellar Astronomy Sample Questions for Exam 3

... 1. Briefly describe the nebular model for the formation of the solar system. Include details about the formation of both the central star and the planets around it. 2. Describe some of the evidence we have for how we think solar systems like ours form. Where do they form? What types of objects have ...
Teacher Resource Pack Unit Planning Resources
Teacher Resource Pack Unit Planning Resources

... much younger than our sun. Most of them apparently are not an isolated single star as our sun is but are part of systems of two or more stars orbiting around a common center of mass. So too there are other galaxies and clusters of galaxies different from our own in size, shape, and direction of moti ...
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IAU definition of planet



The definition of planet set in Prague in 2006 by the International Astronomical Union (IAU) states that, in the Solar System, a planet is a celestial body which: is in orbit around the Sun, has sufficient mass to assume hydrostatic equilibrium (a nearly round shape), and has ""cleared the neighborhood"" around its orbit.A non-satellite body fulfilling only the first two of these criteria is classified as a ""dwarf planet"". According to the IAU, ""planets and dwarf planets are two distinct classes of objects"". A non-satellite body fulfilling only the first criterion is termed a ""small Solar System body"" (SSSB). Initial drafts planned to include dwarf planets as a subcategory of planets, but because this could potentially have led to the addition of several dozens of planets into the Solar System, this draft was eventually dropped. The definition was a controversial one and has drawn both support and criticism from different astronomers, but has remained in use.According to this definition, there are eight planets in the Solar System. The definition distinguishes planets from smaller bodies and is not useful outside the Solar System, where smaller bodies cannot be found yet. Extrasolar planets, or exoplanets, are covered separately under a complementary 2003 draft guideline for the definition of planets, which distinguishes them from dwarf stars, which are larger.
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