Name
... Locate Mercury and try it. Was it any different from your prediction? ______________________ How often does Mercury do this? __________________ Is it different from Saturn? Display the zodiacal constellations. The reason for this loopy behavior is more apparent if you show the sun as well as Mercury ...
... Locate Mercury and try it. Was it any different from your prediction? ______________________ How often does Mercury do this? __________________ Is it different from Saturn? Display the zodiacal constellations. The reason for this loopy behavior is more apparent if you show the sun as well as Mercury ...
The Seasons (PowerPoint)
... ON ANY GIVEN DAY, the Sun is just like any other star, except that it is extraordinarily bright. It lights up the whole sky. During our Winter, it acts like a Southern star, and follows a relatively low daily ‘arc’ across the southern skies. During our Summer, it is a Northern star, and climbs much ...
... ON ANY GIVEN DAY, the Sun is just like any other star, except that it is extraordinarily bright. It lights up the whole sky. During our Winter, it acts like a Southern star, and follows a relatively low daily ‘arc’ across the southern skies. During our Summer, it is a Northern star, and climbs much ...
Unit I – The Seasons
... ON ANY GIVEN DAY, the Sun is just like any other star, except that it is extraordinarily bright. It lights up the whole sky. During our Winter, it acts like a Southern star, and follows a relatively low daily ‘arc’ across the southern skies. During our Summer, it is a Northern star, and climbs much ...
... ON ANY GIVEN DAY, the Sun is just like any other star, except that it is extraordinarily bright. It lights up the whole sky. During our Winter, it acts like a Southern star, and follows a relatively low daily ‘arc’ across the southern skies. During our Summer, it is a Northern star, and climbs much ...
Astronomy 101 Exam 2 Form A Name: SUID: Lab section number:
... exerts on Jupiter. However, since the Sun is at the center of the Solar System,it does not move at all. (B) Jupiter exerts no gravitational force at all on the Sun; thus the Sun does not move. (C) The force of gravity that Jupiter exerts on the Sun is equal to the force of gravity thatthe Sun exerts ...
... exerts on Jupiter. However, since the Sun is at the center of the Solar System,it does not move at all. (B) Jupiter exerts no gravitational force at all on the Sun; thus the Sun does not move. (C) The force of gravity that Jupiter exerts on the Sun is equal to the force of gravity thatthe Sun exerts ...
What causes eclipses?
... parallax could mean one of two things: 1. Stars are so far away that stellar parallax is too small to notice with the naked eye. 2. Earth does not orbit the Sun; it is the center of the universe. With rare exceptions such as Aristarchus, the Greeks rejected the correct explanation (1) because they ...
... parallax could mean one of two things: 1. Stars are so far away that stellar parallax is too small to notice with the naked eye. 2. Earth does not orbit the Sun; it is the center of the universe. With rare exceptions such as Aristarchus, the Greeks rejected the correct explanation (1) because they ...
UCCS Solar Energy ENSC/PES 1600 Fall 2010 Earth, Sun, Time
... C) standard time D) daylight saving time E) sidereal time 16) All the following statements are true. Which one explains why mean solar time differs from apparent solar time? A) The length of a solar day is not always exactly 24 hours. B) Earth's rotation period is actually about 23 hours 56 minutes, ...
... C) standard time D) daylight saving time E) sidereal time 16) All the following statements are true. Which one explains why mean solar time differs from apparent solar time? A) The length of a solar day is not always exactly 24 hours. B) Earth's rotation period is actually about 23 hours 56 minutes, ...
SCI 103
... 18) Kepler’s first two Laws of Planetary Motion contradicted the Aristotelian/Ptolemaic Model of the Universe in two fundamental ways. What are Kepler’s first two Laws of Planetary Motion and how were they anti-Aristotelian? Kepler’s 1ST law states that planets orbit, not on circles, but on ellipse ...
