The Origin of Our Solar System
... Formation of Planets • Condensation temperature determines whether a certain substance is a solid or a gas. – Above the condensation temperature, gas state – Below the condensation temperature, solid sate • Hydrogen and Helium: always in gas state, because concentration temperatures close to absolu ...
... Formation of Planets • Condensation temperature determines whether a certain substance is a solid or a gas. – Above the condensation temperature, gas state – Below the condensation temperature, solid sate • Hydrogen and Helium: always in gas state, because concentration temperatures close to absolu ...
The Solar System (Ch. 6 in text) The solar system consists of the Sun
... B. Astrometric method—search for periodic motions of the star in the plane of the sky, detecting the “wobble” directly. Size of the angular variation depends of the mass of the invisible planet. Works best for massive planets far from star (so center of mass is located further from center of star, s ...
... B. Astrometric method—search for periodic motions of the star in the plane of the sky, detecting the “wobble” directly. Size of the angular variation depends of the mass of the invisible planet. Works best for massive planets far from star (so center of mass is located further from center of star, s ...
AST301.Ch6.15.SolarSystems - University of Texas Astronomy
... B. Astrometric method—search for periodic motions of the star in the plane of the sky, detecting the “wobble” directly. Size of the angular variation depends of the mass of the invisible planet. Works best for massive planets far from star (so center of mass is located further from center of star, s ...
... B. Astrometric method—search for periodic motions of the star in the plane of the sky, detecting the “wobble” directly. Size of the angular variation depends of the mass of the invisible planet. Works best for massive planets far from star (so center of mass is located further from center of star, s ...
PSC1010 Introduction to Astronomy Quiz #3 Review Thursday 3
... --> Water, ethane, methane, ammonia may only condense from gas to liquid or solid where it is cool, far from the sun --> Therefore, inner planets are rocky; outer planets are mostly gas and liquid with rocky cores --> Since more elements may condense where the nebula is cool, there are more planetbu ...
... --> Water, ethane, methane, ammonia may only condense from gas to liquid or solid where it is cool, far from the sun --> Therefore, inner planets are rocky; outer planets are mostly gas and liquid with rocky cores --> Since more elements may condense where the nebula is cool, there are more planetbu ...
From Big bang to lives on planets
... • The biggest surprises are findings of many Jupiter-sized planets very close to their parent stars • Some, called "Hot Jupiters", are on orbits smaller than that of Mercury, and have periods less than 10 days! • What is going on? This is a subject of much current research. • The discovery of extras ...
... • The biggest surprises are findings of many Jupiter-sized planets very close to their parent stars • Some, called "Hot Jupiters", are on orbits smaller than that of Mercury, and have periods less than 10 days! • What is going on? This is a subject of much current research. • The discovery of extras ...
Document
... The Sun is a star at the center of our Solar System. The Sun will consume the Earth one day. When all the hydrogen has been burned, the Sun will continue for about 130 million more years burning helium. It will expand and engulf Mercury, Venus, and Earth. At that point it will become a Red Gi ...
... The Sun is a star at the center of our Solar System. The Sun will consume the Earth one day. When all the hydrogen has been burned, the Sun will continue for about 130 million more years burning helium. It will expand and engulf Mercury, Venus, and Earth. At that point it will become a Red Gi ...
Quiz # 1 - Oglethorpe University
... c. the Sun moved among the planets, and pulled them out of their circular orbits d. the planets moved on a small circle whose center in turn circled a point near the Earth e. you can't fool me, Ptolemy's system did not include ANY explanation of retrograde motion We now know that the orbit of a stab ...
... c. the Sun moved among the planets, and pulled them out of their circular orbits d. the planets moved on a small circle whose center in turn circled a point near the Earth e. you can't fool me, Ptolemy's system did not include ANY explanation of retrograde motion We now know that the orbit of a stab ...
