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december 2010 - Holt Planetarium
december 2010 - Holt Planetarium

... Season’s greetings to one and all. There are a couple of interesting astronomical events this month. On December 21 there is a total eclipse of the Moon. The total phase of this eclipse lasts for just over 72 minutes, with the partial umbral eclipse spanning almost 3.5 hours. All stages of the total ...
Astronomical Beliefs - Communicating Astronomy With The Public
Astronomical Beliefs - Communicating Astronomy With The Public

... http://living.oneindia.in/insync/2008 But these are halos produced by refraction/reflection ...
History of Astronomy
History of Astronomy

... mechanical computer • ~ 100 BC, Greek ...
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HR.MOON.doc

... called Moon phases. New Moon means no Moon. When the right side of the Moon is lit up it is called first quarter. ...
Kepler - STScI
Kepler - STScI

... •Mass-Radius leads to degenerate solutions: •Mostly water with a small rocky core •A “failed” giant planet core? •Lower ice/rock ratio, with a H/He envelope •A mini Neptune? What is the cooling history and interior state of these two kinds of models? ...
Training Guide
Training Guide

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APOM 2014 April
APOM 2014 April

... This week's issue of Naturefeatures an interesting announcement by Chadwick Trujillo (Gemini Observatory) and Scott Sheppard (Carnegie Institution for Science). These two observers have found an object orbiting the Sun, designated 2012 VP113, that they first spotted 17 months ago with the 4-m Blanc ...
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... allowed extremely accurate predictions of planetary orbits.  Cavendish measured gravitational forces between human-scale objects before 1800. ...
sunmoon - University of Glasgow
sunmoon - University of Glasgow

... The two end stars are the ‘Pointers’, and point towards the Pole Star, (which is in the Little Bear). ...
Opposition of Jupiter - Hong Kong Observatory
Opposition of Jupiter - Hong Kong Observatory

... Opposition of Jupiter  Jupiter is the largest planet in the Solar System and the fifth planet away from the Sun. Jupiter is characterized by the brightly coloured bands on its surface and the Great Red Spot near the equator.  Jupiter revolves around the Sun with a period of about 11.86 years. In anc ...
early astronomical history
early astronomical history

... – Ptolemy of Alexandria improved the geocentric model by assuming each planet moved on a small circle, which in turn had its center move on a much larger circle centered on the Earth – The small circles were called epicycles and were incorporated so as to explain retrograde motion – Ptolemy’s model ...
Astronomy in Ancient Cultures
Astronomy in Ancient Cultures

... observe, without the aid of technology! (The Sun, Mercury, Venus, Mars, Jupiter, Saturn, Meteors, Comets, and Stars.) Astronomy is the oldest science. There is evidence of crude astronomy even in prehistoric times. Early astronomy was about observing the motion of these celestial objects. ...
Introduction to Astronomy
Introduction to Astronomy

... Lesson 6: Inside the Earth: Rocks and Minerals There are many different types of rock on our planet. These can be divided into three groups: metamorphic, igneous and sedimentary. The category a rock goes into is dependent on how it was formed. Igneous means ‘made by fire’ – for example, granite. So ...
Slide 1
Slide 1

... •When the moon has completed half its trip around the earth, the full moon is illuminated. •During the third and fourth quarters of the moon’s trip around the earth, the illuminated portion gradually decreases so only the left side is illuminated and finally no lit portion of the moon is visible fro ...
Slide 1 - leslie09
Slide 1 - leslie09

... the sun. Earth, our home planet, is the only planet in our solar system known to harbor life . Planet in our solar system known to harbor life . Scientists around the world have discovered many things about our planet by working together and sharing their findings. ...
Bringing Our Solar System to Life Grade 5 Overview Since the Solar
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... The classroom contains roughly 20 fifth graders. The genders in the classroom are about even. These students have had one prior lesson on the solar system and its planets which was presented in a lecture form, with pictures, by the teacher. The setting of the school is rural. 5.2.1 Recognize that ou ...
SKYTRACK Glossary of Terms
SKYTRACK Glossary of Terms

