![The Search for Extrasolar Planets](http://s1.studyres.com/store/data/017376087_1-e485ab6fc89e184b0ce51c8144055291-300x300.png)
The Search for Extrasolar Planets
... The need for additional information about extrasolar planetary orbits pushed astronomers to look for more ways to detect and study them, other than radial velocities. This led to the first discoveries of planetary transits. The phenomenon is well-known in the context of the Solar System, where Venus ...
... The need for additional information about extrasolar planetary orbits pushed astronomers to look for more ways to detect and study them, other than radial velocities. This led to the first discoveries of planetary transits. The phenomenon is well-known in the context of the Solar System, where Venus ...
View/Open - SUNY DSpace
... debatable. One of the strongest theories on it is called The Solar Nebula Theory; Our solar system was probably formed out of a spinning ball of gas (Stander). When this ball became bright enough, it exploded and blew dust and gases into space, leaving gravity to work for the dust and gas to form to ...
... debatable. One of the strongest theories on it is called The Solar Nebula Theory; Our solar system was probably formed out of a spinning ball of gas (Stander). When this ball became bright enough, it exploded and blew dust and gases into space, leaving gravity to work for the dust and gas to form to ...
Dynamics of disks with planets
... discovered extrasolar planetary systems. The properties of these systems were unexpected. This motivated theorists to extend and revise many preexisting theories. Important extensions include migration of bodies and planetary eccentricity pumping by planet-planet interaction, and primordial disk-pla ...
... discovered extrasolar planetary systems. The properties of these systems were unexpected. This motivated theorists to extend and revise many preexisting theories. Important extensions include migration of bodies and planetary eccentricity pumping by planet-planet interaction, and primordial disk-pla ...
Keplerian Motion
... Kepler’s Third Law • Relationship between semi-major axis a (size of orbit) and sidereal period P • P2 = a3 • P is in years, a is in AU units ...
... Kepler’s Third Law • Relationship between semi-major axis a (size of orbit) and sidereal period P • P2 = a3 • P is in years, a is in AU units ...
We see apparent retrograde motion when we pass by a
... too small to notice with the naked eye 2. Earth does not orbit Sun; it is the center of the universe With rare exceptions such as Aristarchus, the Greeks rejected the correct explanation (1) because they did not think the stars could be that far away Thus setting the stage for the long, historical ...
... too small to notice with the naked eye 2. Earth does not orbit Sun; it is the center of the universe With rare exceptions such as Aristarchus, the Greeks rejected the correct explanation (1) because they did not think the stars could be that far away Thus setting the stage for the long, historical ...
There are three main classes of meteorites:
... The Perth Meteorite fell in 1830, but very little was recovered, and now only 2 grams are known to survive. The Strathmore Meteorite fell in 1917. It broke into four fragments (Easter Essendy (22.25lb), Carsie (2lb 6oz), and Keithick(2.5lb), and one in Forfarshire at South Corston (2lb 5oz)) In tota ...
... The Perth Meteorite fell in 1830, but very little was recovered, and now only 2 grams are known to survive. The Strathmore Meteorite fell in 1917. It broke into four fragments (Easter Essendy (22.25lb), Carsie (2lb 6oz), and Keithick(2.5lb), and one in Forfarshire at South Corston (2lb 5oz)) In tota ...
accel solar system computer
... 17. What is the composition of Jupiter’s atmosphere? How does this compare to our Sun? Click on Size comparison. How does Earth compare in size to its Great Red Spot? Go back to Jupiter Stats. Click on Saturn on the diagram. Click on “Saturn Stats” 18. How fast are its wind speeds? 19. What is Satur ...
... 17. What is the composition of Jupiter’s atmosphere? How does this compare to our Sun? Click on Size comparison. How does Earth compare in size to its Great Red Spot? Go back to Jupiter Stats. Click on Saturn on the diagram. Click on “Saturn Stats” 18. How fast are its wind speeds? 19. What is Satur ...
Chapter 22: The Precambrian Earth
... rocks are between 4.1- and 4.2 billion years old. The zircon existed before it became cemented into the sedimentary rocks, and scientists theorize that the zircon is the eroded residue left behind from 4.1 to 4.2-billion-year-old granitic crustal rocks. Based on this evidence, Earth must be at least ...
