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Habitability and Life Parameters in our Solar System
Habitability and Life Parameters in our Solar System

... 2001 paper by Gonzalez, Brownlee, and Ward, did not demarcate any specific boundaries, merely stating that the zone was an annulus encompassing a region of the galaxy that was both enriched with metals and spared from excessive radiation, and that habitability would be more likely in the galaxy’s th ...
Chapter 2. Discovering the Universe for Yourself
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... telescope would make a difference, illustrating a misconception about telescopes being able to “see through” things that our eyes cannot see through. Building on this idea, you can also foreshadow later discussions of nonvisible light by pointing out that while no telescope can help the problem in v ...
the outer planets: gas giants
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... times denser than the Gas Giants. All planets become denser toward their middle because the weight of material packs everything tighter. After Mars, there is a huge gap of space before the next four planets are met. They are the Gas Giants, spheres of gas and swirling atmospheres. There is no clear ...
Igneous, metamorphic and sedimentary rocks.
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... First order classification: based on average crystal size (termed texture). ...
AnnexA_26apr05
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Science in the news – Voyager`s 11 billion mile
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... Science in the news – Voyager’s 11 billion mile journey Much of what we know about the outer planets and their moons is as a result of the Voyager missions since the data would have been impossible to collect from Earth. Now Voyager is beginning to leave our solar system and it is sending back data ...
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Did Saturn`s rings form during the Late Heavy Bombardment?
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... (Gomes et al., 2005), but also the orbital architecture of the giant planet system: orbital separations, eccentricities, inclinations (Tsiganis et al., 2005), the capture of the Trojan populations of Jupiter (Morbidelli et al., 2005) and Neptune (Tsiganis et al., 2005; Sheppard and Trujillo, 2006), ...
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Our Solar System - Barbara Kehr`s Web Site
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Kuiper: A Discovery-class Observatory for Giant Planets, Satellites
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... to  determine  if  the  Jupiter  Trojans  originated   in  the  Kuiper  Belt  and  were  scanered  (“Nice-­‐ like”)  or  if  they  originated  near  Jupiter  or   closer  to  the  Sun  (consistent  with  smooth   migraQon) Jim Bell / OPAG 20 ...
Age aspects of habitability - Cambridge University Press
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... photosynthetic organisms. Photosynthesis is currently the only geologically documented biogenic process (see, e.g., Lyons & Reinhard, 2011; Fomina & Biel 2014 and references therein) that can provide sufficient energy to modify the global planetary (or atmospheric) properties. The large free energy ...
No Slide Title
No Slide Title

... • The radiation disrupts water molecules and releases their oxygen and hydrogen • This could account for 2% of present-day oxygen • but with 2% oxygen, ozone forms, creating a barrier ...
The Anglo-Australian Planet Search – XXI. A Gas-Giant
The Anglo-Australian Planet Search – XXI. A Gas-Giant

... planets with periods of near one year are themselves of great intrinsic interest, because (as was realised by most researchers soon after the first gas-giant planets were discovered within 1 AU – see e.g. Williams et al. 1997) they are likely to host their own satellite systems, which could well be ...
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... have a hidden salty sea. Callisto was previously thought to be a solid sphere of rock and ice. A liquid ocean on Callisto, however, seems to be the only explanation for data sent back by the Galileo spacecraft while in orbit around Jupiter. Observations by Galileo have confirmed that neither Europa ...
Clues to Earth`s Past
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... The radioactive isotopes of different elements decay to form daughter isotopes at different rates. But the rate of decay is constant for a given isotope. This rate of decay is measured in time units called half-lives. An isotope’s half-life is the time required for half of the parent isotopes to dec ...
Giant Planets at Small Orbital Distances
Giant Planets at Small Orbital Distances

... The equations of state for H2O and olivine (as representative of rock) were taken from the ANEOS compilation (Thompson 1990). The large mean molecular weight of giant rocky planets ensures that thermal e ects are small in most of the interior (Hubbard 1984), so that an olivine or ice planet in close ...
Vegetarian: Greco-Roman Warrior Cycle
Vegetarian: Greco-Roman Warrior Cycle

... sixth and final orbital cycle, collecting more gravity data and conducting radar and radio science experiments. By the end of the mission, Magellan will have captured high-resolution gravity data for an estimated 95 percent of the planet's surface. In September 1994, Magellan's orbit was lowered onc ...
Standard Four: Earth in Space
Standard Four: Earth in Space

... to always be illuminated by the Sun (day) and one half to not be illuminated by the Sun (night). Apply this model of the rotating Earth to explain why the Sun appears to move across the sky each day from east to west. Using newspapers, the internet, and actual sky observations when possible, charts ...
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Late Heavy Bombardment



The Late Heavy Bombardment (abbreviated LHB and also known as the lunar cataclysm) is a hypothetical event thought to have occurred approximately 4.1 to 3.8 billion years (Ga) ago, corresponding to the Neohadean and Eoarchean eras on Earth. During this interval, a disproportionately large number of asteroids apparently collided with the early terrestrial planets in the inner Solar System, including Mercury, Venus, Earth, and Mars. The LHB happened after the Earth and other rocky planets had formed and accreted most of their mass, but still quite early in Earth's history.Evidence for the LHB derives from lunar samples brought back by the Apollo astronauts. Isotopic dating of Moon rocks implies that most impact melts occurred in a rather narrow interval of time. Several hypotheses are now offered to explain the apparent spike in the flux of impactors (i.e. asteroids and comets) in the inner Solar System, but no consensus yet exists. The Nice model is popular among planetary scientists; it postulates that the gas giant planets underwent orbital migration and scattered objects in the asteroid and/or Kuiper belts into eccentric orbits, and thereby into the path of the terrestrial planets. Other researchers argue that the lunar sample data do not require a cataclysmic cratering event near 3.9 Ga, and that the apparent clustering of impact melt ages near this time is an artifact of sampling materials retrieved from a single large impact basin. They also note that the rate of impact cratering could be significantly different between the outer and inner zones of the Solar System.
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