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Goal: To understand life in our universe.
Goal: To understand life in our universe.

... • We examine the velocity of the star moving towards and away from us. • If an alien species were looking along the plane of our solar system they would be able to see our sun moving towards them at one point at a velocity of 0.13 km/s • This is a pretty small velocity, and tough to actually observe ...
Pluto
Pluto

... exhaustive series of photographs and to examine them for objects that were not stars. He exposed 14-by-17-inch plates by night, and by day, examined the images in an instrument called a blink comparator. By rapidly alternating a magnified view of two photographs of the same area of the sky taken at ...
25drake3s
25drake3s

... Due Friday Project should be neat, organized, labeled and have all questions fully answered Telescope objects:  Venus, Uranus, Neptune, Saturn, Moon ...
Powerpoint
Powerpoint

... that not all bodies orbit Earth – Observed phases of Venus (and correlation of apparent size and phase); evidence that Venus orbits the Sun ...
SCI 103
SCI 103

... 18) Kepler’s first two Laws of Planetary Motion contradicted the Aristotelian/Ptolemaic Model of the Universe in two fundamental ways. What are Kepler’s first two Laws of Planetary Motion and how were they anti-Aristotelian? Kepler’s 1ST law states that planets orbit, not on circles, but on ellipse ...
Big Bang
Big Bang

... the interstellar medium. These regions are called molecular clouds mainly composed of hydrogen plus helium • Main Sequence: Stars spend about 90% of their lifetime at this stage, fusing hydrogen to produce helium near the core (main sequence). • Fate of Stars: Massive stars process up to iron, and f ...
Identifying Patterns in the Solar System
Identifying Patterns in the Solar System

... objects too big or too far away to test and study in a lab. This is fortunate, because it turns out that sizes and distances in space are huge! Using this data, scientists analyze solar system objects like planets and moons to look for patterns or relationships. One very useful form of analysis is t ...
Geocentric System
Geocentric System

... The Moon is Falling! Newton’s insight: same force causes apple to fall and keeps Moon in orbit; decreases as square of distance, as does ...
8.1_Formation of the Universe
8.1_Formation of the Universe

... Our Galaxy- Milky Way ...
Lesson 4: Object`s Motion in the Sky
Lesson 4: Object`s Motion in the Sky

... already in motion, it will stay in motion at that same speed and direction unless an outside force acts on it. This is called Newton’s first law of motion. ...
Origin of Solar System Study Guide
Origin of Solar System Study Guide

... terrestrial planets). When astronomers see a rocky or icy surface with few craters, they know that the surface is new. For example, the moon and Mercury are very old surfaces – they are marked with craters – while Europa and the Earth show far fewer craters. Earth’s and Europa’s surfaces are, due to ...
PPTX - University of Colorado Boulder
PPTX - University of Colorado Boulder

... The sum of the distances from any point P on the ellipse to those two foci is constant and equal to the major diameter ( PF1 + PF2 = 2a ). ...
Unit 7 Planets Day 1!
Unit 7 Planets Day 1!

... I can classify the inner and outer planets by looking at their characteristics. ...
Ch. 26 The Sun and the Solar System
Ch. 26 The Sun and the Solar System

... History of solar System Study • Geocentric Models: Earth is the center of the Solar System. The stars were holes in a solid celestial sphere that surrounded the Earth. Beyond the sphere was a source of intense light. The belief was then that the sphere rotated with certain patterns coming around at ...
Solar System
Solar System

... • A coma is the fuzzy, gaseous component of a comet’s head. • A small glowing nucleus with a diameter of only a few kilometers can sometimes be detected within a coma. As comets approach the sun, some, but not all, develop a tail that extends for millions of kilometers. ...
Playground planets - Earth Learning Idea
Playground planets - Earth Learning Idea

... © Earthlearningidea team. The Earthlearningidea team seeks to produce a teaching idea regularly, at minimal cost, with minimal resources, for teacher educators and teachers of Earth science through school-level geography or science, with an online discussion around every idea in order to develop a g ...
Class 11 and 12 lecture slides (giant planets)
Class 11 and 12 lecture slides (giant planets)