L1 Solar system
... •rocky composition, some with significant water content •a few 100’000 known. •total mass 1/30 of lunar mass (1 lunar mass ~1/81 ME): not a destroyed planet. •26 with diameters larger than 200 km. Largest: Ceres 900 km. •2.2 AU < a < 3.2 AU for 95%: between Mars and Jupiter •existence of families (g ...
... •rocky composition, some with significant water content •a few 100’000 known. •total mass 1/30 of lunar mass (1 lunar mass ~1/81 ME): not a destroyed planet. •26 with diameters larger than 200 km. Largest: Ceres 900 km. •2.2 AU < a < 3.2 AU for 95%: between Mars and Jupiter •existence of families (g ...
Star Systems FINAL EXAM STUDY GUIDE
... -Even though you wont be asked to identify images of them, you should know the names of Uranus’ and Pluto’s major Moons, as well as some of the other moons of Saturn. The fact that Uranus’ moons are named after Shakespeare characters. Pluto’s known moons are Charon, Styx, Nix, Kerberos, and Hydra. K ...
... -Even though you wont be asked to identify images of them, you should know the names of Uranus’ and Pluto’s major Moons, as well as some of the other moons of Saturn. The fact that Uranus’ moons are named after Shakespeare characters. Pluto’s known moons are Charon, Styx, Nix, Kerberos, and Hydra. K ...
Lecture17 - UCSB Physics
... originally described "wanderers" that were known only as moving lights in the sky. Recent discoveries lead us to create a new definition, which we can make using currently available scientific information. ...
... originally described "wanderers" that were known only as moving lights in the sky. Recent discoveries lead us to create a new definition, which we can make using currently available scientific information. ...
Astronomy 1 – Winter 2011
... originally described "wanderers" that were known only as moving lights in the sky. Recent discoveries lead us to create a new definition, which we can make using currently available scientific information. ...
... originally described "wanderers" that were known only as moving lights in the sky. Recent discoveries lead us to create a new definition, which we can make using currently available scientific information. ...
Unit 3: Understanding the Universe
... Enduring Understandings The solar system contains planets, dwarf planets, comets, asteroids, and other small solar system bodies. ...
... Enduring Understandings The solar system contains planets, dwarf planets, comets, asteroids, and other small solar system bodies. ...
New Scientist Magazine - Surrey, England… 19th November 2008
... It sounds like a simple enough wish list, but finding a planet that fulfils all of these criteria has kept astronomers busy for decades. Until recently, it meant finding a planet in the "Goldilocks zone" - orbiting its star at just the right distance to keep surface water liquid rather than being bo ...
... It sounds like a simple enough wish list, but finding a planet that fulfils all of these criteria has kept astronomers busy for decades. Until recently, it meant finding a planet in the "Goldilocks zone" - orbiting its star at just the right distance to keep surface water liquid rather than being bo ...
ExoplanetWorksheet
... *There are two ways to plot the data on each axis (linear and logarithmic). For ‘planet mass’ do you get better detail when you plot with linear or logarithmic data points? __________________________________ *All of the rocky planets in our Solar System are at least 3 times more dense than Jupiter. ...
... *There are two ways to plot the data on each axis (linear and logarithmic). For ‘planet mass’ do you get better detail when you plot with linear or logarithmic data points? __________________________________ *All of the rocky planets in our Solar System are at least 3 times more dense than Jupiter. ...
The Origin of the Solar System
... Earth has diameter 0.3 mm. Sun: ~ size of a small plum. Mercury, Venus, Earth, Mars: ~ size of a grain of salt. Jupiter: ~ size of an apple seed. Saturn: ~ slightly smaller than Jupiter’s “apple seed”. ...
... Earth has diameter 0.3 mm. Sun: ~ size of a small plum. Mercury, Venus, Earth, Mars: ~ size of a grain of salt. Jupiter: ~ size of an apple seed. Saturn: ~ slightly smaller than Jupiter’s “apple seed”. ...
WARM-UP # 32 Which planets are the terrestrial planets and which
... anymore? What makes it a dwarf planet? Pluto does not clear its orbit. There are many space objects in Pluto’s orbit. ...
