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Events: - Temecula Valley Astronomers
Events: - Temecula Valley Astronomers

... We still have to answer the question of Pluto’s status. Is Pluto a planet or not? In the early 2000s Caltech’s Mike Brown discovered small objects in the outer reaches of the Solar System, well beyond Neptune’s orbit. One of these objects turned out to be about the size of Pluto. The new object was ...
PowerPoint Presentation - A Tour of the Solar System
PowerPoint Presentation - A Tour of the Solar System

... Asteroids are either rocky or metallic objects that orbit the Sun. They are too small to considered planets but are sometimes called planetoids. ...
Ch. 13
Ch. 13

... Miranda, Ariel, Umbriel, Titania, and Oberon Very similar to Saturn’s medium-sized moons, except that all are much less reflective. Umbriel is the darkest: ...
Goal: To understand what the Kuiper Belt is, and why it is
Goal: To understand what the Kuiper Belt is, and why it is

... Classical Region Ranges from 42-47 AUs. Quaoar and Varuna are the most famous objects from this region. ...
Outer Solar System Exploration - Lunar and Planetary Institute
Outer Solar System Exploration - Lunar and Planetary Institute

... • Europa remains the highest priority mission destination for the outer planets community. The next Europa mission should address a majority of the goals for Europa science outlined in Vision and Voyages (V&V). We continue to strongly support the Europa Clipper as a scientifically compelling, techno ...
Pluto naomi
Pluto naomi

... rock with the remainder being water and other ices much like Neptune’s moon Triton. • Pluto's composition is not very well known since it is so far away from Earth. Astronomers believe that it's mostly made of rock and frozen methane, water, nitrogen and carbon dioxide. This is probably covered by a ...
júpiter, king of the moon
júpiter, king of the moon

... eruptions over the past million years are the cause of the satellite is found permanently covered by a 10 meter thick layer of sulphurous lava. The temperature of Io's surface is about -148 C, but there are many "hot spots" on Io's surface that reach up to +25 C. Europa is the second nearest of the ...
Sky Diary - Society for Popular Astronomy
Sky Diary - Society for Popular Astronomy

... Which brings us to the outer ice giant planets of Uranus and Neptune: Neptune reaches opposition, due south at midnight UT, on 2 September and Uranus reaches opposition on 15 October. This means that both planets are visible during nearly all of the available darkness on any night in the period, wit ...
April - Magic Valley Astronomical Society
April - Magic Valley Astronomical Society

... 8th. Mercury reaches greatest eastern elongation on April 18th, when it will shine at magnitude 0 and attain a sunset altitude of 19 degrees at latitude 40 degrees north. Mercury is illuminated approximately 38% and subtends approximately 7.5 arc seconds on that date. It is still 10 degrees above th ...
solar system-where are we? - Iowa State University Extension and
solar system-where are we? - Iowa State University Extension and

... know how long a full rotation of the moon around the earth usually takes? What do they call it when you have 2 full moons in a month? Ask, " What direction does the moon rotate around the Earth?" Answer: Counterclockwise. What did the ball/moon look like when it was a new moon?" Answer: all black. D ...
CHAPTER 20
CHAPTER 20

... Because of its thin atmosphere and its great distance from the sun, Mars is a cold planet. Mid-summer temperatures recorded by the Pathfinder-lander ranged from -130 C to -770 C. The atmosphere of Mars is so thin that the air pressure at the planet’s surface is roughly equal to the pressure 30 km ab ...
CHAPTER 20
CHAPTER 20

... Because of its thin atmosphere and its great distance from the sun, Mars is a cold planet. Mid-summer temperatures recorded by the Pathfinder-lander ranged from -130 C to -770 C. The atmosphere of Mars is so thin that the air pressure at the planet’s surface is roughly equal to the pressure 30 km ab ...
Skymobile: Comet Demonstration
Skymobile: Comet Demonstration

... This is a great list everybody! Now before we go any further we have to talk about the states of matter. (Take out the three plastic cups and line them up in a row and take out a bottle of water.) Now this may seem tricky at first, but I know you’ll understand what I’m talking about when we’re throu ...
Dwarf Planets
Dwarf Planets

... has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a (near-spherical) shape has not cleared the neighborhood around its orbit is not a satellite The term "dwarf planet" applies only to objects in the Solar System and is distinct from "planet" and "small solar s ...
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... Mercury (always low in twilight) or Venus (usually low), but on this occasion we catch Venus at its greatest apparent distance from the Sun and near peak altitude of a very favorable apparition high in the eastern morning sky. Not until November 2039 will we witness another compact trio of planets s ...
For Space: Our Solar System and Beyond The Solar System Planets
For Space: Our Solar System and Beyond The Solar System Planets

