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Extra-Solar Planets - Buffalo State College
Extra-Solar Planets - Buffalo State College

... They have a much greater chance of transiting their star as seen from a further outlying point than planets of the same mass in larger orbits. Due to high levels of insolation they are of a lower density than they would otherwise be. They are all thought to have migrated to their present positions b ...
name - CBSD.org
name - CBSD.org

... Description: A gravity well warps light passing behind an extrasolar planet. 3. Look through some of the exoplanets on the “extrasolar planet finder.” What is the method that was used to locate the majority of the exoplanets? Radial velocity. ...
Document
Document

... for extra-solar planetary systems, one of the most challenging astronomical activities. While spectroscopic, astrometric and photometric studies may only provide indirect evidence for planets around other stars, coronographic images like this one in principle enable astronomers to detect dusty disks ...
Physics 2028: Great Ideas in Science II: The Changing Earth Module
Physics 2028: Great Ideas in Science II: The Changing Earth Module

... produce H II regions from their strong ionizing UV flux, which initially expand outward away from the OB association. This ionization front heats the gas causing a shock to form. The shock can compress the gas such that M > MJ , which once again, leads to star formation. ...
Lecture 42
Lecture 42

... stars, of which the star T-Tauri (now known to be a binary pair) is the type example. During this phase, a visible star begins to emerge from its cocoon of gas and dust, but it remains surrounded by its circumstellar disk. The luminosity is due entirely to continued accretion and gravitational colla ...
Kepler`s Laws:
Kepler`s Laws:

... 6. )A large object called Sedna has been found past the orbit of Pluto. Parallax measurements from the Hubble Space telescope indicate Sedna is at a distance of 990 A.U. Calculations indicate its average distance from the Sun is 532 A.U., and its Perihelion is at 76 A.U. Based on this information, i ...
Basic Observations Star Formation favors smaller stars (more
Basic Observations Star Formation favors smaller stars (more

... favors smaller stars (more smaller stars observed than larger stars) favors binary or multiple star systems young stars tend to be found in clusters (=> formation occurs in localized regions bound together by gravity) associations (formed near each other, but too far apart to be bound by mutual grav ...
Grade 7 Solar system: definitions
Grade 7 Solar system: definitions

... Orbit – to circle around an object. Satellite – an object orbiting a star or planet. Star – ball of tremendously hot gas which produces heat and light from nuclear reactions in its core. Supernova – colossal explosion when a star dies. It is estimated that about 10 000 million years  after the Big ...
Earth
Earth

... standard distance from Earth) from 20 pc. • Since the star will be “closer”, it will be brighter. • A brighter star has a smaller magnitude • Thus, we expect an absolute magnitude less than ...
Great Migrations & other natural history tales
Great Migrations & other natural history tales

... zone boundaries, magnetospheric inner disk cavities, formation-caused radial disk structure) Offers possibility of survival of giant planets at intermediate distances (0.1 - 1 AU), ...and of terrestrial planets during the passage of a giant planet on its way to the star. If type I superseded by type ...
Scientists Observe Star Triplets Being Born : Space
Scientists Observe Star Triplets Being Born : Space

... multiple-star system. Scientists suspected that the process was casused by a gravitational instability, but new observations from the Atacama Large Millimeter/submillimeter Array (ALMA) and the Karl G. Jansky Very Large Array (VLA) showed the process in action. John Tobin, from the University of Okl ...
Evening sky in MARCH 2015 The three brightest stars seen from
Evening sky in MARCH 2015 The three brightest stars seen from

... Sirius, the brightest, is in the constellation of Canis Major, the Big Dog and is to the east of the three Belt Stars in Orion, the Hunter. In isiXhosa it is known as iQhawe, the 'champion'. Second brightest is Canopus in Carina, the Keel of the mythological ship, Argo, sailing high in the southern ...
powerpoint version
powerpoint version

... gas molecules, but in the disc they can be recreated more easily due to high density. 2. New dust grains condense out of the gas. 3. Tens of AU from the Sun the temperature is below 150 K (-123oC), so volatiles can condense to ices, H2O, carbon dioxide, alcohols etc. (1 AU = Earth - Sun distance) 4. ...
How is a Star`s Color Related to Its temperature?
How is a Star`s Color Related to Its temperature?

