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Ch 12 slides - UNLV Physics
Ch 12 slides - UNLV Physics

... Not a gas giant like other outer planets. Has an icy composition like a comet. Has a very elliptical, inclined orbit. Pluto has more in common with comets than with the eight major planets ...
Neptune and Beyond, Asteroids, Comets
Neptune and Beyond, Asteroids, Comets

... On January 1, 1801, an 8th magnitude object moving against stars was found by Giuseppe Piazzi, a catholic monk and astronomer in Sicily. the new object was declared a new planet and named Ceres. Fifteen months later, Heinrich Olbers discovered a second object in the same region and named Pallas. Ove ...
скачати - Essays, term papers, dissertation, diplomas - ua
скачати - Essays, term papers, dissertation, diplomas - ua

... Newton’s laws of motion and law of gravitation can be used to explain the forces, position and motion of all objects in the universe. A simple analogy of how gravity controls the motion of a planet around the Sun can be shown by a mass on the end of a string being spun around in a horizontal plane a ...
The Solar System
The Solar System

... properties, locations, and movements of the Sun, planets, Galilean moons, meteors, asteroids, and comets while completing a foldable and notes. ...
Solar System Distance Activity
Solar System Distance Activity

... accommodate the string within each knot (approximately 4 cm for a double knot around the bead). Tape newspapers to the surface where the students will be marking their strings, so they do not mark up the counter or floor. For older students, measurements are made each time from the Sun to the planet ...
Attachment
Attachment

... together by gravity. The nearest star to Earth is the Sun, which is the source of most of the energy on the planet. Historically, the most prominent stars on the celestial sphere were grouped together into constellations and asterisms, and the brightest stars gained proper names. ...
Inti didn`t form in the X wind (and neither did most CAIs)
Inti didn`t form in the X wind (and neither did most CAIs)

... consistent with outer solar system as a steadystate alpha decretion disk being photoevaporated at about 60 AU (like in Orion) Dust (read: Inti) would have moved from a few AU to comet-forming zone in a few Myr ...
File
File

Dwarf Planets
Dwarf Planets

... probably associated with convection currents in the Surface features are old; Miranda is no longer geologically active. mantle, but not with impacts. ...
P3 1.7 Planetary orbits
P3 1.7 Planetary orbits

Workbook IP
Workbook IP

PPT File - Brandywine School District
PPT File - Brandywine School District

... the intriguing features of Saturn's system of rings and moons. It also delivered the European Space Agency's Huygens Probe into the atmosphere of Saturn's moon Titan. The spacecraft reached speeds of 70,700 mph on its way to the ringed planet after being launched in 1997. Just hours after it arrived ...
Physical Science Lecture Notes
Physical Science Lecture Notes

... A. Observing the Solar System 1. Greeks watched the stars move across the sky and noticed five “stars” that wandered around and did not follow the paths of the normal stars. They called them Wander Stars “planets”. 2. “Wandering Stars” were: Mercury, Venus, Mars, Jupiter and Saturn 3. Greek Astronom ...
SolarSystem Powerpoint lesson
SolarSystem Powerpoint lesson

... the intriguing features of Saturn's system of rings and moons. It also delivered the European Space Agency's Huygens Probe into the atmosphere of Saturn's moon Titan. The spacecraft reached speeds of 70,700 mph on its way to the ringed planet after being launched in 1997. Just hours after it arrived ...
Math Notes - UNC Physics and Astronomy
Math Notes - UNC Physics and Astronomy

...  We continue to discover new asteroids, both in and out of the asteroid belt, to the present day.  Planetary moons  We continue to discover new moons around Jupiter, Saturn, Uranus, and Neptune to the present day.  Neptune (1846) 20th Century  Pluto (1938)  Pluto is the first discovered member ...
Voyage of Discovery Teacher Page
Voyage of Discovery Teacher Page

... 2. Do you think humans will ever go to Mars? To other planets? If humans go to another planet, it would be to Mars because Mars is the planet most like Earth. We are close to having the technology to go. 3. Research the relationship between the distances of the planets and the length of each planet’ ...
New Worlds Observer
New Worlds Observer

