Ch. 20 Classifying Objects in the Solar System
... Directions: Label the name of each object or set of objects within the solar system on the lines provided in the diagram above. Then answer the questions below. 1. The Sun is considered a star because it is the only object in our solar system hot enough to undergo the process of ______________ _____ ...
... Directions: Label the name of each object or set of objects within the solar system on the lines provided in the diagram above. Then answer the questions below. 1. The Sun is considered a star because it is the only object in our solar system hot enough to undergo the process of ______________ _____ ...
Search for Life in the Universe
... – Semi-major axis: minimum:median:maximum = 0.02:1.0:5.9 AU – Solar system: Mercury:Earth:Jupiter = 0.4:1.0:5.2 AU ...
... – Semi-major axis: minimum:median:maximum = 0.02:1.0:5.9 AU – Solar system: Mercury:Earth:Jupiter = 0.4:1.0:5.2 AU ...
File - Mr. Dudek`s Science
... stars consist of two spheres; one that was consistently spun around the Earth and one that seemed to wander (planet translates to “wandering star”) ...
... stars consist of two spheres; one that was consistently spun around the Earth and one that seemed to wander (planet translates to “wandering star”) ...
Presentación de PowerPoint
... more matter than all the other planets put together, and its volume is one thousand times the volume of Earth. It has many satellites, and four of them (Io, Callisto, Europa and Ganymede) were discovered by Galilei in 1610. Its thick atmosphere is complex, and it is made up of hydrogen (90%) and hel ...
... more matter than all the other planets put together, and its volume is one thousand times the volume of Earth. It has many satellites, and four of them (Io, Callisto, Europa and Ganymede) were discovered by Galilei in 1610. Its thick atmosphere is complex, and it is made up of hydrogen (90%) and hel ...
Fig. 16-7, p.363
... from a disk around the Sun as it formed; such protoplanetary disks are seen around many young stars • Planets like Earth are believed therefore to form as normal byproducts of stars forming • There are two types of planets in our solar system, Earth-like and Jupiter-like, results of a process we thi ...
... from a disk around the Sun as it formed; such protoplanetary disks are seen around many young stars • Planets like Earth are believed therefore to form as normal byproducts of stars forming • There are two types of planets in our solar system, Earth-like and Jupiter-like, results of a process we thi ...
Lesson 3 The Solar System
... • Beyond the asteroid belt is another group of planets that includes Jupiter, Saturn, Uranus, and Neptune, known as the outer planets. • They are gas giants which are huge planets with a small, metallic core, and a thick atmosphere. • The gas giants all have rings and many moons. • They spin very ra ...
... • Beyond the asteroid belt is another group of planets that includes Jupiter, Saturn, Uranus, and Neptune, known as the outer planets. • They are gas giants which are huge planets with a small, metallic core, and a thick atmosphere. • The gas giants all have rings and many moons. • They spin very ra ...
Lesson 3 The Solar System - Delaware Valley School District
... asteroids, rocky or metallic objects, that orbit the Sun. • Most asteroids are located in the asteroid belt. • The largest object is about one fourth the diameter of the Moon. • Asteroids orbit the Sun just like planets. • Some asteroids travel as far from the Sun as Saturn’s orbit, other asteroids ...
... asteroids, rocky or metallic objects, that orbit the Sun. • Most asteroids are located in the asteroid belt. • The largest object is about one fourth the diameter of the Moon. • Asteroids orbit the Sun just like planets. • Some asteroids travel as far from the Sun as Saturn’s orbit, other asteroids ...
Outer Space - The Reading Connection
... constellation is outlined in glitter, shining like it's made of stars. Kids in Orbit ...
... constellation is outlined in glitter, shining like it's made of stars. Kids in Orbit ...
The Solar System
... • It has two thick and two thin rings around it. • One day on Neptune lasts about 18 Earth hours. • It takes 165 years to orbit the Sun. www.worldalmanacforkids.com/WAKIViewArticle ...
... • It has two thick and two thin rings around it. • One day on Neptune lasts about 18 Earth hours. • It takes 165 years to orbit the Sun. www.worldalmanacforkids.com/WAKIViewArticle ...
