Lining Up the Planets - Math-4326
... 2. Divide the class into teams of four. 3. Explain that each team member will have a card that he or she reads to the group. Other team members are not to read each other’s cards, but they are to practice listening and then apply what they hear. 4. Have the students use the scaled planet drawings to ...
... 2. Divide the class into teams of four. 3. Explain that each team member will have a card that he or she reads to the group. Other team members are not to read each other’s cards, but they are to practice listening and then apply what they hear. 4. Have the students use the scaled planet drawings to ...
Test 2 review session
... • Get plenty of rest the night before 2) During the Test: • Draw simple sketches to help visualize problems • Solve numerical problems in the margin • Come up with your answer first, then look for it in the choices • If you can’t find the answer, try process of elimination • If you don’t know the an ...
... • Get plenty of rest the night before 2) During the Test: • Draw simple sketches to help visualize problems • Solve numerical problems in the margin • Come up with your answer first, then look for it in the choices • If you can’t find the answer, try process of elimination • If you don’t know the an ...
THE BIRTH AND DEATH OF A LOW/MEDIUM MASS STAR
... • THE STAGE WHEN A STAR IS IN IT’S “BEST” LIFE CYCLE • OUR SUN IS A MAIN SEQUENCE STAR • MAIN SEQUENCE STARS HAVE MOSTLY HYDROGEN. • THE HYDROGEN EXPLODES, GIVING OFF LIGHT AND HEAT • AS IT EXPLODES, THE HYDROGEN TURNS TO HELIUM. • HELIUM IS LIGHTER THAN HYDROGEN. • OUR SUN IS 4.6 BILLION YEARS OLD. ...
... • THE STAGE WHEN A STAR IS IN IT’S “BEST” LIFE CYCLE • OUR SUN IS A MAIN SEQUENCE STAR • MAIN SEQUENCE STARS HAVE MOSTLY HYDROGEN. • THE HYDROGEN EXPLODES, GIVING OFF LIGHT AND HEAT • AS IT EXPLODES, THE HYDROGEN TURNS TO HELIUM. • HELIUM IS LIGHTER THAN HYDROGEN. • OUR SUN IS 4.6 BILLION YEARS OLD. ...
Formation of the Solar System
... concentrated in the center of the disk, where the Sun eventually formed. The growth of the planets began as solid bits of matter began to collide and clump together through a process called accretion. The colliding matter formed small, irregularly shaped bodies called planetesimals. AS the collision ...
... concentrated in the center of the disk, where the Sun eventually formed. The growth of the planets began as solid bits of matter began to collide and clump together through a process called accretion. The colliding matter formed small, irregularly shaped bodies called planetesimals. AS the collision ...
Playground planets - Earth Learning Idea
... with minimal resources, for teacher educators and teachers of Earth science through school-level geography or science, with an online discussion around every idea in order to develop a global support network. ‘Earthlearningidea’ has little funding and is produced largely by voluntary effort. Copyrig ...
... with minimal resources, for teacher educators and teachers of Earth science through school-level geography or science, with an online discussion around every idea in order to develop a global support network. ‘Earthlearningidea’ has little funding and is produced largely by voluntary effort. Copyrig ...
New Earthlike Planet Discovered
... degrees and that set off celebrations among astronomers. Until now, all 220 planets astronomers have found outside our solar system have had the "Goldilocks problem." They've been too hot, too cold or just plain too big and gaseous, like uninhabitable Jupiter. The new planet seems just right — or at ...
... degrees and that set off celebrations among astronomers. Until now, all 220 planets astronomers have found outside our solar system have had the "Goldilocks problem." They've been too hot, too cold or just plain too big and gaseous, like uninhabitable Jupiter. The new planet seems just right — or at ...
Methods for the detection of exoplanets
... Conditions: the position and width of the HZ depends on the presence and composition of the atmosphere (greenhouse effect - GE). On EARTH: GE raises temperature by ~32 °C ...
... Conditions: the position and width of the HZ depends on the presence and composition of the atmosphere (greenhouse effect - GE). On EARTH: GE raises temperature by ~32 °C ...
Kepler`s Laws - Harnett County High Schools Wiki
... The two points are called the foci (singular focus) Each planet’s ellipse is a different shape and size, and the Sun is always at one focus The major axis is the line that runs through both foci and is the maximum diameter of the ...
... The two points are called the foci (singular focus) Each planet’s ellipse is a different shape and size, and the Sun is always at one focus The major axis is the line that runs through both foci and is the maximum diameter of the ...
UBD - Solar System
... list the planets in our solar system in order from the sun. describe the forces that keep objects in orbit in the solar system. describe the size, surface, atmosphere, orbit, and unique features of each of the 8 planets in our solar system identify dangers on other planets. ...
