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History of Astronomy
History of Astronomy

... exponent, Euclid. These students pity also the man of to-morrow, who is not to be allowed to read, in the original Latin of the brilliant Kepler, how he was able--by observations taken from a moving platform, the earth, of the directions of a moving object, Mars--to deduce the exact shape of the pat ...
INTRODUCTION As in the last years, the Ephemerides of Minor
INTRODUCTION As in the last years, the Ephemerides of Minor

... As in the last years, the Ephemerides of Minor Planets for 2017 are prepared by the IAA RAS only in the electronic form. Distribution of the EMP-2017 is accomplished via Internet or through sending compact disks (CD) by mail. As compared with period before 2012, the substantial changes are introduce ...
Outer Solar System Exploration - Lunar and Planetary Institute
Outer Solar System Exploration - Lunar and Planetary Institute

... seen the concepts submitted in response to the 2014 RFI for $1B Europa mission concepts, thus cannot assess if these meet a majority of the V&V goals.) • OPAG finding: OPAG commends NASA for the significant progress that has been made on Europa exploration opportunities, especially releasing the PEA ...
Grade 5 CPSD Science Curriculum Guide
Grade 5 CPSD Science Curriculum Guide

... ESS1.B: Earth and the Solar System The orbits of Earth around the sun and of the moon around Earth, together with the rotation of Earth about an axis between its North and South poles, cause observable patterns. These include day and night; daily changes in the length and direction of shadows; and d ...
September 2016
September 2016

... As the Moon continues on its orbit around Earth, the dark half of the Moon begins to appear and the sunlit side begins to move out of view. This is called the ‘Waning Gibbous’ phase. After about 20 days, only the left half of the Moon appears illuminated which is called the ‘Last Quarter’. The final ...
PDF format
PDF format

... a)  rotation of Earth; motion of the Sun around the center of the Milky Way; motion of Earth around the Sun b)  motion of the Sun around the center of the Milky Way; motion of Earth around the Sun; rotation of Earth c)  motion of Earth around the Sun; rotation of Earth; motion of the Sun around the ...
SIM-Lite Space Astrometric Observatory
SIM-Lite Space Astrometric Observatory

... 48 Planetary systems 95 planets & ~300 Asteroids 48 detectable planets (<5yr, SNR>5.8) Threshold 1Me @ 1AU Two key metrics Confidence of detection Completeness ...
Is the Sun anomalous?
Is the Sun anomalous?

... the Sun is likely to be among the top ~9% of stars by mass in the solar neighborhood. Among the categories of solar anomalies listed in the previous section, perhaps the weakest case is the low photometric variability of the Sun. The number of nearby Sun-like stars with long-term high-precision phot ...
Chapter 2: The Solar System and Beyond
Chapter 2: The Solar System and Beyond

... Seasons Who doesn’t love summer? The long, warm days are great for swimming, biking, and relaxing. Why can’t summer last all year? Blame it on Earth’s axis and revolution around the Sun. The axis is not straight up and down like a skyscraper—it is slightly tilted. It’s because of this tilt and Earth ...
History of Saturn Discovery
History of Saturn Discovery

... rings were not solid but individual particles. ...
SOLAR ECLIPSES
SOLAR ECLIPSES

... The motion of nodes’ line on the ecliptic, together with moon phases’ periodicity (known as sinodic period or ”lunation“ = 29.53 days), generates a period of 18 years and 10.32, 11.32 or 12.32 days (depending on how many leap years are included in a 18-year period), for eclipses creation in the same ...
Exploring Solar Systems Across the Universe
Exploring Solar Systems Across the Universe

... fusion of the light elements into heavier ones began to occur. Fusion released great amounts of energy over millions of years. Eventually, some stars exploded, producing clouds of ...
Document
Document

Adventures in the Attic Educator Guide
Adventures in the Attic Educator Guide

... touch the star. As the Earth orbits around the Sun, its axis is continually tilted in this direction. This is why, to people living on Earth, Polaris appears to remain in the same place while all the stars rotate around it. The Earth rotates about its axis once each day. It takes one year for the Ea ...
The Moon
The Moon