Spring `03 final exam study guide
... spectroscope asteroid escape velocity ion stellar wind asteroid belt Kuiper belt meteor meteoroid meteorite sunspot luminosity pressure hydrostatic equilibrium conduction convection radiation apparent magnitude main sequence parsec absolute magnitude white dwarf+ electron degeneracy+ Hertzsprung-Rus ...
... spectroscope asteroid escape velocity ion stellar wind asteroid belt Kuiper belt meteor meteoroid meteorite sunspot luminosity pressure hydrostatic equilibrium conduction convection radiation apparent magnitude main sequence parsec absolute magnitude white dwarf+ electron degeneracy+ Hertzsprung-Rus ...
AST 301 Fall 2007 Review for Exam 3 This exam covers only
... techniques? Of the numerous extrasolar planets that have been discovered, what are some of the surprising results? They are all massive (e.g. like Jupiter or larger)—was this a surprise? Explain. Why do these discoveries point to the importance of the protostellar ...
... techniques? Of the numerous extrasolar planets that have been discovered, what are some of the surprising results? They are all massive (e.g. like Jupiter or larger)—was this a surprise? Explain. Why do these discoveries point to the importance of the protostellar ...
Planet formation
... The core accretion model states that planets form from the build-up of dust into larger and larger bodies. But planet formation is not simple. Interactions with the disc can cause the migration of massive planets, and multiple massive planets can interact in complex ways. Planetary systems can also ...
... The core accretion model states that planets form from the build-up of dust into larger and larger bodies. But planet formation is not simple. Interactions with the disc can cause the migration of massive planets, and multiple massive planets can interact in complex ways. Planetary systems can also ...
PowerPoint
... Formation of OUR Solar System? • Looks like a supernova explosion nearby may have done the job… Probably a type II high-mass star supernova, from the relative abundances of elements in meteorites. • Blast wave compresses interstellar cloud, and the debris of that explosion is contained in the first ...
... Formation of OUR Solar System? • Looks like a supernova explosion nearby may have done the job… Probably a type II high-mass star supernova, from the relative abundances of elements in meteorites. • Blast wave compresses interstellar cloud, and the debris of that explosion is contained in the first ...
Methods Of Discovering Extra solar Planets.
... Method 3: Radial Velocity! • Radial Velocity is one of the motions of the star does known as stellar motion. • Radial Velocity is use in redshift. As it will be altered slightly when a planet goes by. • To use radial velocity astronomers look for an altercation in the movement of the star, Possibly ...
... Method 3: Radial Velocity! • Radial Velocity is one of the motions of the star does known as stellar motion. • Radial Velocity is use in redshift. As it will be altered slightly when a planet goes by. • To use radial velocity astronomers look for an altercation in the movement of the star, Possibly ...
Chapter 8 Powerpoint
... Understanding the Solar System • By definition, there are eight planets which consist of four terrestrial planets which are closer to the Sun and four gaseous giant planets which are further away. The terrestrial and gas planets are separated by a belt of rocky debris known as the ...
... Understanding the Solar System • By definition, there are eight planets which consist of four terrestrial planets which are closer to the Sun and four gaseous giant planets which are further away. The terrestrial and gas planets are separated by a belt of rocky debris known as the ...
Hunting for Extrasolar Planets: Methods and Results
... because 1. It does not require a large telescope! 2. Chances of finding a planet-star system nearly edge-on is small, so need lots of observations; 3. Big payoff: you can learn about a stars diameter and mass, and so get density. Also: can observe planet’s spectrum! ...
... because 1. It does not require a large telescope! 2. Chances of finding a planet-star system nearly edge-on is small, so need lots of observations; 3. Big payoff: you can learn about a stars diameter and mass, and so get density. Also: can observe planet’s spectrum! ...
Document
... The rocky inner planets (Mercury, Venus, Earth and Mars) are called the terrestrial planets. The gaseous outer planets (Jupiter, Saturn, Uranus and Neptune) are the Jovian planets. An asteroid belt lies between the inner and outer planets. The outermost icy planet, Pluto, is in a class called Trans- ...