... Exo-planets are the planets that circle stars other than our Sun. There are probably 10,000 exo-planets within 10pc (30 light years) of the Earth. Indirect means have now found over 200.  If we can observe them directly, we will have a new field of astronomy every bit as rich as extragalactic. ...
Chapter 4. Orbits
Chapter 4. Orbits

... This means that they are almost not moving at all when at their aphelion points and it turns out that those points are generally way beyond the orbit of Pluto and as much as 1/3 of the way to the nearest star! Nonetheless, the comets do not have hyperbolic orbits, which is the case one gets if the t ...
Gravitation
Gravitation

... A satellite is moving around the Earth in a circular orbit. Over the course of an orbit, the Earth’s gravitational force 1. does positive work on the satellite 2. does negative work on the satellite 3. does positive work on the satellite during part of the orbit and negative work on the satellite du ...
A Geometer`s Sketchpad Solar System
A Geometer`s Sketchpad Solar System

... (a) First, drag each planet to the point in its orbit where the dashed-line ray crosses the orbit. This will be the “start line”. (b) When you are ready, animate your solar system. (c) Watch how the planets move around their orbits. Look for such things as: • Which planets stay lined up as they orbi ...
Powerpoint - Sandhills Astronomical Society
Powerpoint - Sandhills Astronomical Society

... Resolution B5 (continued) (3) All other objects, except satellites, orbiting the Sun shall be referred to collectively as “Small Solar System Bodies.” These currently include most of the solar system asteroids, most Trans-Neptunian Objects (TNOs), comets, and other small bodies. ...
1698 - Lunar and Planetary Institute
1698 - Lunar and Planetary Institute

... orbital location of Neptune could easily be obtained using Kepler‘s Laws. The mass of Neptune could be estimated based on numerical simulations that produce patterns that match the brightness variation along the ring from the observations. Since Uranus does not trap IDPs efficiently and is not massi ...
About Uranus - COSTA VERDE production
About Uranus - COSTA VERDE production

Circumstellar Zones
Circumstellar Zones

... Open the Circumstellar Zone Simulator. There are four main panels:  The top panel simulation displays a visualization of a star and its planets looking down onto the plane of the solar system. The habitable zone is displayed for the particular star being simulated. One can click and drag either tow ...
Assessment - hrsbstaff.ednet.ns.ca
Assessment - hrsbstaff.ednet.ns.ca

... 10. What information do you need to find the period of a planet using Kepler’s ...
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Planets beyond Neptune



Following the discovery of the planet Neptune in 1846, there was considerable speculation that another planet might exist beyond its orbit. The search began in the mid-19th century and culminated at the start of the 20th with Percival Lowell's quest for Planet X. Lowell proposed the Planet X hypothesis to explain apparent discrepancies in the orbits of the giant planets, particularly Uranus and Neptune, speculating that the gravity of a large unseen ninth planet could have perturbed Uranus enough to account for the irregularities.Clyde Tombaugh's discovery of Pluto in 1930 appeared to validate Lowell's hypothesis, and Pluto was officially named the ninth planet. In 1978, Pluto was conclusively determined to be too small for its gravity to affect the giant planets, resulting in a brief search for a tenth planet. The search was largely abandoned in the early 1990s, when a study of measurements made by the Voyager 2 spacecraft found that the irregularities observed in Uranus's orbit were due to a slight overestimation of Neptune's mass. After 1992, the discovery of numerous small icy objects with similar or even wider orbits than Pluto led to a debate over whether Pluto should remain a planet, or whether it and its neighbours should, like the asteroids, be given their own separate classification. Although a number of the larger members of this group were initially described as planets, in 2006 the International Astronomical Union reclassified Pluto and its largest neighbours as dwarf planets, leaving Neptune the farthest known planet in the Solar System.Today, the astronomical community widely agrees that Planet X, as originally envisioned, does not exist, but the concept of Planet X has been revived by a number of astronomers to explain other anomalies observed in the outer Solar System. In popular culture, and even among some astronomers, Planet X has become a stand-in term for any undiscovered planet in the outer Solar System, regardless of its relationship to Lowell's hypothesis. Other trans-Neptunian planets have also been suggested, based on different evidence. As of March 2014, observations with the WISE telescope have ruled out the possibility of a Saturn-sized object out to 10,000 AU, and a Jupiter-sized or larger object out to 26,000 AU.
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