... moves with respect to Sun as well. • Times of moonrise and moonset grow later throughout the month; an hour later each day. ...
Fulltext
Fulltext

... cloud around the newly formed planets. Some moons can be captured bodies that were created somewhere else in the system. After that, the newly created planetary system evolves gravitationally, resulting in a complicated pattern of orbital changes of planets, which results in a set of orbits that are ...
Scientific Revolution - W W W . M R S O B R Y A N . W E E B L Y
Scientific Revolution - W W W . M R S O B R Y A N . W E E B L Y

... • After Brahe’s death, his assistant, the German astronomer and mathematician Johannes Kepler, used Brahe’s data to calculate the orbits of the planets revolving around the sun. • Kepler’s calculations supported Copernicus’ heliocentric theory. • His calculations also showed that the planets moved i ...
The Natural Clock
The Natural Clock

... Here is a short list of natural clocks: The rate the sun is shrinking; The rate the earth’s rotation is slowing down; The rate of decay in the Earth’s magnetic field; The rate of the Earth’s sediment (river and ocean sediments (silt, sand)) deposits; The rate of the Moon’s dust deposits; The rate of ...
Dec - National Capital Astronomers
Dec - National Capital Astronomers

... Planetary Destinations On November 28th, an update on the search for extraterrestrial life was released. It was in regard to K2-3d, an extrasolar planet, which was actually discovered in 2015 by the Kepler Spacecraft (NASA) as part of the K2 Mission (Kepler’s “Second Light”). K2-3d is 1.5 times Eart ...
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1 Introduction

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L21-OuterPlanets+Titan
L21-OuterPlanets+Titan

... Titan, Saturn’s largest moon, has an atmosphere10 times thicker than Earth’s. This atmosphere is mainly of N2 and contains a lot of organic material. Titan sports a methane cycle, with clouds, rain & seas. Methane is the source of organic material in Titan’s atmosphere and on its surface. It’s not e ...
The Discovery of Planet X
The Discovery of Planet X

... with a 1:2 resonance are also called twotinos, and objects with a 2:3 resonance are called plutinos, after their most prominent member, Pluto. Classical Kuiper belt objects (also called cubewanos) have no such resonance, moving on almost circular orbits, unperturbed by Neptune. Examples are Quaoar a ...
Convocatory Topics 7th Grade TOPICS
Convocatory Topics 7th Grade TOPICS

... Temperature and Size: Analyze the way in which astronomers use color to determine the surface temperature of stars. Compare the size of the sun to the size of other stars. Describe the sun’s composition and structure (including the layers of the sun). Explain how the sun produces energy. Define nucl ...
Atmosphere of Earth &amp; Venus Test 1 • Test1 • Processes that shape
Atmosphere of Earth & Venus Test 1 • Test1 • Processes that shape

... Ideas are important; answers are not. Do not memorize the answers. Models are important; answers are not. Do not memorize the answers. Do not memorize questions: For some questions, the ideas are the same as on homework or practice test, but the wording is different. ...
PDF only - at www.arxiv.org.
PDF only - at www.arxiv.org.

... characterization of planet atmospheres and surfaces based on spectroscopy and photometric variability. If other detection techniques have not already identified suitable planets, then direct detection campaigns would first need to devote considerable observation time to searching for such planets. M ...
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Orrery



An orrery is a mechanical model of the solar system that illustrates or predicts the relative positions and motions of the planets and moons, usually according to the heliocentric model. It may also represent the relative sizes of these bodies; but since accurate scaling is often not practical due to the actual large ratio differences, a subdued approximation may be used instead. Though the Greeks had working planetaria, the first orrery that was a planetarium of the modern era was produced in 1704, and one was presented to Charles Boyle, 4th Earl of Orrery — whence came the name. They are typically driven by a clockwork mechanism with a globe representing the Sun at the centre, and with a planet at the end of each of the arms.
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