... list the planets in our solar system in order from the sun. describe the forces that keep objects in orbit in the solar system. describe the size, surface, atmosphere, orbit, and unique features of each of the 8 planets in our solar system identify dangers on other planets. ...
AST 301 Fall 2007 Review for Exam 3 This exam covers only
... What do you learn from this technique? What could you learn about a planet from other 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 disco ...
... What do you learn from this technique? What could you learn about a planet from other 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 disco ...
Solar System Webquest
... past the orbits or Neptune and Pluto may be all that’s left of a large number of small, icy bodies that once filled the outer solar system. Most of these bodies probably became part of the giant planets or were flung into the far fringes of the solar system by close encounters with the Jovian planet ...
... past the orbits or Neptune and Pluto may be all that’s left of a large number of small, icy bodies that once filled the outer solar system. Most of these bodies probably became part of the giant planets or were flung into the far fringes of the solar system by close encounters with the Jovian planet ...
Temperature and Formation of our Solar System
... bombarded the inner planets after they were formed. Thus, the water on Earth originated in comets. ...
... bombarded the inner planets after they were formed. Thus, the water on Earth originated in comets. ...
Planet Hunters
... exoplanet revolution has been the tremendous diversity of our neighboring systems. With only our own solar system as a model, scientists once assumed that most solar systems would consist of small rocky planets near the star and massive gas giants at greater distances, which took decades to round th ...
... exoplanet revolution has been the tremendous diversity of our neighboring systems. With only our own solar system as a model, scientists once assumed that most solar systems would consist of small rocky planets near the star and massive gas giants at greater distances, which took decades to round th ...
Melbourne Solar System Trail.pub
... 10. Pluto, discovered in 1930, is a tiny world smaller than Earth. Charon, one of its three moons, is half the size of Pluto. Beyond Neptune are thousands of asteroids of ice and rock left over from when the planets were formed called ‘Kuiper Belt’. In 2005 a Kuiper Belt Object or ‘KBO’ larger than ...
... 10. Pluto, discovered in 1930, is a tiny world smaller than Earth. Charon, one of its three moons, is half the size of Pluto. Beyond Neptune are thousands of asteroids of ice and rock left over from when the planets were formed called ‘Kuiper Belt’. In 2005 a Kuiper Belt Object or ‘KBO’ larger than ...
Viking
... How are the gas giants similar to each other? How are they different? How is Pluto different from the gas giants? What is the most prominent feature of Jupiter’s surface? What cuases this feature? Why do astrnomoers think Uranus may have been hit by another object billions of years ago? ...
... How are the gas giants similar to each other? How are they different? How is Pluto different from the gas giants? What is the most prominent feature of Jupiter’s surface? What cuases this feature? Why do astrnomoers think Uranus may have been hit by another object billions of years ago? ...
Chapter 16 - The Solar System
... Direction of pendulum swing appears to change Apparent change due to Earth’s rotation. At the North pole rotation is 90O in 6 hours Direction is constant relative to external reference ...
... Direction of pendulum swing appears to change Apparent change due to Earth’s rotation. At the North pole rotation is 90O in 6 hours Direction is constant relative to external reference ...
14. 1 A Travel Guide to the Outer Planets 14.2 Jupiter 14.3 Saturn
... Saturn's rings are composed of icy particles ranging in size from boulders to dust. In some regions the ice is purer than in other regions. Grooves and other features in the rings can be produced by resonances w ith moons or by w aves that propagate through the rings. Narrow rings and sharp ring edg ...
... Saturn's rings are composed of icy particles ranging in size from boulders to dust. In some regions the ice is purer than in other regions. Grooves and other features in the rings can be produced by resonances w ith moons or by w aves that propagate through the rings. Narrow rings and sharp ring edg ...
Lesson #5: Ch 3, Section 3, The Inner Planets
... They have great insight into the solar system and I feel that this project will allow them to dive deeper into the solar system and showcase their skills in two ways instead of a typical exam style assessment. My planning was solid for this and I plan on having a solid discussion and explanation of ...
... They have great insight into the solar system and I feel that this project will allow them to dive deeper into the solar system and showcase their skills in two ways instead of a typical exam style assessment. My planning was solid for this and I plan on having a solid discussion and explanation of ...
4. THE SOLAR SYSTEM 1.1. THE SUN - Ciencias SEK
... A planet is a spherical celestial body, which moves around a star because of gravity and have cleared their orbit of other celestial bodies, that is, there are no more elements describing its same orbit. Planets don´t have their own light. We can see them because of the sunlight. The four planets th ...
... A planet is a spherical celestial body, which moves around a star because of gravity and have cleared their orbit of other celestial bodies, that is, there are no more elements describing its same orbit. Planets don´t have their own light. We can see them because of the sunlight. The four planets th ...
