SHORT ANSWER. Answer the questions, showingh your work for
... 40) Suppose a star four times more massive than our Sun has a planet the same mass as Earth, orbiting at a distance of 1 AU. a. What is the orbital period P of the planet (in years)? ...
... 40) Suppose a star four times more massive than our Sun has a planet the same mass as Earth, orbiting at a distance of 1 AU. a. What is the orbital period P of the planet (in years)? ...
earthmoonsunnotes-120923124709-phpapp02
... B. Motion of the Moon 1. The moons orbital period is 27.3 days. The time it takes to go all the way around the earth. 2. The moons rotational period is ALSO 27.3 days. This is why only one side of the moon faces the earth. (more to come) - Not because it's not rotating, because it rotates at the sa ...
... B. Motion of the Moon 1. The moons orbital period is 27.3 days. The time it takes to go all the way around the earth. 2. The moons rotational period is ALSO 27.3 days. This is why only one side of the moon faces the earth. (more to come) - Not because it's not rotating, because it rotates at the sa ...
The Solar System
... Early Thought and Models • Nicolaus Copernicus (1473-1543)- proposed the heliocentric model • Johannes Kepler (15711630)- propsed that the orbits around the sun were ellipses ...
... Early Thought and Models • Nicolaus Copernicus (1473-1543)- proposed the heliocentric model • Johannes Kepler (15711630)- propsed that the orbits around the sun were ellipses ...
Astronomy
... • research and describe the use of astronomy in ancient civilizations such as the Egyptians, Mayans, Aztecs, Europeans, and the native Americans.[4A] • research and describe the contributions of scientists to our changing understanding of astronomy, including Ptolemy, Copernicus, Tycho Brahe, Kepler ...
... • research and describe the use of astronomy in ancient civilizations such as the Egyptians, Mayans, Aztecs, Europeans, and the native Americans.[4A] • research and describe the contributions of scientists to our changing understanding of astronomy, including Ptolemy, Copernicus, Tycho Brahe, Kepler ...
Astronomy
... contains • Orbit – curved path that an object follows as it revolves around another object ...
... contains • Orbit – curved path that an object follows as it revolves around another object ...
Homework # 2 1. For each of the following, make a sketch showing
... o Belief 1: If Earth were moving, objects in the air would be left behind. Galileo used experiments to show how objects in motion will stay in motion (an early form of Newton's first law), so objects in Earth's atmosphere could conceivably continue to move with the planet o Belief 2: The heavens m ...
... o Belief 1: If Earth were moving, objects in the air would be left behind. Galileo used experiments to show how objects in motion will stay in motion (an early form of Newton's first law), so objects in Earth's atmosphere could conceivably continue to move with the planet o Belief 2: The heavens m ...
PowerPoint. - teachearthscience.org
... In small bodies such as asteroids, the gravitational pull is too weak to overcome the mechanical strength of the asteroid. As a result, these bodies do not form spheres and maintain irregular shapes. ...
... In small bodies such as asteroids, the gravitational pull is too weak to overcome the mechanical strength of the asteroid. As a result, these bodies do not form spheres and maintain irregular shapes. ...
A) greatest in diameter at the Equator B) greatest in diameter at the
... Base your answers to questions 4 and 5 on the time-exposure photograph shown below. The photograph was taken by aiming a camera at a portion of the night sky above a New York State location and leaving the camera's shutter open for a period of time to record star trails. ...
... Base your answers to questions 4 and 5 on the time-exposure photograph shown below. The photograph was taken by aiming a camera at a portion of the night sky above a New York State location and leaving the camera's shutter open for a period of time to record star trails. ...
The Celestial Sphere
... rotation with respect to the stars. A solar day is one rotation with respect to the Sun. Sidereal and solar days differ by about 4 minutes. ...
... rotation with respect to the stars. A solar day is one rotation with respect to the Sun. Sidereal and solar days differ by about 4 minutes. ...
Planet Earth – Could There be Life?
... Now that we know the Sun star is a good candidate to support life, let’s look at planet Earth’s position relative to the Sun! ...
... Now that we know the Sun star is a good candidate to support life, let’s look at planet Earth’s position relative to the Sun! ...
File
... Sky appears tilted at an angle equal to our latitude. Stars appear to move in arcs across the sky that are not perpendicular to horizon. ...
... Sky appears tilted at an angle equal to our latitude. Stars appear to move in arcs across the sky that are not perpendicular to horizon. ...
coSmoS in youR PockET
... Look outside your window tonight and try to see the Moon. Can you see it? ...
... Look outside your window tonight and try to see the Moon. Can you see it? ...
Planet Earth – Could There be Life?
