
Venus
... Named after the Roman goddess of love and beauty, Venus. (Aphrodite in Greek) Venus is a terrestrial planet, basically it's known as Earth's "sister planet" because of the similiar size, mass, and density. It's atmosphere is 96% carbon dioxide. It is the 2nd brightest object in the night sky with a ...
... Named after the Roman goddess of love and beauty, Venus. (Aphrodite in Greek) Venus is a terrestrial planet, basically it's known as Earth's "sister planet" because of the similiar size, mass, and density. It's atmosphere is 96% carbon dioxide. It is the 2nd brightest object in the night sky with a ...
here in Powerpoint format
... Sunday = Sun Day Monday = Moon Day Tuesday = Mars (Twis) Day Wednesday = Mercury (Woden) Day Thursday = Jupiter (Thor) Day Friday = Venus (Frige) Day Saturday = Saturn Day ...
... Sunday = Sun Day Monday = Moon Day Tuesday = Mars (Twis) Day Wednesday = Mercury (Woden) Day Thursday = Jupiter (Thor) Day Friday = Venus (Frige) Day Saturday = Saturn Day ...
Astronomy Exam - domenicoscience
... What causes phases of the moon? (A drawing is required as well as a written response.) If I am a “Gemini”, what does that mean? Why is it no longer accurate? Explain the process of a super nova. How is the “red shift” used in astronomy? The big bang has some supporting evidence. Explain it here. Wha ...
... What causes phases of the moon? (A drawing is required as well as a written response.) If I am a “Gemini”, what does that mean? Why is it no longer accurate? Explain the process of a super nova. How is the “red shift” used in astronomy? The big bang has some supporting evidence. Explain it here. Wha ...
July - Westchester Amateur Astronomers
... their planets are freshly formed, and thus warmer and brighter than older planetary bodies. Astronomers know of more than five hundred distant planets, but very few have actually been seen. Many exoplanets are detected indirectly by means of their “wobbles”—the gravitational tugs they exert on their ...
... their planets are freshly formed, and thus warmer and brighter than older planetary bodies. Astronomers know of more than five hundred distant planets, but very few have actually been seen. Many exoplanets are detected indirectly by means of their “wobbles”—the gravitational tugs they exert on their ...
TOF Bible society 7.indd
... Try to do this fairly quickly, and leave time at the end to look at the final few slides and enjoy the immensity of it all. Show PowerPoint slide 1 and explain: We’ve already been hearing during this service about God who made the universe. It’s incredibly beautiful, and it’s incredibly big. Have yo ...
... Try to do this fairly quickly, and leave time at the end to look at the final few slides and enjoy the immensity of it all. Show PowerPoint slide 1 and explain: We’ve already been hearing during this service about God who made the universe. It’s incredibly beautiful, and it’s incredibly big. Have yo ...
Planetary Taxonomy
... i t t geophysics-based h i b d ttaxonomy, th the answer iis YES. Planetary status is determined by intrinsic properties (“roundness”). It is context-independent and the Earth remains a planet whether it is moved to 5, 100, or 2000 AU. The iinevitable Th it bl consequence off a geophysics-based h i b ...
... i t t geophysics-based h i b d ttaxonomy, th the answer iis YES. Planetary status is determined by intrinsic properties (“roundness”). It is context-independent and the Earth remains a planet whether it is moved to 5, 100, or 2000 AU. The iinevitable Th it bl consequence off a geophysics-based h i b ...
Space Science Distance Definitions
... means of measuring the luminosity of a star should find the same value. However, apparent brightness is not an intrinsic property of the star; it depends on your location. • Why do light sources appear fainter as a function of distance? The reason is that as light travels towards you, it is spreadin ...
... means of measuring the luminosity of a star should find the same value. However, apparent brightness is not an intrinsic property of the star; it depends on your location. • Why do light sources appear fainter as a function of distance? The reason is that as light travels towards you, it is spreadin ...
FREE Sample Here
... For what appears to be an easy concept, many students find it remarkably difficult to understand the phases of the Moon. You may want to do an in-class demonstration of phases by darkening the room, using a lamp to represent the Sun, and giving each student a Styrofoam ball to represent the Moon. If ...
... For what appears to be an easy concept, many students find it remarkably difficult to understand the phases of the Moon. You may want to do an in-class demonstration of phases by darkening the room, using a lamp to represent the Sun, and giving each student a Styrofoam ball to represent the Moon. If ...
From last time Gravitational force Equal accelerations A fortunate
... distance b of 17 light hours (120 A.U. or close to three times the distance to Pluto) at speed v=5000 km/s, period 15 years. • From the orbit we can derive the mass. • The mass is 2.6 million solar masses. • It is mostly likely a black hole at the center of ...
... distance b of 17 light hours (120 A.U. or close to three times the distance to Pluto) at speed v=5000 km/s, period 15 years. • From the orbit we can derive the mass. • The mass is 2.6 million solar masses. • It is mostly likely a black hole at the center of ...
