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EXPLORATION OF THE KUIPER BELT BY HIGH
EXPLORATION OF THE KUIPER BELT BY HIGH

... them to diffraction profiles of interplanetary objects. The synthetic profiles depend on two parameters: the object’s radius and its distance from the Sun. The synthetic profile is computed assuming a circular orbit and zero-impact parameter. The parameters of the synthetic profiles given in Table 2 ...
Astro110-01 Lecture 7 The Copernican Revolution
Astro110-01 Lecture 7 The Copernican Revolution

... Earth, the size and distance to our Moon, the size and distance to our Sun • He even deduced that the points of light we see at night are not dots painted on some celestial sphere but stars like our Sun at enormous distances. • Aristarchus' discoveries remained truly unbelievable to the people of hi ...
The Cosmic Perspective Other Planetary Systems: The New Science
The Cosmic Perspective Other Planetary Systems: The New Science

... •  GAIA is a European mission planned for 2013 that will use interferometry to measure precise motions of a billion stars © 2014 Pearson Education, Inc. ...
No Slide Title
No Slide Title

... • If the star has planets, the magnification pattern experienced by a background source is no longer circularly symmetric on the sky • The combined gravitational field of the star and planet can create strong deviations in the lensing pattern, called caustics – This means that the changes in the lig ...
A Planetary Overview
A Planetary Overview

... neighborhood around its orbit”. The process of “clearing” is a continuous one and is related to how much an object dominates the dynamics of other objects in its neighborhood. The wording might need to be fixed still, but the concept is clear. The arguments have given us another example of how scien ...
Chapter 13 Other Planetary Systems: The New Science of Distant
Chapter 13 Other Planetary Systems: The New Science of Distant

... • A transit is when a planet crosses in front of a star. • The resulting eclipse reduces the star’s apparent brightness and tells us planet’s radius. • No orbital tilt: accurate measurement of planet mass © 2010 Pearson Education, Inc. ...
PDF format
PDF format

... Thought Question Suppose you found a star with the same mass as the Sun moving back and forth with a period of 16 months. What could you conclude? A.  B.  C.  D.  ...
Apr 2016 - Bays Mountain Park
Apr 2016 - Bays Mountain Park

... public telescope viewing every clear Friday evening at the Broemmelsiek Park Astronomy Site in St. Charles County, Missouri. The C-14 telescope that we had permanently mounted in the Park observatory was recently stolen. If you hear of anyone getting a pre-owned C-14, and have suspicions about the t ...
Climate Change
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... Closure: Planetary Temperatures 1. What determined the temperature of your planets? 2. Did your planets come to an equilibrium temperature? What is happening at that temperature? 3. If your sun got hotter, would the temperature change? How? 4. If your planet got farther away, would the temperature ...
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... were derived using observations made by Tycho Brahe ...
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Outline of Lecture on Copernican Revolution: 5b: So, what was

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Astronomy Lecture 1a

... ___ 67. ? was the first scientist to accurately determine the circumference of the Earth, differing from the true value by only about 15%. A.Ptolemy B.Copernicus C.Brahe D.Hipparchus E.Eratosthenes ___ 68. When one body exerts a force on a second body, the second body also exerts a force on the firs ...
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... Pluto was closest to the Sun in 1989 and moved farther away from the Sun than Neptune in 1999. So Pluto is still relatively near its closest approach to the Sun out of its 248-year period, and it appears about as bright as it ever does to viewers on Earth. ...
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Outline of Lecture on Copernican Revolution: 1. Source of word

... god, who should more properly have better things to be attending to. Ptolemy’s epicycles derived the back and forth motion of the planets from circles turning on circles. • This motion might seem possible for a god to set going and then have it run on forever, since uniform circular motion seemed li ...
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... worlds. Most are relatively nearby, within 5,000 light years, although one candidate was discovered in September 2005 via "microlensing" at a distance of 17,000 light years. Our whole solar system, along with all the local stars you can see on a clear dark night, reside in one of our galaxy's spiral ...
Volume 2 - Euresis Journal
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... group led by Mayor, and the California group led by Marcy and Butler. The first planets discovered were, naturally, those that are easiest to find – massive objects like Jupiter. However, the big surprise was that these planets were orbiting their stars at tiny separations, smaller than Mercury’s or ...
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... calculate its diameter without uncertainties, the images taken by LORRI have confirmed the previous estimated value of 1,208 km. On 13 July, the picture shot from a distance of 768,000 km will be probably considered the iconic image of the entire mission, a spectacular overview ...
Designing Curriculum and Instruction in Elementary School
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... 100 miles across. A few, like Ida, even have their own moons. Further out, beyond the orbit of the minor planet Pluto, sits another belt known as the Kuiper Belt. Like the Asteroid Belt, the Kuiper Belt is also made up of thousands, possibly even millions of objects too small to be considered planet ...
Million years - The Origin Of Life
Million years - The Origin Of Life

... almost zero? Such a massive collision should have affected its eccentricity but there is no evidence for any massive impact. Earth The Earth is tidally locking to the Moon. 1 This is actually hastening the Sun’s tidal locking influence on the Earth. With both working together the tidal locking time ...
Solar System Formation
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... buildup of terrestrial planets took ~ 100 Myr slow accumulation of small bodies not much mass involved buildup of giant planets took ~ 10 Myr (need to have gas around) all giant planets have roughly the same heavy element mass… 5, 15, 300, 300 X solar heavy/light element ratios in J/S/U/N H and He t ...
Measuring the ligth
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... When instead of a punctual body we observe an extended one, like for instance a near comet, we can distinguish and specify the incoming light from different areas of the object, we define then, the intensity, <>, as the radiated energy per second by a region of the object that we can see under a ...
benchmarks and task analyses - I
benchmarks and task analyses - I

... 4. Divide students into groups to research the planets. Each group would be responsible for creating two pages for a class book about planets. This book can stay in the classroom or be shared with others. ASSESSMENT 1. Complete observational assessments as student groups are working together- note i ...
Search for Other Worlds - Science fiction 20 years
Search for Other Worlds - Science fiction 20 years

... each other in their orbits, the system is called an eclipsing binary star system. If a planet has a large orbit that carries it around both members of an eclipsing double star system, then the planet can be detected through small variations in the timing of the stars' eclipses of each other. CM Drac ...
The Solar System
The Solar System

... Venus is sometimes called Earth’s twin because its size and mass are similar to Earth’s. In 1962, Mariner 2 flew past Venus and sent back information about Venus’s atmosphere and rotation. The former Soviet Union landed the first probe on the surface of Venus in 1970. Venera 7, however, stopped work ...
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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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