... Apogee – The point in the orbit of the Moon or other satellite where it is furthest from the Earth. Celestial body – Any object beyond the Earth and visible in the sky. Celestial Sphere – An imaginary sphere of immense radius around the Earth which serves as the abstract backdrop for celestial bodie ...
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... intersects with celestial equator ...
The Swansong of Stars Orbiting Massive Black Holes
The Swansong of Stars Orbiting Massive Black Holes

... The signal is expected to be weak. To detect it, it is necessary to know in advance the shape of the wave trains, and to do that, it is necessary to know the eccentricity of the inspiral orbits. High eccentricity can change the nature of the signal drastically. The eccentricity also determines how m ...
Chapter 2
Chapter 2

... •Not all of the planetesimals ended up becoming planets •Some were made up primarily of rocky and metallic substances, and they became asteroids •Most asteroids reside in a belt of rocky debris between Earth and Jupiter that may be left over from the early solar system •The total mass of all the as ...
View SKYTRACK_Glossary of Terms
View SKYTRACK_Glossary of Terms

... Apogee – The point in the orbit of the Moon or other satellite where it is furthest from the Earth. Celestial body – Any object beyond the Earth and visible in the sky. Celestial Sphere – An imaginary sphere of immense radius around the Earth which serves as the abstract backdrop for celestial bodie ...
Theme 7.2 -- The Complete Solar System
Theme 7.2 -- The Complete Solar System

... system over the passage of many millions of years. Small planets may even be ejected from the system entirely. So, the system as we see it now is not as it was at the time of formation: planets have drifted in their positions. Computer modelling now suggests that effects of this sort may have been i ...
ASTR 300 Stars and Stellar Systems Spring 2011
ASTR 300 Stars and Stellar Systems Spring 2011

... Since a star’s brightness varies as√ the inverse square of the distance, the distance would have to decrease by a factor of 15.85 = 3.981. (I.e., 3.9812 = 15.85.) Since Barnard’s star is now at 5.9 ly, we would have to move it to 5.9/3.981 = 1.48 ly. Barnard’s star is actually moving towards us at 1 ...
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Formation of the Solar System Chapter 8

... Outside the “Frost line”, there was more efficiently capture (by their bigger gravitational pull) of H/He gas before it was dispersed by the Sun’s radiation and solar wind ...
Explore the Planets
Explore the Planets

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Satellite system (astronomy)



A satellite system is a set of gravitationally bound objects in orbit around a planetary mass object or minor planet. Generally speaking, it is a set of natural satellites (moons), although such systems may also consist of bodies such as circumplanetary disks, ring systems, moonlets, minor-planet moons and artificial satellites any of which may themselves have satellite systems of their own. Some satellite systems have complex interactions with both their parent and other moons, including magnetic, tidal, atmospheric and orbital interactions such as orbital resonances and libration. Individually major satellite objects are designated in Roman numerals. Satellite systems are referred to either by the possessive adjectives of their primary (e.g. ""Jovian system""), or less commonly by the name of their primary (e.g. ""Jupiter system""). Where only one satellite is known, or it is a binary orbiting a common centre of gravity, it may be referred to using the hyphenated names of the primary and major satellite (e.g. the ""Earth-Moon system"").Many Solar System objects are known to possess satellite systems, though their origin is still unclear. Notable examples include the largest satellite system, the Jovian system, with 67 known moons (including the large Galilean moons) and the Saturnian System with 62 known moons (and the most visible ring system in the Solar System). Both satellite systems are large and diverse. In fact all of the giant planets of the Solar System possess large satellite systems as well as planetary rings, and it is inferred that this is a general pattern. Several objects farther from the Sun also have satellite systems consisting of multiple moons, including the complex Plutonian system where multiple objects orbit a common center of mass, as well as many asteroids and plutinos. Apart from the Earth-Moon system and Mars' system of two tiny natural satellites, the other terrestrial planets are generally not considered satellite systems, although some have been orbited by artificial satellites originating from Earth.Little is known of satellite systems beyond the Solar System, although it is inferred that natural satellites are common. J1407b is an example of an extrasolar satellite system. It is also theorised that Rogue planets ejected from their planetary system could retain a system of satellites.
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