Excellence
... the red giants which are still burning fuel but it makes sense when you compare their surface area and mass. White dwarfs have an extremely dense inner core, which means they have a small surface area but a large mass, which causes high temperature. Looking at the H/ R diagram you can tell that whit ...
... the red giants which are still burning fuel but it makes sense when you compare their surface area and mass. White dwarfs have an extremely dense inner core, which means they have a small surface area but a large mass, which causes high temperature. Looking at the H/ R diagram you can tell that whit ...
I. What is an Exoplanet?
... Launched on March 9, 2009. Duration of the mission is expected to be about 7 to 8 years Surveying our neighbourhood in Milky way As per Jan. 2013, it has found 2740 likely candidates 105 of them have been confirmed by further studies Next space mission: Gaia. To be launched in August ...
... Launched on March 9, 2009. Duration of the mission is expected to be about 7 to 8 years Surveying our neighbourhood in Milky way As per Jan. 2013, it has found 2740 likely candidates 105 of them have been confirmed by further studies Next space mission: Gaia. To be launched in August ...
Solar System Formation
... • This was one of the big problems that astronomers in the early 1900s found with the nebular hypothesis: what sort of collapse could end up with most of the angular momentum in the solar system in Jupiter (biggish mass, big radius) but not in the Sun? ...
... • This was one of the big problems that astronomers in the early 1900s found with the nebular hypothesis: what sort of collapse could end up with most of the angular momentum in the solar system in Jupiter (biggish mass, big radius) but not in the Sun? ...
Other Solar Systems Around Other Stars
... Encounters w/ Other Planets • Planets should, by physics, form in fairly circular orbits with plenty of space between them by the time formation is about done. • But resonances can amplify eccentricity of an orbit, to the point of orbit-crossing (close encounter possible!), and then the two planets ...
... Encounters w/ Other Planets • Planets should, by physics, form in fairly circular orbits with plenty of space between them by the time formation is about done. • But resonances can amplify eccentricity of an orbit, to the point of orbit-crossing (close encounter possible!), and then the two planets ...
File - We All Love Science
... • Our Moon • Jupiter has 63, Saturn 61, Uranus 27 and Neptune 13. Mars has 2. Pluto has 4, Eris 1. ...
... • Our Moon • Jupiter has 63, Saturn 61, Uranus 27 and Neptune 13. Mars has 2. Pluto has 4, Eris 1. ...
File
... inner planets, the only one known to have current geological activity, and the only place where life is known to exist. Its liquid hydrosphere is unique among the terrestrial planets, and it is also the only planet where plate tectonics has been observed. Earth's atmosphere is radically different fr ...
... inner planets, the only one known to have current geological activity, and the only place where life is known to exist. Its liquid hydrosphere is unique among the terrestrial planets, and it is also the only planet where plate tectonics has been observed. Earth's atmosphere is radically different fr ...
Lecture 2 - University of Chicago, Astronomy
... in the telescope, but stars did not; observed all four phases of the Venus (gibbous phases could not be explained by the Ptolemaic model); discovered four largest satellites of Jupiter; they are still called Galilean moons; this was another blow to the dying Ptolemaic system. Galileo resolved the Mi ...
... in the telescope, but stars did not; observed all four phases of the Venus (gibbous phases could not be explained by the Ptolemaic model); discovered four largest satellites of Jupiter; they are still called Galilean moons; this was another blow to the dying Ptolemaic system. Galileo resolved the Mi ...
The Solar System
... approximately 55 AU from the Sun.[2] It is similar to the asteroid belt, although it is far larger—20 times as wide and 20 to 200 times as massive.[3][4] Like the asteroid belt, it consists mainly of small bodies, or remnants from the Solar System's formation. While the asteroid belt is composed pri ...
... approximately 55 AU from the Sun.[2] It is similar to the asteroid belt, although it is far larger—20 times as wide and 20 to 200 times as massive.[3][4] Like the asteroid belt, it consists mainly of small bodies, or remnants from the Solar System's formation. While the asteroid belt is composed pri ...
Chapter 29 Our Solar System
... 5. Interior: Solid core of __________, ___________, & ____________ Asteroid belt 1. Left over planetary debris from solar system formation, that never formed planets 2. Located between Mars & Jupiter 3. Separates terrestrial planets and gas giants ...
... 5. Interior: Solid core of __________, ___________, & ____________ Asteroid belt 1. Left over planetary debris from solar system formation, that never formed planets 2. Located between Mars & Jupiter 3. Separates terrestrial planets and gas giants ...
ppt
... Apparently the fine tuning of the laws of nature, the physical constants, the initial density and rate of expansion of the universe God established was sufficient over time to bring about a cosmos with unnumbered star systems that God could choose from to populate In this period God established many ...
... Apparently the fine tuning of the laws of nature, the physical constants, the initial density and rate of expansion of the universe God established was sufficient over time to bring about a cosmos with unnumbered star systems that God could choose from to populate In this period God established many ...
