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07_Jovian planets
07_Jovian planets

... The planet probably received this name because it moves so quickly across the sky. Venus is the Roman goddess of love and beauty. The planet is aptly named since it makes a beautiful sight in the sky, with only the Sun and the Moon being brighter. Earth is the only planet whose English name does not ...
Beyond Mnemonics: Pluto and the Nature of Science
Beyond Mnemonics: Pluto and the Nature of Science

... If your students were upset following the August 24th announcement from the International Astronomical Union that Pluto was demoted from its standing among the now eight major planets to a new category of “dwarf planet”, you are not alone. Students, many of whom were taught the order of the planets ...
Neptune is the eighth planet from the Sun and the fourth largest (by
Neptune is the eighth planet from the Sun and the fourth largest (by

... predicted by Adams and Le Verrier from calculations based on the observed positions of Jupiter, Saturn and Uranus. An international dispute arose between the English and French (though not, apparently between Adams and Le Verrier personally) over priority and the right to name the new planet; they a ...
Uranus project cd
Uranus project cd

... Uranus mass is more than 14 times larger than Earth. Uranus and Neptune are both known as Ice Giants. It takes 30,685 Earth days for Uranus to complete an orbit around the sun. Even though Neptune is further from the sun, Uranus is the coldest planet in the solar system. Uranus is the seventh planet ...
2 choices
2 choices

... a. It has a thin carbon dioxide atmosphere. b. It is cold, dry, and barren. c. Its winter temperatures may be 200 degrees below freezing. d. It has seasons. 17. The largest volcano in the Solar System is found on Mars. What is its name? a. Arsia Mons b. Elysium Mons ...
ppt
ppt

... Frozen ices and rocks. Pluto has a higher proportion of rocks than most moons of giant planets. ...
Zoom Astronomy is a comprehensive on
Zoom Astronomy is a comprehensive on

... Mercury's thin atmosphere consist of trace amounts of hydrogen and helium. The atmospheric pressure is only about 1 x 10-9 millibars; this is a tiny fraction (about 2 trillionths) of the atmospheric pressure on Earth. Since the atmosphere is so slight, the sky would appear pitch black (except for th ...
Chapter 13
Chapter 13

... • Uranus has 27 moons, five of which are major: Miranda, Ariel, Umbriel, Titania, and Oberon • Similar to Saturn’s medium-sized moons, except that all are much less reflective • Umbriel is the darkest ...
Sorting the Solar System - Indianapolis Public Schools
Sorting the Solar System - Indianapolis Public Schools

... our definitions in new ways, so that sometimes revisions need to be made. The discovery of Eris (early on referred to as the “tenth planet”) forced astronomers to give a fresh look at their definition of a planet and make revisions. As they discover ever more planets around other stars, some of them ...
Giant planet formation
Giant planet formation

... • prograte or retrograde, high eccentricity, high inclination orbits • outside the regular satellites system • usually quite small (non-spherical) Formed elsewhere, captured by the planet * The Hill sphere is the area (with radius RH) in which the gravity of a secondary body (m2) exceeds that of a p ...
minimum mass solar nebulæ and planetary migration
minimum mass solar nebulæ and planetary migration

... The Minimum Mass Solar Nebula (hereafter MMSN) is the protoplanetary disk of solar composition that has the amount of metals necessary to build the eight planets of the Solar System (and the asteroid belts). From the masses and compositions of the planets, a density of solids is derived at several l ...
Q in the Solar System
Q in the Solar System

... The asymmetrical position of lhe tidal bulges with respect to the line of centers, Mm, introduces a net torque between the planet and satellite. Because the satellite is attracted more strongly b y the near side bulge which is leading it in longitude, the torque acts to transfer angular momentum and ...
IMPACT CRATERING ON THE SMALL PLANETS CERES AND
IMPACT CRATERING ON THE SMALL PLANETS CERES AND

... are also visible along rimwalls. Boulders are common on the rims and floors of fresh complex craters, consistent with formation of abundant secondary craters in craters > ~50 km on Ceres and at a few craters on Vesta, and at ~1D from crater rims. The transition to complex craters begins ~10+/2.5 km ...
Beyond Neptune: The Kuiper Belt
Beyond Neptune: The Kuiper Belt

... few hundred AU, so maybe plants could form that far out. • Problems: very small sample of KBO’s. Sample size should get much better soon, so stay tuned. ...
Pictures in the Sky Teacher`s Guide
Pictures in the Sky Teacher`s Guide

... We examine numerous sky related objects and decide together when these things can be seen: during the day, the night, or both. Objects examined may include: clouds, the Sun, planets, rain, rainbow, lightning, kites, birds, stars, constellations, snow, bats, airplanes, and more. After examining all t ...
Pluto and definition of planet
Pluto and definition of planet

... of those forces is locking of orbital periods. While Neptune makes three orbits, Pluto makes just two. All these non typical attributes where cause for suspicion about his planetary status. Until early 90’s that suspicions where not argumented. There were not such large body like Pluto with similar ...
NEPTUNE*!
NEPTUNE*!

... They are composed of rock and ice. The first four moons of Neptune, Naiad, Thalassa, Despina, and Galatea, are so close to Neptune that they orbit within its ring system ...
Colburn Earth Science Museum - Asheville Museum of Science
Colburn Earth Science Museum - Asheville Museum of Science

... planets in our solar system, Pluto does not orbit along the same orbital plane. Tilted at 17 degrees, Pluto orbits on a more elliptical path than the 8 planets. Additionally, it crosses another planet’s orbit (Neptune), something no other planet does. For these afore mentioned reasons, Pluto present ...
Celestial Bodies INSTRUCTIONS - The Challenger Learning Center
Celestial Bodies INSTRUCTIONS - The Challenger Learning Center

... 69. Students should note in MOVEMENT of Asteroids that Most asteroids revolve around the Sun in orbits between Mars and Jupiter. Some asteroids do cross Earth’s orbit. 70. Rather than trying to double-click on individual asteroids, it is easier to use the Destination controls. 71. Click on the up ar ...
Jupiter`s Radio Signals
Jupiter`s Radio Signals

... band to 20 MHz and when I did the noise was S2.5 which was 1.5 dB higher. I tried 19MHz (S2.0), 18MHz (S1.5) and at 17MHz it was even with background noise and some QRM splatter from a short wave broadcast station. I wrote it all up in my combined log book/technical notebook. I had been working on a ...
accel solar system computer
accel solar system computer

... 13. Describe how the surface of Mars looks in these images. (Is it Flat? Rocky? Sandy? etc). ...
Planetary migration and the Late Heavy
Planetary migration and the Late Heavy

... reservoirs, such as the Trojans of various planets, for material that could suddenly be released by collisional or dynamical processes, long after primary accretion was finished in the inner Solar System. Unfortunately, each of these proposals has weaknesses which have precluded general acceptance a ...
Sample Schedule 2012
Sample Schedule 2012

... sun in the protoplanetary disk. They formed from compounds that had high melting points as this region was too hot for gaseous molecules like water and methane. The compounds they formed from (eg, metals [like iron, nickel, and aluminium] and rocky silicates) are relatively rare in the universe so t ...
Neptune Project
Neptune Project

... entire Solar System. Neptune has huge storms with extremely high winds. The atmosphere has dark spots, which come and go, and bright cirrus-like clouds, which change rapidly. ...
joelcrespo  - UpWardBoundGeneralScience
joelcrespo - UpWardBoundGeneralScience

... Space Probes, Pioneer 11 in 1979 and later on by the Voyager 1 and the Voyager 2. ...
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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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