... rocks are between 4.1- and 4.2 billion years old. The zircon existed before it became cemented into the sedimentary rocks, and scientists theorize that the zircon is the eroded residue left behind from 4.1 to 4.2-billion-year-old granitic crustal rocks. Based on this evidence, Earth must be at least ...
Planetary Systems Around White Dwarfs Given the ubiquity of
... Boris Gänsicke, [email protected] ...
... Boris Gänsicke, [email protected] ...
CURRICULUM TOOL – Insolation and Seasons
... 1.1h The Sun’s apparent path through the sky varies with latitude and season. Major Understandings: 2.2a Insolation (solar radiation) heats Earth’s surface and atmosphere unequally due to variations in: The intensity caused by differences in atmospheric transparency and angle of incidence which va ...
... 1.1h The Sun’s apparent path through the sky varies with latitude and season. Major Understandings: 2.2a Insolation (solar radiation) heats Earth’s surface and atmosphere unequally due to variations in: The intensity caused by differences in atmospheric transparency and angle of incidence which va ...
Document
... were revealed by the ROSAT all-sky survey. The XMM-Newton observatory allows us to resolve more point sources than ever before. When these are removed, spectra of the underlying soft x-ray background (SXRB) can be extracted and high resolution spectroscopy performed. ...
... were revealed by the ROSAT all-sky survey. The XMM-Newton observatory allows us to resolve more point sources than ever before. When these are removed, spectra of the underlying soft x-ray background (SXRB) can be extracted and high resolution spectroscopy performed. ...
Terrestrial Planets
... • A world can have a magnetic field if charged particles are moving inside. • Three requirements: – Molten, electrically conducting interior – Convection – Moderately rapid rotation ...
... • A world can have a magnetic field if charged particles are moving inside. • Three requirements: – Molten, electrically conducting interior – Convection – Moderately rapid rotation ...
We Are Stardust … Concentrated by Earth!
... and iron (O, Mg, Si, Fe)—with traces of many other elements, among which the great components of the solar system, hydrogen and helium, are very minor. Somehow, Earth has selectively accumulated some of the rarer elements of the solar system. Let us see how this great geochemical discovery can be ex ...
... and iron (O, Mg, Si, Fe)—with traces of many other elements, among which the great components of the solar system, hydrogen and helium, are very minor. Somehow, Earth has selectively accumulated some of the rarer elements of the solar system. Let us see how this great geochemical discovery can be ex ...
The Search for Extrasolar Earth-like Planets
... calculations of the orbital stability of an Earth-mass planet at various semi-major axes for specific systems with known giant planets give a more concrete answer about which stars are dynamically able to harbor terrestrial planets at terrestrial-like semi -major axes. Transits as a Planet Detection ...
... calculations of the orbital stability of an Earth-mass planet at various semi-major axes for specific systems with known giant planets give a more concrete answer about which stars are dynamically able to harbor terrestrial planets at terrestrial-like semi -major axes. Transits as a Planet Detection ...
By Shannon and Sonia
... • The rings are made of water ,ice and rock. Saturn's rings discovered? • There are over a dozen rings around Saturn. ...
... • The rings are made of water ,ice and rock. Saturn's rings discovered? • There are over a dozen rings around Saturn. ...
P3 1.7 Planetary orbits
... Be able to explain that; 1. The force of gravity provides the centripetal force that keeps planets and satellites moving in their orbits. 2. To stay at a particular distance, a planet must move at a particular speed around the sun. 3. The larger the orbit the slower the speed and the longer it takes ...
... Be able to explain that; 1. The force of gravity provides the centripetal force that keeps planets and satellites moving in their orbits. 2. To stay at a particular distance, a planet must move at a particular speed around the sun. 3. The larger the orbit the slower the speed and the longer it takes ...
File
... • It is considered a gas planet because it is composed of only gasses. Methane is one of the prominent gasses in it’s structure which is why it is blue. • Uranus has 16 moons* • Revolution Period: 83.75 Years* • Rotation Period: .72 days* ...
... • It is considered a gas planet because it is composed of only gasses. Methane is one of the prominent gasses in it’s structure which is why it is blue. • Uranus has 16 moons* • Revolution Period: 83.75 Years* • Rotation Period: .72 days* ...
October 2006 - Skyscrapers, Inc.
... and metal. Most asteroids appear to be made of some combination of relatively heavy metals such as nickel and iron with some stone and carbonaceous material thrown in. [11, pages 113, 119, 131, 200, 204] Some theorists maintain that many if not most asteroids are what is left when all the ices in a ...