Low-budget satellite tracking system for highly elliptical orbits
... applied to “scan” any orbit, as long as it is circular and parallel to the equatorial plane (as for example used for the aiming of astronomical instruments). Such imaginary circles can also be drawn simply by connecting all apogees of an elliptical orbit, as they are shifting over time. Knowing in a ...
... applied to “scan” any orbit, as long as it is circular and parallel to the equatorial plane (as for example used for the aiming of astronomical instruments). Such imaginary circles can also be drawn simply by connecting all apogees of an elliptical orbit, as they are shifting over time. Knowing in a ...
Wadhurst Astronomical Society Newsletter May 2017
... There are many different ways of observing the Moon. Occultation observing is something the Society has done as a group. This is where a star is accurately timed at the instant the dark side of the Moon passes in front of it. Also, in a waning Moon, the instant the star reappears is recorded, altho ...
... There are many different ways of observing the Moon. Occultation observing is something the Society has done as a group. This is where a star is accurately timed at the instant the dark side of the Moon passes in front of it. Also, in a waning Moon, the instant the star reappears is recorded, altho ...
Astronomy
... Play first aid game: one scout pulls a condition out of a jar and can either choose to describe the condition or how to treat it. A second scout must describe the opposite (if the first scout describes the condition, the second scout must describe how to treat, or visa versa). If the second scout ...
... Play first aid game: one scout pulls a condition out of a jar and can either choose to describe the condition or how to treat it. A second scout must describe the opposite (if the first scout describes the condition, the second scout must describe how to treat, or visa versa). If the second scout ...
Astronomy - Dallas ISD
... In our solar system, some planets are composed mostly of gas and liquid, and some planets are composed mostly of solid rock. Which statement about these two kinds of planets is ...
... In our solar system, some planets are composed mostly of gas and liquid, and some planets are composed mostly of solid rock. Which statement about these two kinds of planets is ...
Eclipse Unit Brief Lesson Description: This lesson serves as a pre
... Learning about models - the what, how, and why: Brief presentation on what scientific models are, how they are used in the scientific world and how they can be used in the classroom, and why they are important to communicating and furthering scientific understanding. Information will be acquired mai ...
... Learning about models - the what, how, and why: Brief presentation on what scientific models are, how they are used in the scientific world and how they can be used in the classroom, and why they are important to communicating and furthering scientific understanding. Information will be acquired mai ...
Jan 2011 Regents
... **W and Y are high tides because it is the moon’s gravitational pull that causes tidal changes. X and Y will experience low tides until those locations rotate into the appropriate positions.(approx 6 hours later)** ...
... **W and Y are high tides because it is the moon’s gravitational pull that causes tidal changes. X and Y will experience low tides until those locations rotate into the appropriate positions.(approx 6 hours later)** ...
The Solar System - Junta de Andalucía
... The Earth revolves around the Sun in orbit, at the same time that it rotates on its axis. It takes one year and six hours for the Earth to complete its orbit around the Sun. As a result, every four years we have an extra day in February. This year is called a leap year. The Earth’s revolution causes ...
... The Earth revolves around the Sun in orbit, at the same time that it rotates on its axis. It takes one year and six hours for the Earth to complete its orbit around the Sun. As a result, every four years we have an extra day in February. This year is called a leap year. The Earth’s revolution causes ...
Measuring the Masses of Galaxies in the Sloan Digital Sky Survey
... the redshift is measured from the observed positions of atomic lines in the spectra of galaxies and quasars for example, the red line of hydrogen (Hα) has a wavelength of 6.563 × 10-5 cm, 6563 Ångstroms, 656.3 nm suppose it were observed at 6603 Ångstroms (1 + z) = 6603 / 6563 = 1.0061 all other li ...
... the redshift is measured from the observed positions of atomic lines in the spectra of galaxies and quasars for example, the red line of hydrogen (Hα) has a wavelength of 6.563 × 10-5 cm, 6563 Ångstroms, 656.3 nm suppose it were observed at 6603 Ångstroms (1 + z) = 6603 / 6563 = 1.0061 all other li ...
ppt
... The space station is falling… …similar to Newton’s apple • In its circular orbit, once around the Earth every 90 minutes, it is continuously accelerating toward the Earth at ~8.8 m/s2. • Everything inside it is also falling (accelerating toward Earth at that same rate). • The astronauts are freely ...
... The space station is falling… …similar to Newton’s apple • In its circular orbit, once around the Earth every 90 minutes, it is continuously accelerating toward the Earth at ~8.8 m/s2. • Everything inside it is also falling (accelerating toward Earth at that same rate). • The astronauts are freely ...
Astrophysics 2012_2013 Grade 10 April 29, 2013
... 1. What is the correct order of the 8 planets from the Sun? 2. Which planet used to be named "Georgium Sidus" after King George III? 3. Which two planets have retrograde rotation (backwards/clockwise)? 4. Which two planets do not have any moons? 5. Which massive planet is a "brown dwarf" or "failed ...
... 1. What is the correct order of the 8 planets from the Sun? 2. Which planet used to be named "Georgium Sidus" after King George III? 3. Which two planets have retrograde rotation (backwards/clockwise)? 4. Which two planets do not have any moons? 5. Which massive planet is a "brown dwarf" or "failed ...