... The inner planets of Mercury, Venus, Earth, and Mars are small and mostly solid. The outer planets of Jupiter, Saturn, Uranus, and Neptune are large and made mostly of gases. Between the inner and outer planets is a belt of rocks called asteroids that orbit the sun. Lying beyond the gas giants, the ...
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Lecture 23: Jupiter Solar System Jupiter`s Orbit

... Atmosphere of Jupiter •Jupiter’s atmosphere shows very complex patterns of motion •There are bands, clouds, and storms •The bands display shear flow •The Great Red Spot is a storm a few times the size of Earth that has lasted for hundreds of years •The complex motions are explained by the combinatio ...
Abrams Planetarium Galileo & the Telescope—Sept 12 • Sky preview 2008-2009
Abrams Planetarium Galileo & the Telescope—Sept 12 • Sky preview 2008-2009

... the moon, the four moons of Jupiter, the phases of Venus, and the mysterious disappearance of Saturn’s rings. Long-time skywatcher, Bob Victor, author of the planetarium’s Sky Calendar, comes out of retirement to give the presentations. ...
Saturn - Kansas City Public Schools
Saturn - Kansas City Public Schools

... Each races around Saturn at speeds of up to 50,000 miles per hour. Such a setting of great beauty, enormity and complexity naturally begs the question: How did these rings form in the first place? Observations from Cassini indicate that the rings may have been created when a moon was shattered by an ...
Programme 16
Programme 16

... runs allocated to our group at the telescopes of ESO (NTT telescope) and TNG . This important observational campaign has produced until now one of the largest spectrophotometric data base of NEOs for the large spectral range covered (0.40-2.5 micron) and the number of observed objects (about 100 spe ...
1 The Solar System - e
1 The Solar System - e

... Have you carefully observed the sun, moon and the other celestial bodies in the sky? There is evidence that man had shown an interest in knowing about them since ancient times. At present man can explore more than what is visible to the naked eye, as scientists have invented modern equipment to obs ...
Celestia Activity 2013
Celestia Activity 2013

... observe the many orbiting moons. You can even fly around Jupiter a bit and try to find the Great Red Spot. Please research and answer the following: ...
Origin of the orbital architecture of the planets of the Solar System
Origin of the orbital architecture of the planets of the Solar System

... Once Jupiter and Saturn are blocked in their 3:2 resonance, Uranus and Neptune, which migrate by type I migration, have to be trapped in resonances with Saturn and with each other (Morbidelli et al., 2007) ...
CONTENTS OF THE SOLAR SYSTEM DATABASE
CONTENTS OF THE SOLAR SYSTEM DATABASE

... Even though Venus’ orbit brings it closer to Earth than any other planet, its blanket of clouds kept much of Venus a mystery. But space probes sent by the Soviet Union and the United States, as well as studies with ground-based radar, have allowed astronomers to “see” the surface of Venus for the f ...
solar system - Math/Science Nucleus
solar system - Math/Science Nucleus

... to see things never observed before. Kepler developed mathematical models to explain motion, which helped to allow humans to predict what is going on. Galileo's inquiry on motion would be used by Sir Isaac Newton to uncover more mysteries of the Universe. Newton's law of motion would take astronomy ...
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Naming of moons

The naming of moons has been the responsibility of the International Astronomical Union's committee for Planetary System Nomenclature since 1973. That committee is known today as the Working Group for Planetary System Nomenclature (WGPSN).Prior to its formation, the names of satellites have had varying histories. The choice of names is often determined by a satellite's discoverer; however, historically some satellites were not given names for many years after their discovery; for instance, Titan was discovered by Huygens in 1655, but was not named until 1847, almost two centuries later.Before the IAU assumed responsibility for astronomical nomenclature, only twenty-five satellites had been given names that were in wide use and are still used. Since then, names have been given to 129 additional satellites: 45 satellites of Jupiter, 43 of Saturn, 22 of Uranus, 11 of Neptune, 5 of Pluto, 1 of Eris, and 2 of Haumea. The number will continue to rise as current satellite discoveries are documented and new satellites are discovered.At the IAU General Assembly in July 2004, the WGPSN suggested it may become advisable to not name small satellites, as CCD technology makes it possible to discover satellites as small as 1 km in diameter. To date, however, names have been applied to all moons discovered, regardless of size.
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