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Slides in PDF format
Slides in PDF format

...  Asteroids  =  key  population  to  progress  on  the  following  questions:      The  role  of  planetary ...
Ch11_Lecture
Ch11_Lecture

... Origin of the Asteroids • From their composition, size, and location, asteroids support the solar nebula hypothesis and are thought to be fragments of planetesimals • For this connection to be established, differentiation needed to occur in large asteroids • Fragmentation of these early large aster ...
pdf format
pdf format

... • Asteroids are small, generally rocky bodies that orbit Sun • Most asteroids (thousands – 5000 known perhaps about 100,000) lie in the asteroid belt (2-5 A.U.), a region between the orbits of Mars and Jupiter • The first asteroid (Ceres, 1801 by G. Piazzi) of this asteroid belt was discovered as a ...
The Adventure Is Waiting
The Adventure Is Waiting

... Objective ...
CIENCIAS NATURAIS – 1º de ESO
CIENCIAS NATURAIS – 1º de ESO

... In 1989 the spacecraft Galileo was launched to study the atmosphere of Jupiter and its moons. One year laterit entered the Asteroid Belt and came close to the asteroid Gaspra. Graspra is a small asteroid about 19 km long. It is composed of rock and metal typical of most of the many thousands of aste ...
Guided Notes - Duplin County Schools
Guided Notes - Duplin County Schools

... Some asteroids have very eccentric orbits and travel very near the sun, and a few larger ones regularly pass close to Earth and the moon Many of the most recent impact craters on the moon and Earth were probably caused by _____________________________ with asteroids Inevitably, future Earth-asteroid ...
Assignment #1
Assignment #1

... Assignment #1 Answer these questions using complete sentences. Be as brief but still complete and accurate as possible. A. What is basalt, and where is it found? Why? B. What ices dominate the solar system? C. Where do asteroids fit into the Solar System? D. Are asteroids found in particular orbits? ...
Asteroid Belt
Asteroid Belt

... President Barack Obama set a lofty next goal this week for Americans in space: Visiting an asteroid by 2025. But reaching a space rock in a mere 15 years is a daunting mission, and one that might also carry the ultimate safety of the planet on its shoulders. "By 2025, we expect new spacecraft design ...
Asteroids and Meteoroids
Asteroids and Meteoroids

... What are the two main parts of a comet and what are they made of? What happens to most meteor when the enter Earth’s atmosphere? If you found the next asteroid, what would you name it? According to the IAU, what can asteroids also be considered? Where are the majority of asteroids found? ...
Dwarf planets and small solar system bodies
Dwarf planets and small solar system bodies

... • A planet is a celestial body that 1. is in orbit around the Sun, 2. has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium ...
The Solar System (Planetary Debris) - NATSCI-A7
The Solar System (Planetary Debris) - NATSCI-A7

... 10 and 70 km/sec. But all but the very largest are quickly decelerated to a few hundred km/hour by atmospheric friction and hit the Earth's surface with very little fanfare. However meteoroids larger than a few hundred tons are slowed very little; only these large (and fortunately rare) ones make cr ...
The Main Points Asteroids
The Main Points Asteroids

... sky than the stars ...
Lecture 7 - University of Minnesota
Lecture 7 - University of Minnesota

... but are resupplied from the moons of the planets ...
Chapter 10 - Relativity Group
Chapter 10 - Relativity Group

... • Radioactive material in chondrules allows dating back to when they first condensed from the solar nebula • Some chondrules contain ancient dust grains that have survived from before the Solar System’s birth! ...
Universe Now - Course Pages of Physics Department
Universe Now - Course Pages of Physics Department

... dynamics of the outer Solar System during 100 years (with a time step of 200 days). White: plutinos (Pluto as large, white circle) Blue squares: comets (in perihelion around year 2002) Orange: centaurs Red: Classical TNOs Magenta: scattered disc objects Cyan: higheccentricity objects Planets: Jupite ...
Worksheet 1
Worksheet 1

... A. A small, rocky solid body orbiting the Sun and ranging in diameter from a few meters to hundreds of kilometers B. The technical name for the small, solid bodies moving within the Solar System C. A small spherical body embedded in a meteorite D. A type of meteorite containing many tiny spheres of ...
Powerpoint - BU Imaging Science
Powerpoint - BU Imaging Science