... Hydrogen phase diagram Hydrogen undergoes a phase change at ~100 GPa to metallic hydrogen (conductive) It is also theorized that He may be insoluble in metallic H. Interior temperatures are adiabats ...
Composition Of The Solar System
Composition Of The Solar System

... a spiral galaxy like the Milky Way but is 4 times as massive and is 2 million light years away. The planets, most of the satellites of the planets and the asteroids revolve around the Sun in the same direction, in nearly circular orbits. When looking down from above the Sun's north pole, the planets ...
Planet Hunters
Planet Hunters

... of several hundred worlds, but astronomers have never given up the combined efforts of many hard-working scientists and brilliant young dream of seeing such worlds directly. Such observations would let planet hunters. Maybe they’ll even be answered by some of you! i us find new planets with a single ...
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... 16) Why were the first planets that were discovered around other stars much bigger than Earth and found very close to their stars? A) These planets produce a larger gravitational force on the star than an Earth-like planet far from the star B) These planets produce a smaller gravitational force on t ...
Movement around the sun - E
Movement around the sun - E

... time. Earth also rotates, or spins, on its axis. It takes one day to spin around itself one complete time. Earth’s axis is not straight up and down, but tilted at an angle of 23.5 degrees. The rotation is what causes the change from day to night. This tilt is responsible for having seasons. If Earth ...
The Gas Giant Planets
The Gas Giant Planets

... • The gas giants have many satellites as well as ring systems, and they are all very large. ...
Powerpoint
Powerpoint

... The size, shape, and orientation of cometary orbits depend on their location. Oort cloud comets rarely enter the inner solar system. ...
The Solar System
The Solar System

... • Unstable orbits; astronomers believe that they are refugees from the Kuiper Belt • Some may become comets ...
February 18
February 18

... • Tycho Brahe was the greatest naked eye observer of all time • He lived before the invention of the telescope • His observations of the alignment of Jupiter and Saturn occurred two days later than when predicted by Copernicus • Tycho came up with a model where the planets orbit the Sun but the Sun ...
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Planets beyond Neptune



Following the discovery of the planet Neptune in 1846, there was considerable speculation that another planet might exist beyond its orbit. The search began in the mid-19th century and culminated at the start of the 20th with Percival Lowell's quest for Planet X. Lowell proposed the Planet X hypothesis to explain apparent discrepancies in the orbits of the giant planets, particularly Uranus and Neptune, speculating that the gravity of a large unseen ninth planet could have perturbed Uranus enough to account for the irregularities.Clyde Tombaugh's discovery of Pluto in 1930 appeared to validate Lowell's hypothesis, and Pluto was officially named the ninth planet. In 1978, Pluto was conclusively determined to be too small for its gravity to affect the giant planets, resulting in a brief search for a tenth planet. The search was largely abandoned in the early 1990s, when a study of measurements made by the Voyager 2 spacecraft found that the irregularities observed in Uranus's orbit were due to a slight overestimation of Neptune's mass. After 1992, the discovery of numerous small icy objects with similar or even wider orbits than Pluto led to a debate over whether Pluto should remain a planet, or whether it and its neighbours should, like the asteroids, be given their own separate classification. Although a number of the larger members of this group were initially described as planets, in 2006 the International Astronomical Union reclassified Pluto and its largest neighbours as dwarf planets, leaving Neptune the farthest known planet in the Solar System.Today, the astronomical community widely agrees that Planet X, as originally envisioned, does not exist, but the concept of Planet X has been revived by a number of astronomers to explain other anomalies observed in the outer Solar System. In popular culture, and even among some astronomers, Planet X has become a stand-in term for any undiscovered planet in the outer Solar System, regardless of its relationship to Lowell's hypothesis. Other trans-Neptunian planets have also been suggested, based on different evidence. As of March 2014, observations with the WISE telescope have ruled out the possibility of a Saturn-sized object out to 10,000 AU, and a Jupiter-sized or larger object out to 26,000 AU.
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