Powerpoint file
... before: • Demonstrated precision of 1 mas and noise floor of 0.3 mas amplitude. • Multiple measurements of nearest 60 F-, G-, and K- stars. • Directly test rocky planet formation ...
... before: • Demonstrated precision of 1 mas and noise floor of 0.3 mas amplitude. • Multiple measurements of nearest 60 F-, G-, and K- stars. • Directly test rocky planet formation ...
PPT - osmaston.org.uk
... would inhibit nucleation or induce evaporation thereafter. So we must be seeing these systems not long after they have moved out of their planetogenic cloud. 2. The two-stage scenario. Despite its close-in position (0.052 AU), the planet of 51 Pegasi, an early discovery, belongs to a star ~8 Ga old; ...
... would inhibit nucleation or induce evaporation thereafter. So we must be seeing these systems not long after they have moved out of their planetogenic cloud. 2. The two-stage scenario. Despite its close-in position (0.052 AU), the planet of 51 Pegasi, an early discovery, belongs to a star ~8 Ga old; ...
PISGAH Text by Dr. Bob Hayward ASTRONOMICAL Astronomer
... Sagittarius with its distinctive teapot asterism. Incidentally, way far behind Mercury is the planet Pluto. Of course, Pluto is much, much too faint to be seen with the naked eye; a large telescope is needed for that. Why are the planets clustered in the morning skies these mornings? There is no par ...
... Sagittarius with its distinctive teapot asterism. Incidentally, way far behind Mercury is the planet Pluto. Of course, Pluto is much, much too faint to be seen with the naked eye; a large telescope is needed for that. Why are the planets clustered in the morning skies these mornings? There is no par ...
The solar system - MissWilsonastrounit
... List the planets in order from closest to the sun to furthest. (NB Pluto is no longer considered to be a planet, it is a dwarf planet) ...
... List the planets in order from closest to the sun to furthest. (NB Pluto is no longer considered to be a planet, it is a dwarf planet) ...
The Solar Nebula Theory
... – Mathematical models indicate that the reason asteroids are there and not a planet is that Jupiter’s massive size disturbed the planetesimals and they did not accrete – instead they collided at high speeds. ...
... – Mathematical models indicate that the reason asteroids are there and not a planet is that Jupiter’s massive size disturbed the planetesimals and they did not accrete – instead they collided at high speeds. ...
Mountain Skies - Pisgah Astronomical Research Institute
... god of war. We have kept this name on modern star maps. This summer we have two naked-eye planets nearby. To the east in the constellation of Libra the scales is that god of war, Mars/Ares. Note its color in comparison with Antares. And just above Antares is the planet Saturn. This Antares–Mars–Sat ...
... god of war. We have kept this name on modern star maps. This summer we have two naked-eye planets nearby. To the east in the constellation of Libra the scales is that god of war, Mars/Ares. Note its color in comparison with Antares. And just above Antares is the planet Saturn. This Antares–Mars–Sat ...
Terrestrial Planet (and Life) Finder
... before: • Demonstrated precision of 1 µas and noise floor of 0.3 µas amplitude. • Multiple measurements of nearest 60 F-, G-, and K- stars. • Directly test rocky planet formation ...
... before: • Demonstrated precision of 1 µas and noise floor of 0.3 µas amplitude. • Multiple measurements of nearest 60 F-, G-, and K- stars. • Directly test rocky planet formation ...
Group 1 Notes for Week 8 - UGA Physics and Astronomy
... = Terrestrial Planets: small; rocky/metallic; 0-2 moons; high density vs. Outer Solar System = Jovian Planets (“Gas Giants”): lots of moons; ring systems; low density So, there is an enormous difference between the inner and outer planets: quantitatively and qualitatively. So, an explanation for the ...
... = Terrestrial Planets: small; rocky/metallic; 0-2 moons; high density vs. Outer Solar System = Jovian Planets (“Gas Giants”): lots of moons; ring systems; low density So, there is an enormous difference between the inner and outer planets: quantitatively and qualitatively. So, an explanation for the ...
Test 2 review session
... disk around young star with ring structure. Unseen planet sweeping out gap? ...
... disk around young star with ring structure. Unseen planet sweeping out gap? ...
The Solar System
... • Pieces of rocks that accumulated to form planets • Left over planetesimals are in the Kuiper belt beyond the orbit of Neptune • Pluto may actually just be the largest object in this belt ...
... • Pieces of rocks that accumulated to form planets • Left over planetesimals are in the Kuiper belt beyond the orbit of Neptune • Pluto may actually just be the largest object in this belt ...
The Solar System 2003
... Apart from the eight planets in the Solar System, there is also known a few hundreds of extrasolar planets, which orbit foreign stars. Contemporary astronomical instruments do not allow to observe these distant planets directly, but their properties are calculated from photometric and astrometric m ...
... Apart from the eight planets in the Solar System, there is also known a few hundreds of extrasolar planets, which orbit foreign stars. Contemporary astronomical instruments do not allow to observe these distant planets directly, but their properties are calculated from photometric and astrometric m ...
Document
... Planet – A celestial object, larger than asteroids or comets that revolve around a star without giving off its own light. Background source: 1Wyrmshadow1 website ...
... Planet – A celestial object, larger than asteroids or comets that revolve around a star without giving off its own light. Background source: 1Wyrmshadow1 website ...