HABITABLE PLANETS For every star with planets, how many of
... water was delivered by asteroids that were scattered into Earth-crossing orbits by Jupiter. If no Jupiter, then maybe no water! We already saw (in Planet Formation presentation) the potentially significant effects of the presence of a giant planet and its properties on water delivery by icy planetes ...
... water was delivered by asteroids that were scattered into Earth-crossing orbits by Jupiter. If no Jupiter, then maybe no water! We already saw (in Planet Formation presentation) the potentially significant effects of the presence of a giant planet and its properties on water delivery by icy planetes ...
Lecture 21
... shift pattern for its spectral lines? (f) What is the orbital speed of the star in its orbit around the center of mass? (g) What will be the wavelength shift for a visible line (say with wavelength 500 nm)? ...
... shift pattern for its spectral lines? (f) What is the orbital speed of the star in its orbit around the center of mass? (g) What will be the wavelength shift for a visible line (say with wavelength 500 nm)? ...
where it is, how big it
... The four large Galilean moons are named after other people in Zeus’ life, most are his lovers. Jupiter is considered one of the gas planets. The gas planets are the planets in our solar system which do not have solid surfaces, their gaseous material simply gets denser with depth. What we see when l ...
... The four large Galilean moons are named after other people in Zeus’ life, most are his lovers. Jupiter is considered one of the gas planets. The gas planets are the planets in our solar system which do not have solid surfaces, their gaseous material simply gets denser with depth. What we see when l ...
Solar System
... The Kuiper Belt is an area beyond Neptune from about 30 AU out to about 50 AU that has at least 70,000 small objects with diameters greater than 100 km. (Recall that Pluto has a diameter of about 2,300 km and the earth has a diameter of about 12,800 km. Note that Pluto and Eris are Kuiper belt objec ...
... The Kuiper Belt is an area beyond Neptune from about 30 AU out to about 50 AU that has at least 70,000 small objects with diameters greater than 100 km. (Recall that Pluto has a diameter of about 2,300 km and the earth has a diameter of about 12,800 km. Note that Pluto and Eris are Kuiper belt objec ...
Basics of Atmospheres and their Formation
... • Desch et.al. (2008) show that packing the solar nebula tighter and evolving that forward can produce all the planets and Kuiper Belt observed in the time (~10 million years) needed to avoid major losses of the planetary material due to the solar wind. • His simulations show the solar nebula’s mass ...
... • Desch et.al. (2008) show that packing the solar nebula tighter and evolving that forward can produce all the planets and Kuiper Belt observed in the time (~10 million years) needed to avoid major losses of the planetary material due to the solar wind. • His simulations show the solar nebula’s mass ...
Chapter 7
... (g) All planets and moons that have a solid surface show evidence of craters. (h) All Jovian planets have ring systems. (i) Asteroids, comets, and meteoroids populate the solar system along with the planets, and each category of objects has its own pattern of motion and location. (j) The planets hav ...
... (g) All planets and moons that have a solid surface show evidence of craters. (h) All Jovian planets have ring systems. (i) Asteroids, comets, and meteoroids populate the solar system along with the planets, and each category of objects has its own pattern of motion and location. (j) The planets hav ...
DTU 8e Chap 5 Formation of the Solar System
... Uranus and Neptune were also initially worlds of rock and metal, but they attracted more water and less hydrogen and helium than the other giant planets. The Nice model of solar system formation proposes that in the outer solar system, Jupiter formed first, followed by Saturn, and then by Neptune an ...
... Uranus and Neptune were also initially worlds of rock and metal, but they attracted more water and less hydrogen and helium than the other giant planets. The Nice model of solar system formation proposes that in the outer solar system, Jupiter formed first, followed by Saturn, and then by Neptune an ...
The Origin of the Solar System
... The two types of planets can be understood with the condensation sequence caused by different conditions in the inner and the outer parts of the nebula The Solar System is different from the other planetary systems found so far: they frequently have Jovian planets close to parent stars (after migrat ...
... The two types of planets can be understood with the condensation sequence caused by different conditions in the inner and the outer parts of the nebula The Solar System is different from the other planetary systems found so far: they frequently have Jovian planets close to parent stars (after migrat ...
Slide 1
... taking a shower. Terrestrial organisms have been found in boiling water or ice cold. But it must be liquid which means the temperature cannot be too high or too low. In addition to have water on a planet’s surface, a thick atmosphere must exist. The atmospheric pressure prevents the evaporation of t ...
... taking a shower. Terrestrial organisms have been found in boiling water or ice cold. But it must be liquid which means the temperature cannot be too high or too low. In addition to have water on a planet’s surface, a thick atmosphere must exist. The atmospheric pressure prevents the evaporation of t ...
(the largest solar system planet) represents at
... Planets orbit the sun along the elliptical plane counterclockwise looking downward from above the sun’s north pole. Pluto does not orbit along the elliptical plane like the other seven planets. In fact, Pluto’s orbital plane is tilted approximately 18 degrees above the elliptical plane and is roughl ...
... Planets orbit the sun along the elliptical plane counterclockwise looking downward from above the sun’s north pole. Pluto does not orbit along the elliptical plane like the other seven planets. In fact, Pluto’s orbital plane is tilted approximately 18 degrees above the elliptical plane and is roughl ...