... Many Kuiper Belt Objects are in stable orbital resonances with Neptune, whereas unstable orbital resonances with Jupiter cause gaps in Asteroid Belt ...
Remnants of Rock and Ice (Chapter 12)
Remnants of Rock and Ice (Chapter 12)

... Many Kuiper Belt Objects are in stable orbital resonances with Neptune, whereas unstable orbital resonances with Jupiter cause gaps in Asteroid Belt ...
Chapter15_New
Chapter15_New

... meteor — A streak of light produced by a meteoroid moving rapidly through the Earth’s atmosphere. Friction vaporizes the meteoroid and heats atmospheric gases along the path of the meteoroid. meteor shower — A temporary increase in the normal rate at which meteors occur. Meteor showers last for a fe ...
Comets & Meteors (10)
Comets & Meteors (10)

... What is it about the outer planets that their atmospheres appear blue or blue-green? ...
A Storm of Asteroids - Lunar and Planetary Institute
A Storm of Asteroids - Lunar and Planetary Institute

... One of the largest craters in our solar system –South Pole-Aiken Basin – was discovered on the far side of our Moon. It is twice as wide as Texas and 8 miles (13 kilometers) deep, 8 times deeper than the Grand Canyon! These impact basins formed long ago during a time when a huge storm of giant aster ...
lagrange - The Institute of Mathematical Sciences
lagrange - The Institute of Mathematical Sciences

... figure) are now called Lagrange points. Two of the Lagrange points (L4 and L5) are on the orbit of the planet itself, forming equilateral triangles with the Sun and the planet. L4 will be ahead of the planet in its orbit and L5 will be behind the planet in its orbit. A contour plot of the effective ...
What are Asteroids, Meteors and Comets? How are they similar
What are Asteroids, Meteors and Comets? How are they similar

... gas that orbit the sun. Jets of gas and dust form long tails that reflect sunlight and can be seen from Earth Consist of a solid nucleus core that is surrounded by a cloudy atmosphere called a coma and has one or two tails Comets are usually only seen through a ...
OAT Asteroids:Comets
OAT Asteroids:Comets

... Sometimes they hit us… Some meteors are large enough to survive passage through the atmosphere and strike the ground with enough force to be vaporized and release large amounts of energy. They hit at 50 km/s, so a rock the size of a building can make a hole a mile across. ...
8. Welcome to the Solar System
8. Welcome to the Solar System

... • Asteroids are “minor planets” that orbit the sun (rather than objects that orbit planets as moons). • They are much smaller than the planets, with the largest being Ceres at about 1,000 km in diameter, (remember that the diameter of the Earth is about 12,800 km) and only another five or so having ...
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Asteroid



Asteroids are minor planets, especially those of the inner Solar System. The larger ones have also been called planetoids. These terms have historically been applied to any astronomical object orbiting the Sun that did not show the disc of a planet and was not observed to have the characteristics of an active comet. As minor planets in the outer Solar System were discovered and found to have volatile-based surfaces that resemble those of comets, they were often distinguished from asteroids of the asteroid belt. In this article, the term ""asteroid"" is restricted to the minor planets of the inner Solar System or co-orbital with Jupiter.There are millions of asteroids, many thought to be the shattered remnants of planetesimals, bodies within the young Sun's solar nebula that never grew large enough to become planets. The large majority of known asteroids orbit in the asteroid belt between the orbits of Mars and Jupiter, or are co-orbital with Jupiter (the Jupiter Trojans). However, other orbital families exist with significant populations, including the near-Earth asteroids. Individual asteroids are classified by their characteristic spectra, with the majority falling into three main groups: C-type, S-type, and M-type. These were named after and are generally identified with carbon-rich, stony, and metallic compositions, respectively.Only one asteroid, 4 Vesta, which has a relatively reflective surface, is normally visible to the naked eye, and this only in very dark skies when it is favorably positioned. Rarely, small asteroids passing close to Earth may be visible to the naked eye for a short time. As of September 2013, the Minor Planet Center had data on more than one million objects in the inner and outer Solar System, of which 625,000 had enough information to be given numbered designations.On 22 January 2014, ESA scientists reported the detection, for the first definitive time, of water vapor on Ceres, the largest object in the asteroid belt. The detection was made by using the far-infrared abilities of the Herschel Space Observatory. The finding is unexpected because comets, not asteroids, are typically considered to ""sprout jets and plumes"". According to one of the scientists, ""The lines are becoming more and more blurred between comets and asteroids.""
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