Exoplanet Working Group
... • Background eclipsing binaries are source of confusion • Characterization of the transits requires other analysis of the signal • CoRoT detectivity limitation: (1.1 R 3days) on M0 dwarf stars Results are to be published and LCs will be available on request CoRoT-Brazil ...
... • Background eclipsing binaries are source of confusion • Characterization of the transits requires other analysis of the signal • CoRoT detectivity limitation: (1.1 R 3days) on M0 dwarf stars Results are to be published and LCs will be available on request CoRoT-Brazil ...
Goal: To understand how Saturn formed and what its core is like
... • Others could have been captured comets later. • All orbit the planet backwards (retrograde). ...
... • Others could have been captured comets later. • All orbit the planet backwards (retrograde). ...
presentation format
... Copernicus, a Polish astronomer, suggested a dramatically different model of the Solar System, a heliocentric model, with the Sun at the center Copernicus preserved the idea that planets orbited in circular orbits around the Sun, however. Big debate ensued, between geocentric and heliocentric mode ...
... Copernicus, a Polish astronomer, suggested a dramatically different model of the Solar System, a heliocentric model, with the Sun at the center Copernicus preserved the idea that planets orbited in circular orbits around the Sun, however. Big debate ensued, between geocentric and heliocentric mode ...
Another Earth in the Universe
... large stars and therefore are the best candidates for planetary systems in which life could be present. In fact, for biological evolution and for biochemical reactions to take place, very long periods of time are required, longer than the average age of the large stars. Furthermore, M dwarfs are ver ...
... large stars and therefore are the best candidates for planetary systems in which life could be present. In fact, for biological evolution and for biochemical reactions to take place, very long periods of time are required, longer than the average age of the large stars. Furthermore, M dwarfs are ver ...
The Origin of the Solar System Chapter 8:
... 1) Observations of extrasolar planets indicate that Jovian planets are common. 2) Protoplanetary disks tend to be evaporated quickly (typically within ~ 100,000 years) by the radiation of nearby massive stars. ...
... 1) Observations of extrasolar planets indicate that Jovian planets are common. 2) Protoplanetary disks tend to be evaporated quickly (typically within ~ 100,000 years) by the radiation of nearby massive stars. ...
The Solar System - Belle Vernon Area School District
... white, red, tan and brown swirling in high pressure gas • The Giant Red Spot is a continuous storm that has been raging for at least 300 years ...
... white, red, tan and brown swirling in high pressure gas • The Giant Red Spot is a continuous storm that has been raging for at least 300 years ...
Question 1 (7-5 thru 7-7 PPT Questions)
... 3. The temperature of a substance is defined by the average energy of its molecules. 4. There is little free hydrogen in Earth’s atmosphere because low-mass hydrogen molecules can achieve escape velocity at the temperatures of the upper atmosphere. 5. On the sunlit side of the Moon even molecules o ...
... 3. The temperature of a substance is defined by the average energy of its molecules. 4. There is little free hydrogen in Earth’s atmosphere because low-mass hydrogen molecules can achieve escape velocity at the temperatures of the upper atmosphere. 5. On the sunlit side of the Moon even molecules o ...
Characteristic Properties
... 1. Planets isolated in space=cleared orbit 2. Disk shape of solar system- small orbit inclination; prograde circular motion; same tilt&direction of rotation axes (almost) 3. Jovian/Terrestrial planets: low/high density, huge/small atmospheres, fast/slower rotation rates, many/few moons & rings 4. ...
... 1. Planets isolated in space=cleared orbit 2. Disk shape of solar system- small orbit inclination; prograde circular motion; same tilt&direction of rotation axes (almost) 3. Jovian/Terrestrial planets: low/high density, huge/small atmospheres, fast/slower rotation rates, many/few moons & rings 4. ...
THE DEFINITION OF PLANET: A DYNAMICIST`S POINT OF VIEW
... 2. THE IAU RESOLUTION IAU Resolution B5, adopted at the 26th IAU General Assembly, states: A planet is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, a ...
... 2. THE IAU RESOLUTION IAU Resolution B5, adopted at the 26th IAU General Assembly, states: A planet is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, a ...
Teacher notes and student sheets
... There are a lot of stars in the galaxy – about 100 billion, which we can write as 100 000 000 000 or as 1011. That is the value of S in the equation. Since the 1990s, very many ‘exoplanets’ have been found. It is estimated that much more than 10% of Sun-like stars have planets in orbit around them. ...
... There are a lot of stars in the galaxy – about 100 billion, which we can write as 100 000 000 000 or as 1011. That is the value of S in the equation. Since the 1990s, very many ‘exoplanets’ have been found. It is estimated that much more than 10% of Sun-like stars have planets in orbit around them. ...
Ch 8.3 - The Solar System
... Figure 2: Pluto does not meet the criteria for a planet because its tilted orbit crosses Neptune’s orbit. - Pluto was once considered a planet. - After 2006, the definition of a planet changed, Pluto was no longer considered a planet. - It was newly categorized as a Dwarf Planet. - Pluto orbits the ...
... Figure 2: Pluto does not meet the criteria for a planet because its tilted orbit crosses Neptune’s orbit. - Pluto was once considered a planet. - After 2006, the definition of a planet changed, Pluto was no longer considered a planet. - It was newly categorized as a Dwarf Planet. - Pluto orbits the ...
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.