Navigating by the Stars
... e prhttp://www.space.com/5849-navigating-stars.htmloportional to the star formation rate, though this makes technical sense. (The product of all the terms except L tells how many new communicating civilizations are born each year. Then you multiply by the lifetime to get the expected number. For exa ...
... e prhttp://www.space.com/5849-navigating-stars.htmloportional to the star formation rate, though this makes technical sense. (The product of all the terms except L tells how many new communicating civilizations are born each year. Then you multiply by the lifetime to get the expected number. For exa ...
The Sun and planets
... The Sun and planets The Sun On our stage, the role of main actor cannot but be conferred to the Sun, a star like many others in space, but very special for us because from the remains of its formation all the planets and the smaller bodies that rotate around it, and of which we are a part, have orig ...
... The Sun and planets The Sun On our stage, the role of main actor cannot but be conferred to the Sun, a star like many others in space, but very special for us because from the remains of its formation all the planets and the smaller bodies that rotate around it, and of which we are a part, have orig ...
THE DOCTRINE OF ORIGINAL SPIN
... I presented a paper entitled “Discontinuous Ether Model” at a meeting of the NPA in Berkeley in May, 2000. I have copies here for those of you who might want one. Also it can be accessed on my web-site: www2.cruzio.com/~ftc or a slightly edited version was published by: www.journaloftheoretics.com ...
... I presented a paper entitled “Discontinuous Ether Model” at a meeting of the NPA in Berkeley in May, 2000. I have copies here for those of you who might want one. Also it can be accessed on my web-site: www2.cruzio.com/~ftc or a slightly edited version was published by: www.journaloftheoretics.com ...
Extrasolar Planets - University of Maryland Astronomy
... earlier. High-mass, short-period planets are much easier to detect than low-mass or longperiod planets. None of the terrestrial planets (Mercury through Mars) could be seen, for example. It is therefore not surprising that we have this bias. As the time of observation has lengthened, so has the maxi ...
... earlier. High-mass, short-period planets are much easier to detect than low-mass or longperiod planets. None of the terrestrial planets (Mercury through Mars) could be seen, for example. It is therefore not surprising that we have this bias. As the time of observation has lengthened, so has the maxi ...
Planet
A planet (from Ancient Greek ἀστήρ πλανήτης (astēr planētēs), or πλάνης ἀστήρ (plánēs astēr), meaning ""wandering star"") is an astronomical object orbiting a star, brown dwarf, or stellar remnant that is massive enough to be rounded by its own gravity, is not massive enough to cause thermonuclear fusion, and has cleared its neighbouring region of planetesimals.The term planet is ancient, with ties to history, science, mythology, and religion. Several planets in the Solar System can be seen with the naked eye. These were regarded by many early cultures as divine, or as emissaries of deities. As scientific knowledge advanced, human perception of the planets changed, incorporating a number of disparate objects. In 2006, the International Astronomical Union (IAU) officially adopted a resolution defining planets within the Solar System. This definition is controversial because it excludes many objects of planetary mass based on where or what they orbit. Although eight of the planetary bodies discovered before 1950 remain ""planets"" under the modern definition, some celestial bodies, such as Ceres, Pallas, Juno, Vesta (each an object in the solar asteroid belt), and Pluto (the first trans-Neptunian object discovered), that were once considered planets by the scientific community are no longer viewed as such.The planets were thought by Ptolemy to orbit Earth in deferent and epicycle motions. Although the idea that the planets orbited the Sun had been suggested many times, it was not until the 17th century that this view was supported by evidence from the first telescopic astronomical observations, performed by Galileo Galilei. By careful analysis of the observation data, Johannes Kepler found the planets' orbits were not circular but elliptical. As observational tools improved, astronomers saw that, like Earth, the planets rotated around tilted axes, and some shared such features as ice caps and seasons. Since the dawn of the Space Age, close observation by space probes has found that Earth and the other planets share characteristics such as volcanism, hurricanes, tectonics, and even hydrology.Planets are generally divided into two main types: large low-density giant planets, and smaller rocky terrestrials. Under IAU definitions, there are eight planets in the Solar System. In order of increasing distance from the Sun, they are the four terrestrials, Mercury, Venus, Earth, and Mars, then the four giant planets, Jupiter, Saturn, Uranus, and Neptune. Six of the planets are orbited by one or more natural satellites.More than a thousand planets around other stars (""extrasolar planets"" or ""exoplanets"") have been discovered in the Milky Way: as of 1 October 2015, 1968 known extrasolar planets in 1248 planetary systems (including 490 multiple planetary systems), ranging in size from just above the size of the Moon to gas giants about twice as large as Jupiter. On December 20, 2011, the Kepler Space Telescope team reported the discovery of the first Earth-sized extrasolar planets, Kepler-20e and Kepler-20f, orbiting a Sun-like star, Kepler-20. A 2012 study, analyzing gravitational microlensing data, estimates an average of at least 1.6 bound planets for every star in the Milky Way.Around one in five Sun-like stars is thought to have an Earth-sized planet in its habitable zone.