... Now that we know the Sun star is a good candidate to support life, let’s look at planet Earth’s position relative to the Sun! ...
... Now that we know the Sun star is a good candidate to support life, let’s look at planet Earth’s position relative to the Sun! ...
“The Southern Cross”
... of the year was linked with certain sacrifices. Eclipses were also recorded and their causes explained. Unlike some other ancient cultures, Indian astronomy continued well into the modern era. By the first century CE, it had become more scientific, possibly as a result of coming into contact with Me ...
... of the year was linked with certain sacrifices. Eclipses were also recorded and their causes explained. Unlike some other ancient cultures, Indian astronomy continued well into the modern era. By the first century CE, it had become more scientific, possibly as a result of coming into contact with Me ...
Name - MIT
... zenith, to your horizon due south. D) The path the Sun appears to trace around the celestial sphere each year. E) An extension of the meridian out into space. 25) What is the celestial sphere? A) The celestial sphere is a model that shows the true locations of the Sun and a few thousand of the neare ...
... zenith, to your horizon due south. D) The path the Sun appears to trace around the celestial sphere each year. E) An extension of the meridian out into space. 25) What is the celestial sphere? A) The celestial sphere is a model that shows the true locations of the Sun and a few thousand of the neare ...
b 03 Other Obj in Sol System combo ppt
... Due to the elliptical nature of the orbit - Minimum distance: 363 000 km (called perigee) - Maximum distance: 405 000 km (called apogee). • Diameter: 3 500 km (1/4 that of Earth's) – However as viewed from Earth, the size of the Moon appears to change by as much as 11% from perigee and apogee. ...
... Due to the elliptical nature of the orbit - Minimum distance: 363 000 km (called perigee) - Maximum distance: 405 000 km (called apogee). • Diameter: 3 500 km (1/4 that of Earth's) – However as viewed from Earth, the size of the Moon appears to change by as much as 11% from perigee and apogee. ...
The Sun
... sun is just the right size and distance from Earth so that there can be life on our planet. There are stars that are much larger than our sun. A star in the Orion constellation called Betelgeuse is 400 times larger than our sun. If our sun was this size it would engulf Mercury, Venus, Earth and Ma ...
... sun is just the right size and distance from Earth so that there can be life on our planet. There are stars that are much larger than our sun. A star in the Orion constellation called Betelgeuse is 400 times larger than our sun. If our sun was this size it would engulf Mercury, Venus, Earth and Ma ...
33_drake
... of new civilizations is nearly equal to rate of their death. “Writes one number, that we do not know, as the product of seven numbers, that we do not ...
... of new civilizations is nearly equal to rate of their death. “Writes one number, that we do not know, as the product of seven numbers, that we do not ...
Powerpoint for today
... Make high quality observations of some natural phenomenon Come up with a theory that explains the observations Use the theory to predict future behavior Make further observations to test the theory Refine the theory, or if it no longer works, make a new one ...
... Make high quality observations of some natural phenomenon Come up with a theory that explains the observations Use the theory to predict future behavior Make further observations to test the theory Refine the theory, or if it no longer works, make a new one ...
modeling astronomy concepts with a gps receiver and
... and longitude, altitude, and speed; the direction in which you are moving; and the time anywhere on Earth, in any weather, at any time. Because a GPS receiver must track data from at least three satellites at once (4 for precise elevation), it must have a direct line of sight to the sky at any given ...
... and longitude, altitude, and speed; the direction in which you are moving; and the time anywhere on Earth, in any weather, at any time. Because a GPS receiver must track data from at least three satellites at once (4 for precise elevation), it must have a direct line of sight to the sky at any given ...
Document
... ecliptic. Therefore, the Sun and Earth both lie exactly on the plane of the ecliptic, and equivalently the Sun is seen by definition to lie exactly on the ecliptic as viewed from the Earth. The other planets of the solar system lie approximately but not exactly on the ecliptic: their orbits lie on p ...
... ecliptic. Therefore, the Sun and Earth both lie exactly on the plane of the ecliptic, and equivalently the Sun is seen by definition to lie exactly on the ecliptic as viewed from the Earth. The other planets of the solar system lie approximately but not exactly on the ecliptic: their orbits lie on p ...
The Solar System PPT
... Neptune were the first planets discovered since antiquity, and showed astronomers the solar system was bigger than previously thought. ...
... Neptune were the first planets discovered since antiquity, and showed astronomers the solar system was bigger than previously thought. ...
Document
... If on the equator, we see the whole sky once per day In between, we see part of the sky all day long and part only some of the day ...
... If on the equator, we see the whole sky once per day In between, we see part of the sky all day long and part only some of the day ...
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.