Astronomy Glossary Key
... The asteroid belt is chunks of rock and metal between Mars and Jupiter. It may have been a planet that was destroyed or it may not have accreted into a planet because of the strong gravitational pull of Jupiter. One AU is the average distance between the Earth and the sun. The AU is used to measure ...
... The asteroid belt is chunks of rock and metal between Mars and Jupiter. It may have been a planet that was destroyed or it may not have accreted into a planet because of the strong gravitational pull of Jupiter. One AU is the average distance between the Earth and the sun. The AU is used to measure ...
TIĀN DÌ
... time and this played a major role in influencing the course of Aristotle's life. After being a student, Aristotle soon became a teacher at the Academy and he remained there for 20 years. All Aristotle's writings of this time strongly supported Plato’s views and those of the ...
... time and this played a major role in influencing the course of Aristotle's life. After being a student, Aristotle soon became a teacher at the Academy and he remained there for 20 years. All Aristotle's writings of this time strongly supported Plato’s views and those of the ...
Section 2 Movements of the Earth
... • What is the purpose of the International Date Line? • It is a time zone border, the calendar moves ahead one day as you cross it. The purpose of the International Date Line is to locate the border so that the transition would affect the least number of people. So that it will affect the least numb ...
... • What is the purpose of the International Date Line? • It is a time zone border, the calendar moves ahead one day as you cross it. The purpose of the International Date Line is to locate the border so that the transition would affect the least number of people. So that it will affect the least numb ...
planet
... What is a planet? • Complicated definition - “A celestial body orbiting a star 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 neighboring region of planetesimals.” • Simpler definition - A “large” ...
... What is a planet? • Complicated definition - “A celestial body orbiting a star 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 neighboring region of planetesimals.” • Simpler definition - A “large” ...
Aliens
... In space, no atmosphere to limit sensitivity, only limits are from instruments. The probability of an Earthlike planet at 1 AU transiting its star is 0.47%, or about 1 in 210 - assuming it had one. If 100% of stars observed had Earthlike terrestrial planets, Kepler would find about 480 of them. The ...
... In space, no atmosphere to limit sensitivity, only limits are from instruments. The probability of an Earthlike planet at 1 AU transiting its star is 0.47%, or about 1 in 210 - assuming it had one. If 100% of stars observed had Earthlike terrestrial planets, Kepler would find about 480 of them. The ...
6TH GRADE ACCURATE PLANET SIZES AND DISTANCE FROM
... stand for Pluto). The first four planets; Mercury, Venus, Earth, and Mars, are the terrestrial planets. These planets are made of rock and are close to the Sun, relatively small, and similarly sized. The next four planets; Jupiter, Saturn, Uranus, and Neptune, are the gas planets. These planets are ...
... stand for Pluto). The first four planets; Mercury, Venus, Earth, and Mars, are the terrestrial planets. These planets are made of rock and are close to the Sun, relatively small, and similarly sized. The next four planets; Jupiter, Saturn, Uranus, and Neptune, are the gas planets. These planets are ...
Geocentric model

In astronomy, the geocentric model (also known as geocentrism, or the Ptolemaic system) is a description of the cosmos where Earth is at the orbital center of all celestial bodies. This model served as the predominant cosmological system in many ancient civilizations such as ancient Greece including the noteworthy systems of Aristotle (see Aristotelian physics) and Ptolemy. As such, they believed that the Sun, Moon, stars, and naked eye planets circled Earth.Two commonly made observations supported the idea that Earth was the center of the Universe. The stars, the sun, and planets appear to revolve around Earth each day, making Earth the center of that system. The stars were thought to be on a celestial sphere, with the earth at its center, that rotated each day, using a line through the north and south pole as an axis. The stars closest to the equator appeared to rise and fall the greatest distance, but each star circled back to its rising point each day. The second observation supporting the geocentric model was that the Earth does not seem to move from the perspective of an Earth-bound observer, and that it is solid, stable, and unmoving.Ancient Roman and medieval philosophers usually combined the geocentric model with a spherical Earth. It is not the same as the older flat Earth model implied in some mythology, as was the case with the biblical and postbiblical Latin cosmology. The ancient Jewish Babylonian uranography pictured a flat Earth with a dome-shaped rigid canopy named firmament placed over it. (רקיע- rāqîa').However, the ancient Greeks believed that the motions of the planets were circular and not elliptical, a view that was not challenged in Western culture until the 17th century through the synthesis of theories by Copernicus and Kepler.The astronomical predictions of Ptolemy's geocentric model were used to prepare astrological and astronomical charts for over 1500 years. The geocentric model held sway into the early modern age, but from the late 16th century onward was gradually superseded by the heliocentric model of Copernicus, Galileo and Kepler. There was much resistance to the transition between these two theories. Christian theologians were reluctant to reject a theory that agreed with Bible passages (e.g. ""Sun, stand you still upon Gibeon"", Joshua 10:12 – King James 2000 Bible). Others felt a new, unknown theory could not subvert an accepted consensus for geocentrism.