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Distribution of Elements in the Earth`s Crust
Distribution of Elements in the Earth`s Crust

... their gravitational force. Over time, the largest planetesimals began to sweep up all of the matter in their regions of the solar system, becoming planets. This is how the Earth and the planets formed from the expansion of the solar nebula. The formation of Earth and our solar system was affected by ...
arXiv:0905.3008v1 [astro-ph.EP] 19 May 2009
arXiv:0905.3008v1 [astro-ph.EP] 19 May 2009

... unit recently reported by Krasinsky and Brumberg (2004), and suggested a possible explanation for this secular trend by means of the conservation law of total angular momentum. Assuming the existence of some tidal interactions that transfer the angular momentum from the Sun to the planets system, we ...
The Earth from Space
The Earth from Space

... A chilling vision of things to come… 2036 potential impact from Asteroid Apophis (d = 390m) April 13, 2029 enters lowearth space (beneath g.s. satellites). But not hit Earth However, the close encounter will influence its path. If it flies through a 600 m area it will hit the Earth in 2036. (1:5,50 ...
Astronomical distances and Stellar magnitudes
Astronomical distances and Stellar magnitudes

... 1. What is meant by a light year? 2. What is meant by an astronomical unit (AU)? 3. What is meant by a parsec (pc)? 4. What is meant by a mega parsec (Mpc)? 5. What is meant by the apparent magnitude of an astronomical object? 6. Give the approximate distance of the following in AU: (a) Sun to the E ...
The sun gets hotter as it gets closer to its centre Some facts about
The sun gets hotter as it gets closer to its centre Some facts about

... largest planet in our solar system. Neptune is covered in clouds and is blue because of Methane gas in its atmosphere. Fact 2: ...
File - SPACE YEAR 8
File - SPACE YEAR 8

... les as a result of natural processes and human use of resources. Through this substrand, students vie w Earth as part of a solar system, which is part of a galaxy, which is one of many in the universe and explore the immense scales associated with space. They explore how changes on Earth, such as da ...
Powerpoint file
Powerpoint file

... • A multi-planet system around a milli-second pulsar • Candidates around pulsating white dwarfs (GD 66) , one sdB star (V 391 Peg) and eclipsing WD systems (NN Ser & DP ...
Chapter 7
Chapter 7

... •All Jovian planets (and the Earth) have strong magnetic fields . They are caused by the rapid rotation and liquid conductive cores or mantles. •All the Jovian planets (and the Earth) emit low frequency radio emission. The emission is caused by the interaction of electrons with the magnetic field •T ...
Objects in the Universe
Objects in the Universe

... • Distance from the center of the planet • What equation can we use to determine the force due to gravity? • F = Mm r2 ...
Slide 1
Slide 1

Comments from John Saunders.
Comments from John Saunders.

... Church in Hoole. He returned at 3.15 pm and although he had missed the beginning of the transit, he made history. Racing against time he made drawings of the transit until 3.50 pm when the sun set. Aside from its rarity, the original scientific interest in observing a transit of Venus was that it co ...
Day-39
Day-39

... tails.  Ion tail created by the solar wind interacting with ions of the nucleus.  Dust tail created from solar wind and sunlight.  Comet tails point away from the Sun. ...
day of flier
day of flier

... Transit Facts Transits of Mercury only occur when the Sun, Mercury, and the Earth are precisely lined up. Since Mercury’s orbit is tilted slightly, ...
4-6 Script
4-6 Script

... Start with a (light) daytime view of the sky. If it is the wrong time of year to use the current view/time, change to a summer day. Explain that today you are going to talk about astronomy. Discuss the definition: from Greek words that mean "star law," astronomy is a science that studies things in t ...
Witnesses to Local Cosmic History - Max-Planck
Witnesses to Local Cosmic History - Max-Planck

... Research, discovered that the large planets with their immense gravity must have hurled the small bits and pieces to and fro in the solar system. But even the planets themselves did not remain completely unmoved. Depending on their constellation, they lost or gained energy in these processes and thu ...
PHYSICS 1500 - The University of Sydney
PHYSICS 1500 - The University of Sydney

... Question 5 The illustration at left shows an artist’s impression of a ‘hot Jupiter’ – a giant planet in a very close orbit around its parent star. The first such planet discovered was 51 Pegasi b which takes 4.23 days to orbit a sun-like star. The system is about 50 light years from Earth. The plane ...
THE SOLAR SYSTEM
THE SOLAR SYSTEM

... spinning at 1,600 kilometers (1,000 miles) per hour or feel it traveling around the Sun at a rate of 108,000 kilometers (67,000 miles) per hour! Q: Do all the planets rotate and revolve at the same speed? A: No. Each planet rotates on its axis at a different speed and revolves around the Sun at a di ...
Earth Moon Sun Jeopardy (1)
Earth Moon Sun Jeopardy (1)

... What can you tell us about the season and the solar energy received by the northern hemisphere when it is tilted away from the Sun? ...
Extraterrestrial Life
Extraterrestrial Life

... • Earth formed about 4.5 billion years ago • Earth has a large Moon, which has effects on tides, axis and rotation of the Earth. • Earth has a core of iron and other heavy elements and a mantle of silicates. • Early Earth had a high temperature and an atmosphere produced by outgassing with N2 and CO ...
Earth Moon Sun Jeopardy
Earth Moon Sun Jeopardy

TCI_Paper2_ConditionsForLife
TCI_Paper2_ConditionsForLife

... during its formation, developing into a gas giant similar to Jupiter or Uranus. On the other hand, Mars, at about a tenth the mass of Earth, can barely hold onto any atmosphere at all. However, the range of planetary masses suitable for life may be far narrower than this. Terrestrial planets less ma ...
File - IGS Intro Materials
File - IGS Intro Materials

... Section 1 • Planet Motion Section 2: The Inner Planets Section 3: The Outer Planets Section 4: Life in the Solar System ...
Seasons:
Seasons:

... Since antiquity, astronomers have observed all of the visible planets (Mercury, Venus, Mars, Jupiter, and Saturn) undertake similar motions. This motion has been problematic for incorrectly explained for 1000’s of years. ...
Ancient Astronomy
Ancient Astronomy

... • ~190-125 B.C. • Often called “greatest astronomer of antiquity.” • Contributions to astronomy – improved on Aristarchus’ method for calculating the distances to the Sun and Moon, – improved determination of the length of the year, – extensive observations and theories of motions of the Sun and Moo ...
The tenth planet by Francis Reddy November 2005
The tenth planet by Francis Reddy November 2005

... in the solar system and the fourth brightest Kuiper Belt object. It is also our solar system’s tenth planet. Since beginning a 5-year, all-sky survey with Palomar Observatory’s 48-inch Samuel Oschin Telescope in 2001, Brown and his colleagues Chad Trujillo at the Gemini Observatory on Mauna Kea, Haw ...
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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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