... The rocky inner planets (Mercury, Venus, Earth and Mars) are called the terrestrial planets. The gaseous outer planets (Jupiter, Saturn, Uranus and Neptune) are the Jovian planets. An asteroid belt lies between the inner and outer planets. The outermost icy planet, Pluto, is in a class called Trans- ...
tata-surya
... How did the Solar System form? Any theory of the solar system formation must account for the obvious features we see, such as 1) the fact that solar system is a fairly flat place, with all the planets within a few degrees of the ecliptic and revolving in roughly circular oribts that are all goin ...
... How did the Solar System form? Any theory of the solar system formation must account for the obvious features we see, such as 1) the fact that solar system is a fairly flat place, with all the planets within a few degrees of the ecliptic and revolving in roughly circular oribts that are all goin ...
Gemini South telescope makes the case for multiple Earth
... companions to the primary “host” star, to within a distance that is less than that of Mercury from our Sun. Faint “M-class” stars such as TRAPPIST-1 are of great interest to astronomers: their diminutive size allows easier detection of small, terrestrial planets. In the TRAPPIST-1 system, two of the ...
... companions to the primary “host” star, to within a distance that is less than that of Mercury from our Sun. Faint “M-class” stars such as TRAPPIST-1 are of great interest to astronomers: their diminutive size allows easier detection of small, terrestrial planets. In the TRAPPIST-1 system, two of the ...
Lecture7
... • B) Condensation of gas from the original star nebula • C) Capture by the star of objects traversing the depths of space • D) Accretion or slow accumulation of smaller particles by mutual gravitational attraction ...
... • B) Condensation of gas from the original star nebula • C) Capture by the star of objects traversing the depths of space • D) Accretion or slow accumulation of smaller particles by mutual gravitational attraction ...
Word doc - UC-HiPACC - University of California, Santa Cruz
... of data due to stellar surface activity and/or instrumental errors. Tuomi also developed methods for analyzing the long-term pattern of a star’s barycentric motion to calculate number of possible planets, ...
... of data due to stellar surface activity and/or instrumental errors. Tuomi also developed methods for analyzing the long-term pattern of a star’s barycentric motion to calculate number of possible planets, ...
Space - PAMS-Doyle
... very large, and the four inner planets are comparatively small and rocky. On one end write the sun and the other Pluto. Fold your paper in half, at the crease write Uranus. Fold Pluto up to Uranus, at the crease write Neptune. Fold the sun to Uranus, at the crease write Saturn. Fold the sun to Satur ...
... very large, and the four inner planets are comparatively small and rocky. On one end write the sun and the other Pluto. Fold your paper in half, at the crease write Uranus. Fold Pluto up to Uranus, at the crease write Neptune. Fold the sun to Uranus, at the crease write Saturn. Fold the sun to Satur ...
Lecture 36: Strange New Worlds
... Orbital Periods < 10 days Inside the orbit of Mercury Densities like Jupiter and Saturn, so they are gas giants. Selection effect? How does a Jupiter-size gas planet get so close to its parent star? ...
... Orbital Periods < 10 days Inside the orbit of Mercury Densities like Jupiter and Saturn, so they are gas giants. Selection effect? How does a Jupiter-size gas planet get so close to its parent star? ...
Day 9 - Ch. 4 -
... - stellar winds (happening with our sun now) - planetary nebulae (not planets, but similar appearance to early astronomers) - see slides - nova and supernova explosions ...
... - stellar winds (happening with our sun now) - planetary nebulae (not planets, but similar appearance to early astronomers) - see slides - nova and supernova explosions ...
tata - surya
... How did the Solar System form? Any theory of the solar system formation must account for the obvious features we see, such as 1) the fact that solar system is a fairly flat place, with all the planets within a few degrees of the ecliptic and revolving in roughly circular oribts that are all goin ...
... How did the Solar System form? Any theory of the solar system formation must account for the obvious features we see, such as 1) the fact that solar system is a fairly flat place, with all the planets within a few degrees of the ecliptic and revolving in roughly circular oribts that are all goin ...
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.