... different colors. Rigel is blue. and Betelgense is red. Capella and ore" Sun are yellow, in this activity you will make your own Hertzsprung-Russell diagram. You will see how star brightness, color. temperature, and class are related. ~Vlaterials: Colored pencils (red, orange, yellow, blue) Procedur ...
An Assessment: Think Pair Share
An Assessment: Think Pair Share

... The cosmic background radiation is visible in all directions at a temperature of 3 degrees absolute zero. Almost every galaxy has a red-shift, with more distant galaxies having the highest red-shift. The closest galaxies are all blue-shifted, showing that our universe is slowing down. ...
The Great Square in Pegasus is prominent in the northwest while
The Great Square in Pegasus is prominent in the northwest while

... Cross and Pointers are now low down on the southern horizon. To the southeast we find the mythological ship Argo, which consists of three constellations, Carina (Keel), Vela (Sails) and Puppis (Stern). The bright star in the Keel is Canopus, the second brightest star in the night sky. In isiXhosa it ...
5-SolarSystem
5-SolarSystem

... Fundamental Properties of the solar System 1. Planets and their satellites all lie in the same plane - the ecliptic – to within a few degrees 2. Sun’s rotational equator aligned with ecliptic 3. Planetary orbits are nearly circular ellipses 4. Planets all revolve in same W -> E direction 5. Sun and ...
ISO Adds a Critical Ingredient to the Jovian Planet
ISO Adds a Critical Ingredient to the Jovian Planet

... Observatory (ISO). This discovery, presented in the January 4th issue of Nature, may well help to resolve a significant problem with Jovian planet formation that had been posed by previous studies. Molecular hydrogen – H2, two hydrogen atoms joined together by a molecular bond – dominates the primor ...
Star Maps for beginners - Keighley Astronomical Society
Star Maps for beginners - Keighley Astronomical Society

... Can you spot the great square of the constellation of PEGASUS. Actually the square is not so prominent as might be thought from the above map but it should be easy to find, as it is high in the south sky at this time of year. One of its stars ‘51 Pegasi’ was the first star to be found that has an ex ...
How Special Are We? Answer: Not Very
How Special Are We? Answer: Not Very

... The Star Upsilon Andromeda What about on Moons? -We have around 141 moons in our solar system. -Jupiter’s Europa is a good possibility for life. -They are planets like Jupiter, why not moons like Europa? -The moons could also be like Earth. ...
Extrasolar Planets
Extrasolar Planets

... • only for a short fraction of the orbital period (hours) • only if Earth is nearly exactly in the orbital plane • Jupiter: 1% dimming, but Earth: 0.01% dimming! Currently the only method to discover Earth sized planets: only from space! • COROT (ESA, >2006; 30cm telescope) ...
Document
Document

... Distribution of masses of known extrasolar planets. About 1000 stars have been surveyed: a nearly complete sample of solar-type stars within 30 pc. Occurrence varies inversely with mass. ...
Extraterrestrial Life
Extraterrestrial Life

... They contain raw materials ...
New planet discovered in Trinary star system
New planet discovered in Trinary star system

... Until recently, astronomers were highly skeptical of billion years in aged, based on the amount of stellar whether or not planets should be possible in activity and amount of lithium present in the star's multiple star systems. It was expected that the atmosphere (which decreases with time). However ...
The Search for Low Mass Companions to White Dwarf Stars
The Search for Low Mass Companions to White Dwarf Stars

... We think that stars are born out of large clouds of gas that collapse to make star clusters The protostars become stars when they initiate nuclear fussion in their cores Eventually, fussion stops and the outer stellar atmosphere bloats up - a giant star! This atmosphere is blown away revealing a hot ...
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Beta Pictoris



Beta Pictoris (β Pic, β Pictoris) is the second brightest star in the constellation Pictor. It is located 63.4 light years from our solar system, and is 1.75 times as massive and 8.7 times as luminous as the Sun. The Beta Pictoris system is very young, only 8–20 million years old, although it is already in the main sequence stage of its evolution. Beta Pictoris is the title member of the Beta Pictoris moving group, an association of young stars which share the same motion through space and have the same age.Beta Pictoris shows an excess of infrared emission compared to normal stars of its type, which is caused by large quantities of dust and gas (including carbon monoxide) near the star. Detailed observations reveal a large disk of dust and gas orbiting the star, which was the first debris disk to be imaged around another star. In addition to the presence of several planetesimal belts and cometary activity, there are indications that planets have formed within this disk and that the processes of planet formation may still be ongoing. Material from the Beta Pictoris debris disk is thought to be the dominant source of interstellar meteoroids in our solar system.The European Southern Observatory (ESO) has confirmed the presence of a planet, Beta Pictoris b, matching previous predictions, through the use of direct imagery, orbiting in the plane of the debris disk surrounding the star. This planet is currently the closest extrasolar planet to its star ever photographed: the observed separation is roughly the same as the distance between Saturn and the Sun.
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