solar system - cayugascience
... • 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 ...
... • 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 ...
Review Worksheet - Mrs. Sepulveda's Classes
... 2. Briefly outline the theory or hypothesis which best explains the origin of the solar system and explain how the observable properties of the solar system are related to its process of formation. • A large nebula began to collapse gravitationally. As it did so, it began to spin faster, and flatte ...
... 2. Briefly outline the theory or hypothesis which best explains the origin of the solar system and explain how the observable properties of the solar system are related to its process of formation. • A large nebula began to collapse gravitationally. As it did so, it began to spin faster, and flatte ...
Asteroids
... Could human life end with an asteroid? Asteroid impacts have played an enormous role in creating Earth and in altering the course of the evolution of life. It is most likely that an asteroid impact brought the end of the dinosaurs and many other lifeforms at the end of the Mesozoic. Could one astero ...
... Could human life end with an asteroid? Asteroid impacts have played an enormous role in creating Earth and in altering the course of the evolution of life. It is most likely that an asteroid impact brought the end of the dinosaurs and many other lifeforms at the end of the Mesozoic. Could one astero ...
Vagabonds of the Solar System
... – However, Jupiter (5.2 AU) is more than 3 times farther from the Sun than Mars (1.52 AU). – A “missing planet” between 2 and 3 AU • Ceres was found in 1801 – the largest asteroid, diameter of 918 km – Distance 2.77 AU from the Sun, 4.6 years orbit period – It is also called “minor planet”, or “dwar ...
... – However, Jupiter (5.2 AU) is more than 3 times farther from the Sun than Mars (1.52 AU). – A “missing planet” between 2 and 3 AU • Ceres was found in 1801 – the largest asteroid, diameter of 918 km – Distance 2.77 AU from the Sun, 4.6 years orbit period – It is also called “minor planet”, or “dwar ...
1 - Humble ISD
... ___________________: semimajor axes less than 1.0 AU and aphelion distances greater than 0.983 AU; ___________________: semimajor axes greater than 1.0 AU and perihelion distances less than 1.017 AU ___________________: perihelion distances between 1.017 and 1.3 AU; ___________________: located near ...
... ___________________: semimajor axes less than 1.0 AU and aphelion distances greater than 0.983 AU; ___________________: semimajor axes greater than 1.0 AU and perihelion distances less than 1.017 AU ___________________: perihelion distances between 1.017 and 1.3 AU; ___________________: located near ...
asteroids, comets - MSU Solar Physics
... Its orbit is highly eccentric; at times it is closer to the Sun than Neptune. Its orbit inclination is also much larger than other planets. Pluto rotates in the opposite direction from most other planets. Pluto is smaller than 7 satellites in the solar system. It has an average density of about 1900 ...
... Its orbit is highly eccentric; at times it is closer to the Sun than Neptune. Its orbit inclination is also much larger than other planets. Pluto rotates in the opposite direction from most other planets. Pluto is smaller than 7 satellites in the solar system. It has an average density of about 1900 ...
Chart_set_4
... Cloud called "Solar Nebula". This is pre-Newton and modern science. But basic idea correct, and the theory evolved as ...
... Cloud called "Solar Nebula". This is pre-Newton and modern science. But basic idea correct, and the theory evolved as ...
Lecture14: Solar System Debris
... o Like the two categories of planets, asteroids are “inner” “terrestrial” rocky objects, comets are “outer” “Jovian” icy rocks. asteroid belt ...
... o Like the two categories of planets, asteroids are “inner” “terrestrial” rocky objects, comets are “outer” “Jovian” icy rocks. asteroid belt ...
Beyond Planet Earth: Activities for Grades 6-8
... (Answers may include: in the asteroid belt between Mars and Jupiter) What would studying asteroids up-close help scientists understand? (Answers may include: Samples could help them understand the formation of the solar system. Many asteroids contain the original debris from which the planets formed ...
... (Answers may include: in the asteroid belt between Mars and Jupiter) What would studying asteroids up-close help scientists understand? (Answers may include: Samples could help them understand the formation of the solar system. Many asteroids contain the original debris from which the planets formed ...
Asteroids
... • Comets formed near Uranus and Neptune, where water was plentiful and the temperature was low enough for ice to condense with roughly equal amounts of rocky and metallic material into bodies that still orbit the sun • Gravitational forces from Uranus and Neptune flung the comets in every direction ...
... • Comets formed near Uranus and Neptune, where water was plentiful and the temperature was low enough for ice to condense with roughly equal amounts of rocky and metallic material into bodies that still orbit the sun • Gravitational forces from Uranus and Neptune flung the comets in every direction ...
Other Objects in Our Solar System
... Asteroids • Asteroids are pieces of rock and mineral. • There is an asteroid belt which orbits the sun between Mars and Jupiter. • There are pieces which are basketball size to 940 Km (580 mi.) for the dwarf ...
... Asteroids • Asteroids are pieces of rock and mineral. • There is an asteroid belt which orbits the sun between Mars and Jupiter. • There are pieces which are basketball size to 940 Km (580 mi.) for the dwarf ...
8.E.4B.1 Our Solar System
... Our solar system is composed of eight planets in the following order from the Sun out: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune Celestial objects in our solar system include the eight planets that orbit the Sun, the moons that orbit the eight planets, and many asteroids, com ...