... anymore? What makes it a dwarf planet? Pluto does not clear its orbit. There are many space objects in Pluto’s orbit. ...
ph507-16-1exo1
... An extrasolar planet, or exoplanet, is a planet outside the Solar System. 1. Outside our solar system 2. Nuclear fusion not significant 3. Less than 13/1000 of our Suns mass = Less than 13 Jupiter masses Definition of a star/brown dwarf/planet • Stars: burn hydrogen (M > 0.075 Msun) • Brown dwarfs: ...
... An extrasolar planet, or exoplanet, is a planet outside the Solar System. 1. Outside our solar system 2. Nuclear fusion not significant 3. Less than 13/1000 of our Suns mass = Less than 13 Jupiter masses Definition of a star/brown dwarf/planet • Stars: burn hydrogen (M > 0.075 Msun) • Brown dwarfs: ...
What makes a planet habitable?
... to finding a world similar to Earth. MIDDLE: The habitable zone. BOTTOM: Light from exoplanets, if passed through a prism, can be spread out into a rainbow of colors called a spectrum. Different colors correspond to different wavelengths of light. Missing colors show up as black lines, indicating spe ...
... to finding a world similar to Earth. MIDDLE: The habitable zone. BOTTOM: Light from exoplanets, if passed through a prism, can be spread out into a rainbow of colors called a spectrum. Different colors correspond to different wavelengths of light. Missing colors show up as black lines, indicating spe ...
Why SETI will Fail
... creatures will follow the latter path -• Exploration of our solar system began with telescopic observations from Earth. But as soon as we developed the capability, we launched spaceships to explore planets and moons up close because observing from afar is limited and, ultimately, unsatisfying. ...
... creatures will follow the latter path -• Exploration of our solar system began with telescopic observations from Earth. But as soon as we developed the capability, we launched spaceships to explore planets and moons up close because observing from afar is limited and, ultimately, unsatisfying. ...
Article on Pluto (for 1st science news)
... 250-year revolution. This means that Xena is sometimes much closer to Earth than Pluto-although never closer than Neptune. Note: Xena now has the official name of “Eris”. In Greek mythology, Eris is the goddess of warfare and strife. She stirs up jealousy and envy to cause fighting and anger among m ...
... 250-year revolution. This means that Xena is sometimes much closer to Earth than Pluto-although never closer than Neptune. Note: Xena now has the official name of “Eris”. In Greek mythology, Eris is the goddess of warfare and strife. She stirs up jealousy and envy to cause fighting and anger among m ...
pals_20160211_howpla.. - Department of Physics and Astronomy
... “Drag” from proto-planetary nebula gas? Gravitational interactions with each other? We think that Uranus & Neptune formed closer to Sun, were flung to their present orbits by interactions with Jupiter, maybe Saturn ...
... “Drag” from proto-planetary nebula gas? Gravitational interactions with each other? We think that Uranus & Neptune formed closer to Sun, were flung to their present orbits by interactions with Jupiter, maybe Saturn ...
Your Birthday on Another Planet
... By assembling and using the solar system flip book, students realize that the four planets closest to the Sun (Mercury, Venus, Earth and Mars) revolve around the Sun in the same direction, albeit at different speeds. Students use this visual information, along with a table showing the orbital period ...
... By assembling and using the solar system flip book, students realize that the four planets closest to the Sun (Mercury, Venus, Earth and Mars) revolve around the Sun in the same direction, albeit at different speeds. Students use this visual information, along with a table showing the orbital period ...
Our Solar System
... that cannot, and between problems that can be solved by technology and those that cannot with regards to solar system formation. -Estimate quantities of distances in parsec. Estimate the age of the solar system. -Describe and apply classification systems and nomenclature used in the sciences. Classi ...
... that cannot, and between problems that can be solved by technology and those that cannot with regards to solar system formation. -Estimate quantities of distances in parsec. Estimate the age of the solar system. -Describe and apply classification systems and nomenclature used in the sciences. Classi ...
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 ...
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.