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Space – Align the Stars - VUTechieTeacher
Space – Align the Stars - VUTechieTeacher

... Space – Align the Stars 1. The sun, together with all the planets, asteroids, comets, and meteors that orbit around it, collectively make up our _____________. ...
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... final phase of stellar evolution. A total of 58 hours of exposure time have gone in to creating this deep view of the nebula. The white dot at the Helix's center is this Planetary Nebula's hot, central star. ...
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Foundation 1 - Discovering Astronomy

... As the temperature in the interior rises, nuclear reactions produce outward force and balances the inward force of gravity  hydrostatic equilibrium = star becomes stable and contraction stopsmain-sequence star ...
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... the fraction of stars that have “habitable planets” the number of habitable planets per system the fraction of habitable planets where life evolves the fraction of life-planets that evolve intelligence the fraction of civilizations that communicate the fraction of the star’s life that the civilizati ...
Digital Moon - Net Start Class
Digital Moon - Net Start Class

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PHYS 1470 3.0 W16/17 Highlights of Astronomy Assignment #2
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... • Craters like the Imbrium Basin are older than the lunar maria and craters like Erostathenes – This period of muilti-ring craters and extrusions of the lunar maria is known as the Imbrium Period Ejecta from the Imbrium Basin overlap craters like the Nectarian Basin in the lunar highlands. ...
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... contraction continues at a rapid pace. This causes the center to heat more intensely than the outer layers. When the core of a protostar reaches 10 million K, pressure within is so great that nuclear fusion of hydrogen begins. A Star is born. ...
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... no erosion has taken place on its surface. We see Mercury much the way it was soon after it formed. Core We learned that Mercury has an extremely weak magnetic field, which could indicate a hot metallic core, such as molten iron. Geologists think Mercury may be the most iron-rich planet in the solar ...
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Lightest exoplanet found in nearest star system to Earth

... The planet was detected using the HARPS instrument on the 3.6-meter telescope at ESO's La Silla Observatory in Chile. Alpha Centauri is one of the brightest stars in the southern skies and is the nearest stellar system to our solar system-only 4.3 light-years away. It is actually a triple star-a sys ...
Jupiter - Trimble County Schools
Jupiter - Trimble County Schools

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Formation and evolution of the Solar System



The formation of the Solar System began 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud. Most of the collapsing mass collected in the center, forming the Sun, while the rest flattened into a protoplanetary disk out of which the planets, moons, asteroids, and other small Solar System bodies formed.This widely accepted model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.The Solar System has evolved considerably since its initial formation. Many moons have formed from circling discs of gas and dust around their parent planets, while other moons are thought to have formed independently and later been captured by their planets. Still others, such as the Moon, may be the result of giant collisions. Collisions between bodies have occurred continually up to the present day and have been central to the evolution of the Solar System. The positions of the planets often shifted due to gravitational interactions. This planetary migration is now thought to have been responsible for much of the Solar System's early evolution.In roughly 5 billion years, the Sun will cool and expand outward many times its current diameter (becoming a red giant), before casting off its outer layers as a planetary nebula and leaving behind a stellar remnant known as a white dwarf. In the far distant future, the gravity of passing stars will gradually reduce the Sun's retinue of planets. Some planets will be destroyed, others ejected into interstellar space. Ultimately, over the course of tens of billions of years, it is likely that the Sun will be left with none of the original bodies in orbit around it.
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