Untitled - IES Bachiller Sabuco
... of the solar system. All except Mercury and Pluto are very nearly circular. The orbits of the planets are in the same plane called the ecliptic . The numerous smaller bodies that habit in the solar system are the satellites of the planets; the large number of asteroids , (small rocky bodies that orb ...
... of the solar system. All except Mercury and Pluto are very nearly circular. The orbits of the planets are in the same plane called the ecliptic . The numerous smaller bodies that habit in the solar system are the satellites of the planets; the large number of asteroids , (small rocky bodies that orb ...
Scale of the Solar System Modeling the Solar System (Size, distance
... ● Models can help us compare characteristics of planets. ● Planets have measurable properties, such as size, mass, and composition. ● An object's density cannot be determined by its size alone (larger objects are not necessarily more or less dense), but also depends on its mass. ● Things in the Sola ...
... ● Models can help us compare characteristics of planets. ● Planets have measurable properties, such as size, mass, and composition. ● An object's density cannot be determined by its size alone (larger objects are not necessarily more or less dense), but also depends on its mass. ● Things in the Sola ...
Extra-Solar Planets
... star is a possible planetary companion. It is 250 times fainter than the star itself and it located 0.73 arcsecond west. At the distance of GQ Lupi, this corresponds to a distance of roughly 100 astronomical units. The planet probably has a mass of about 2 x Jupiter. ...
... star is a possible planetary companion. It is 250 times fainter than the star itself and it located 0.73 arcsecond west. At the distance of GQ Lupi, this corresponds to a distance of roughly 100 astronomical units. The planet probably has a mass of about 2 x Jupiter. ...
Dark anomalies called on the surface of the Sun allowed early
... Pluto was recently demoted from planet to “dwarf” planet status. Which of the following reasons best explains why its classification was changed? a. Pluto does not have enough gravity to put itself into a spherical shape. Only spherical celestial bodies are now considered planets. b. Pluto actually ...
... Pluto was recently demoted from planet to “dwarf” planet status. Which of the following reasons best explains why its classification was changed? a. Pluto does not have enough gravity to put itself into a spherical shape. Only spherical celestial bodies are now considered planets. b. Pluto actually ...
Dwarf planet
A dwarf planet is a planetary-mass object that is neither a planet nor a natural satellite. That is, it is in direct orbit of the Sun, and is massive enough for its shape to be in hydrostatic equilibrium under its own gravity, but has not cleared the neighborhood around its orbit.The term dwarf planet was adopted in 2006 as part of a three-way categorization of bodies orbiting the Sun, brought about by an increase in discoveries of objects farther away from the Sun than Neptune that rivaled Pluto in size, and finally precipitated by the discovery of an even more massive object, Eris. The exclusion of dwarf planets from the roster of planets by the IAU has been both praised and criticized; it was said to be the ""right decision"" by astronomer Mike Brown, who discovered Eris and other new dwarf planets, but has been rejected by Alan Stern, who had coined the term dwarf planet in 1990.The International Astronomical Union (IAU) currently recognizes five dwarf planets: Ceres, Pluto, Haumea, Makemake, and Eris. Brown criticizes this official recognition: ""A reasonable person might think that this means that there are five known objects in the solar system which fit the IAU definition of dwarf planet, but this reasonable person would be nowhere close to correct.""It is suspected that another hundred or so known objects in the Solar System are dwarf planets. Estimates are that up to 200 dwarf planets may be found when the entire region known as the Kuiper belt is explored, and that the number may exceed 10,000 when objects scattered outside the Kuiper belt are considered. Individual astronomers recognize several of these, and in August 2011 Mike Brown published a list of 390 candidate objects, ranging from ""nearly certain"" to ""possible"" dwarf planets. Brown currently identifies eleven known objects – the five accepted by the IAU plus 2007 OR10, Quaoar, Sedna, Orcus, 2002 MS4 and Salacia – as ""virtually certain"", with another dozen highly likely. Stern states that there are more than a dozen known dwarf planets.However, only two of these bodies, Ceres and Pluto, have been observed in enough detail to demonstrate that they actually fit the IAU's definition. The IAU accepted Eris as a dwarf planet because it is more massive than Pluto. They subsequently decided that unnamed trans-Neptunian objects with an absolute magnitude brighter than +1 (and hence a diameter of ≥838 km assuming a geometric albedo of ≤1) are to be named under the assumption that they are dwarf planets. The only two such objects known at the time, Makemake and Haumea, went through this naming procedure and were declared to be dwarf planets. The question of whether other likely objects are dwarf planets has never been addressed by the IAU. The classification of bodies in other planetary systems with the characteristics of dwarf planets has not been addressed.