... and metal. Most asteroids appear to be made of some combination of relatively heavy metals such as nickel and iron with some stone and carbonaceous material thrown in. [11, pages 113, 119, 131, 200, 204] Some theorists maintain that many if not most asteroids are what is left when all the ices in a ...
Astrobiology: young science, old questions
... planets have yet been discovered, the first will which planets are most suited to the develop- was very young. Consequently, the HZ around be found within the next couple of years, and so ment of life? In this article we provide a brief a given star will gradually drift outwards. Just the time is ri ...
... planets have yet been discovered, the first will which planets are most suited to the develop- was very young. Consequently, the HZ around be found within the next couple of years, and so ment of life? In this article we provide a brief a given star will gradually drift outwards. Just the time is ri ...
Motions of Earth, the Moon, and Planets
... Phases of the Moon The Moon, like all celestial objects in the Solar System, is illuminated by the Sun. However, the illuminated side does not always face Earth, which means that we see different amounts of the lit side as the Moon orbits Earth. Over a period of about 4 weeks, the amount of the illu ...
... Phases of the Moon The Moon, like all celestial objects in the Solar System, is illuminated by the Sun. However, the illuminated side does not always face Earth, which means that we see different amounts of the lit side as the Moon orbits Earth. Over a period of about 4 weeks, the amount of the illu ...
Pluto is no longer a planet.
... Give us back our ninth planet, you planet robbers!! today at the downgrading of Pluto (named after the Disney dog*) to a Dwarf Planet. Pluto has been a planet for as long as we can ...
... Give us back our ninth planet, you planet robbers!! today at the downgrading of Pluto (named after the Disney dog*) to a Dwarf Planet. Pluto has been a planet for as long as we can ...
Document
... abundant in the inner regions of the solar system when planets formed. There was far more water in the outer regions of the solar system than among the inner planets. Where did our water come from?” Still subject of debate, comets - heavy bombardment? Ward and Brownlee Rare Earth, p 261. ...
... abundant in the inner regions of the solar system when planets formed. There was far more water in the outer regions of the solar system than among the inner planets. Where did our water come from?” Still subject of debate, comets - heavy bombardment? Ward and Brownlee Rare Earth, p 261. ...
Rock Identification - Faculty Server Contact
... The earth is a very dynamic body and rock material is continually recycled. Plate tectonics is the description of this dynamic process. New material rising from deep in the mantle of the earth is added to the crust of the earth along mid-ocean ridge systems and crust is returned to the mantle at sub ...
... The earth is a very dynamic body and rock material is continually recycled. Plate tectonics is the description of this dynamic process. New material rising from deep in the mantle of the earth is added to the crust of the earth along mid-ocean ridge systems and crust is returned to the mantle at sub ...
Late Heavy Bombardment
![](https://commons.wikimedia.org/wiki/Special:FilePath/Lunar_cataclysm.jpg?width=300)
The Late Heavy Bombardment (abbreviated LHB and also known as the lunar cataclysm) is a hypothetical event thought to have occurred approximately 4.1 to 3.8 billion years (Ga) ago, corresponding to the Neohadean and Eoarchean eras on Earth. During this interval, a disproportionately large number of asteroids apparently collided with the early terrestrial planets in the inner Solar System, including Mercury, Venus, Earth, and Mars. The LHB happened after the Earth and other rocky planets had formed and accreted most of their mass, but still quite early in Earth's history.Evidence for the LHB derives from lunar samples brought back by the Apollo astronauts. Isotopic dating of Moon rocks implies that most impact melts occurred in a rather narrow interval of time. Several hypotheses are now offered to explain the apparent spike in the flux of impactors (i.e. asteroids and comets) in the inner Solar System, but no consensus yet exists. The Nice model is popular among planetary scientists; it postulates that the gas giant planets underwent orbital migration and scattered objects in the asteroid and/or Kuiper belts into eccentric orbits, and thereby into the path of the terrestrial planets. Other researchers argue that the lunar sample data do not require a cataclysmic cratering event near 3.9 Ga, and that the apparent clustering of impact melt ages near this time is an artifact of sampling materials retrieved from a single large impact basin. They also note that the rate of impact cratering could be significantly different between the outer and inner zones of the Solar System.