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Spring
Spring

... At the equinoxes, the tilt of Earth relative to the Sun is zero, which means that Earth’s axis neither points toward nor away from the Sun. (However, the tilt of Earth relative to its plane of orbit, called the ecliptic plane, is always about 23.5 degrees.) Vernal Equinox Questions and Answers Quest ...
Formation of the Sun and the Planets
Formation of the Sun and the Planets

... 3. Asteroids and Comets a) These are the most numerous objects in the solar system. b) Asteroids are small, rocky bodies and are located mainly in the asteroid belt between the orbits of Mars and Jupiter. c) Asteroids orbit the sun in the same direction as the planets. d) Asteroid orbits lie close ...
The Earth-Moon system
The Earth-Moon system

... Problem: Low Fe of Moon, more likely to be captured on wide orbit (and requires third body to take energy away), no heating of Moon ...
Objective 3 - Shiner ISD
Objective 3 - Shiner ISD

... Seasons  –  caused  by  tilt  of  the  axis One  hemisphere  is  Tilted  away  from  the  Sun  and  receives  less  direct  solar   rays  from  the  Sun.  The  area  around  the  Equator  isn’t  affected  by  Earth’s  Tilt.   Because  it’s  in  the  middle,  it  will  always  have  direct  solar  ra ...
Wasp-17b: An Ultra-Low Density Planet in a Probable Retrograde
Wasp-17b: An Ultra-Low Density Planet in a Probable Retrograde

... http://www.isdc.unige.ch/result.cgi?061127 novaX ...
Lecture03
Lecture03

... In the movie below, you will see the Sun, Mercury, Venus, Earth, Mars, Jupiter, and Saturn looking down on the plane of the solar system from the Earth’s perspective ...
Lecture 1 - Department of Physics and Astronomy
Lecture 1 - Department of Physics and Astronomy

... The speed of light is a universal constant, it does not change over time or from place to place. Thought Experiment: imagine two teams of scientist measuring the speed of a beam of light. One team measures the speed from a ground. The second team measures the speed from a fast moving airplane foll ...
Lecture4
Lecture4

... rotate a little bit more than one full turn to get the sun back up high: stars rise and set a bit ...
Lecture090402
Lecture090402

... They must line up in all 3 dimensions + time If the Moon and Sun followed the same path around the Earth (the ecliptic), we would see an eclipse every month, but the Moon’s orbit is tilted 5o with respect to the ecliptic, so there are only two times a year when the paths overlap ...
Starry Dome: Astronomy in Art and the Imagination
Starry Dome: Astronomy in Art and the Imagination

... stars on the disk below. The example on view, however, is a nonfunctional forgery in the style of a renowned Persian astrolabist. Instead of accurate pointers, this astrolabe uses stylized flourishes that do not line up realistically with the stars below. ...
the K-12 Teacher Resource Packet for
the K-12 Teacher Resource Packet for

... stars on the disk below. The example on view, however, is a nonfunctional forgery in the style of a renowned Persian astrolabist. Instead of accurate pointers, this astrolabe uses stylized flourishes that do not line up realistically with the stars below. ...
Lecture14: Solar System Debris
Lecture14: Solar System Debris

... •  Its radius and mass are not accurately known - it is so small even HST does not view it well. Pluto-Charon binary by HST: they are apart by only 0.9” ...
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... 3.32 MJ in 267 d orbit (a = 0.811 AU) with e = 0.23 (Fisher et al. 2003) ...
Chapter 3: the Sun
Chapter 3: the Sun

... • The combination of convection and rotation sets up strong zonal patterns: 5 in each hemisphere • Rising air from the deeper layers cools and forms clouds as it rises; we see deeper where the high ammonia clouds have been depleted by precipitation, much as on Earth rain will often mean clearer skie ...
Orbit - Geneva 304
Orbit - Geneva 304

...  Synodic month - the time it takes for the Moon to return to the same point on the celestial sphere with respect to the sun (>3600) ~29.5 days Rotation  The Moon has a rotational period of 27.3 days (coincides with it's sidereal period) = tidal lock  Because of this the Moon always keeps the same ...
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Week #2: Mars!

... conjunction: planet is located exactly toward the Sun - not possible to observe planets at all! ...
Is the Sun a Star? - Classroom Websites
Is the Sun a Star? - Classroom Websites

... each planetary system has a central starjust as our own solar system has one star, sometimes called by its Roman name, Sol. In some systems there are two (or even more stars) at the center. • Another approach, appropriate for middle and high school levels, is to have students research the history of ...
MERCURY
MERCURY

... NEARBY OBJECTS ...
June 2013 Kepler Space Telescope Update
June 2013 Kepler Space Telescope Update

... race around the Sun far faster than Earth, with Mercury completing more than four revolutions around the Sun for each one that Earth makes. At the same The image shows the configuration of Mercury, Venus, and Jupiter in the western sky just after time, Jupiter is far sunset on May 26, 2013. Insets s ...
FL_HMH_G10 Selection Test FSA Style No Answer Key
FL_HMH_G10 Selection Test FSA Style No Answer Key

... is surprised that it took so long for astronomers to suggest 53 planets. does not approve of the idea of identifying 53 objects as planets. thinks there are probably many more than 53 planets. believes that astronomers should identify 53 planets. ...
Lecture Summary (11/22)
Lecture Summary (11/22)

... outward force cannot balance the inward force. Gravity causes collapse that heats the interior, and in a shell surrounding the helium core hydrogen fusion begins again. The outer layers of the Sun will expand at this time due to the great temperatures inside and the Sun will become a red giant. Red ...
Rotation Review questions with answers
Rotation Review questions with answers

... Rotation Review questions 1. Our sun is 2.3 x 104 light years from the center of our Milky Way galaxy and is moving roughly in a circle around that center at a speed of 250 km/s. How long does it take the Sun to make one revolution about the galactic center? B) How many revolutions has the Sun compl ...
QUANTUM GRAVITY IN THE SOLAR SYSTEM
QUANTUM GRAVITY IN THE SOLAR SYSTEM

... satisfactory defined theory whose object, in very crude terms, is to define a gravitational correspondent of quantum electrodynamics , so as to hopefully arrive at a unified formulation of the basic laws of universe . A variety of attempts in such direction are reported in literature , among which t ...
Black Holes, Part 3, Dark Energy
Black Holes, Part 3, Dark Energy

... has a thousand-times larger volume, for which its mass density should be a thousand times larger as well, because of the greater gas compression resulting from the greater amassed gravity. But this is not the case. The Sun is a thousand times too light in comparison with the gas-sphere of Jupiter. T ...
Round 1
Round 1

... This is responsible for the presence of the asteroid belt (instead of a ninth planet). (tidal forces due to Jupiter) ...
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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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