... Our solar system is composed of eight planets in the following order from the Sun out: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune Celestial objects in our solar system include the eight planets that orbit the Sun, the moons that orbit the eight planets, and many asteroids, com ...
ASTR100 Class 01
... In summer 2005, astronomers discovered Eris, an iceball even larger than Pluto. Eris even has a moon: Dysnomia. ...
... In summer 2005, astronomers discovered Eris, an iceball even larger than Pluto. Eris even has a moon: Dysnomia. ...
File
... 2. Some from belt / others from Mars or the Moon (not Venus) 3. ~ 1 m wide / 1 ton survive entry 4. Earth has 100 craters > .1 km, best viewed in satellite photos ...
... 2. Some from belt / others from Mars or the Moon (not Venus) 3. ~ 1 m wide / 1 ton survive entry 4. Earth has 100 craters > .1 km, best viewed in satellite photos ...
Chapter One Technology, Science, and Scientific Measurement
... An area called the asteroid belt is filled with a debris field of rocky asteroids that also orbit the Sun between a distance of 2.2 and 3.3 AU from the center of the solar system. Definition: a region in the solar system located between the orbits of Mars and Jupiter where there are a high number of ...
... An area called the asteroid belt is filled with a debris field of rocky asteroids that also orbit the Sun between a distance of 2.2 and 3.3 AU from the center of the solar system. Definition: a region in the solar system located between the orbits of Mars and Jupiter where there are a high number of ...
Slide 1
... NEOs: where do they come from? • Main Belt Asteroids (MBAs) – between Mars and Jupiter • Kuiper Belt – at or beyond the orbit of Neptune • Oort Cloud Comets (may also include larger bodies and some asteroids) – long orbits extending out >10,000 AU, 106-yr periods ...
... NEOs: where do they come from? • Main Belt Asteroids (MBAs) – between Mars and Jupiter • Kuiper Belt – at or beyond the orbit of Neptune • Oort Cloud Comets (may also include larger bodies and some asteroids) – long orbits extending out >10,000 AU, 106-yr periods ...
Chapter 9 Remnants of Rock and Ice
... • Largest is Ceres, diameter ~1,000 km • 150,000 in catalogs, and probably over a million with diameter >1 km. • Small asteroids are more common than large asteroids. • All the asteroids in the solar system wouldn’t add up to even a small terrestrial planet. ...
... • Largest is Ceres, diameter ~1,000 km • 150,000 in catalogs, and probably over a million with diameter >1 km. • Small asteroids are more common than large asteroids. • All the asteroids in the solar system wouldn’t add up to even a small terrestrial planet. ...
Chapter 12 (in pdf)
... orbit? A. There was no rocky material beyond Jupiter s orbit. B. The heaviest rocks sank towards the center of the solar system. C. Ice could form in the outer solar system. D. A passing star probably stripped away all of those asteroids, even if they were there at one time. ...
... orbit? A. There was no rocky material beyond Jupiter s orbit. B. The heaviest rocks sank towards the center of the solar system. C. Ice could form in the outer solar system. D. A passing star probably stripped away all of those asteroids, even if they were there at one time. ...
WHAT ELSE IS OUT THERE BESIDES THE PLANETS
... The word meteor is used to describe the streak of light produced as a rock in the solar system falls into Earth's atmosphere creating temporary light as a result of the friction between the atmosphere and the object. This typically occurs at heights of 50 to 68 miles above Earth's surface. Meteors a ...
... The word meteor is used to describe the streak of light produced as a rock in the solar system falls into Earth's atmosphere creating temporary light as a result of the friction between the atmosphere and the object. This typically occurs at heights of 50 to 68 miles above Earth's surface. Meteors a ...
Lecture
... Asteroids (minor planets) • Bode’s Law suggests a planet between Mars and Jup. at 2.8 AU: – 1801 – Piazzi (It.) discovers Ceres – 1804 – Juno disc. – 1807 – Vesta disc. (these are the largest asteroids) ...
... Asteroids (minor planets) • Bode’s Law suggests a planet between Mars and Jup. at 2.8 AU: – 1801 – Piazzi (It.) discovers Ceres – 1804 – Juno disc. – 1807 – Vesta disc. (these are the largest asteroids) ...
Study Guide
... Comets also come from the _______________________________. The Kuiper Belt begins just beyond the orbit of ___________________ to at least 6,000,000,000 miles from the Sun. _______________________________ (comets that return every __________ years of less) come from the Kuiper Belt. ...
... Comets also come from the _______________________________. The Kuiper Belt begins just beyond the orbit of ___________________ to at least 6,000,000,000 miles from the Sun. _______________________________ (comets that return every __________ years of less) come from the Kuiper Belt. ...
Lecture - Faculty
... Asteroids (minor planets) • Bode’s Law suggests a planet between Mars and Jup. at 2.8 AU: – 1801 – Piazzi (It.) discovers Ceres – 1804 – Juno disc. – 1807 – Vesta disc. (these are the largest ...
... Asteroids (minor planets) • Bode’s Law suggests a planet between Mars and Jup. at 2.8 AU: – 1801 – Piazzi (It.) discovers Ceres – 1804 – Juno disc. – 1807 – Vesta disc. (these are the largest ...
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.""