... 18) Kepler’s first two Laws of Planetary Motion contradicted the Aristotelian/Ptolemaic Model of the Universe in two fundamental ways. What are Kepler’s first two Laws of Planetary Motion and how were they anti-Aristotelian? Kepler’s 1ST law states that planets orbit, not on circles, but on ellipse ...
Opposition of Jupiter - Hong Kong Observatory
... will be very bright, reaching a visual magnitude of about 2.5*. This will be a good time to observe Jupiter, its Great Red Spot and Jupiter's four largest satellites namely Io, Europa, Ganymede and Callisto. A telescope with a magnification of 40 times or above is preferred in observing Jupiter. ...
... will be very bright, reaching a visual magnitude of about 2.5*. This will be a good time to observe Jupiter, its Great Red Spot and Jupiter's four largest satellites namely Io, Europa, Ganymede and Callisto. A telescope with a magnification of 40 times or above is preferred in observing Jupiter. ...
Ch. 22 Honors Study Guide Name 1. How did Eratosthenes
... 7. Even though Copernicus was right about the Heliocentric model, the planets did not line up where he thought they should. What was wrong with Copernicus’ model? 8. Why were Tycho Brahe’s observations so important in Astronomy? 9. Why didn’t Tycho Brahe believe the Sun was the center of the Solar S ...
... 7. Even though Copernicus was right about the Heliocentric model, the planets did not line up where he thought they should. What was wrong with Copernicus’ model? 8. Why were Tycho Brahe’s observations so important in Astronomy? 9. Why didn’t Tycho Brahe believe the Sun was the center of the Solar S ...
Chapter 27 Stars and Galaxies
... Apparent Magnitude The measurement of brightness is assigned a number on a scale – Brightest stars have lowest numbers – Dimmest stars have highest numbers ...
... Apparent Magnitude The measurement of brightness is assigned a number on a scale – Brightest stars have lowest numbers – Dimmest stars have highest numbers ...
How to use custom background????
... – Daily/Diurnal: like Sun, stars rise in east, set in west • Ancients believed this due to rotation of C.S. • from Earth rotating underneath C.S. • To them, the Earth does not appear to move, so easier to believe Earth is stationary ...
... – Daily/Diurnal: like Sun, stars rise in east, set in west • Ancients believed this due to rotation of C.S. • from Earth rotating underneath C.S. • To them, the Earth does not appear to move, so easier to believe Earth is stationary ...
SOL Review - Mr. Gautier`s Biology/Earth Science
... 2. If an area is very karst, it probably has a lot of what? 3. If the water table goes up, what zone gets bigger? 4. Most fossils are found in this type of rock? 5. According to the Law of Superposition, the oldest rock is where? 6. Cold water rising to the surface is an example of what? 7. Ocean Cu ...
... 2. If an area is very karst, it probably has a lot of what? 3. If the water table goes up, what zone gets bigger? 4. Most fossils are found in this type of rock? 5. According to the Law of Superposition, the oldest rock is where? 6. Cold water rising to the surface is an example of what? 7. Ocean Cu ...
Space - Great Barr Academy
... It looks huge, but the The Sun coldest is a veryit small reaches on Venus isto star in comparison 360°C! That is hotter the others. than your oven!! ...
... It looks huge, but the The Sun coldest is a veryit small reaches on Venus isto star in comparison 360°C! That is hotter the others. than your oven!! ...
Unit XII Study Guide
... a. Hydrogen will increase and helium will decrease. b. Hydrogen will decrease and helium will increase. c. Both hydrogen and helium will decrease. d. Both hydrogen and helium will remain the same. ____ 15. The sun remains stable over time because a. Its supply of hydrogen is inexhaustible. b. the pr ...
... a. Hydrogen will increase and helium will decrease. b. Hydrogen will decrease and helium will increase. c. Both hydrogen and helium will decrease. d. Both hydrogen and helium will remain the same. ____ 15. The sun remains stable over time because a. Its supply of hydrogen is inexhaustible. b. the pr ...
The Sun and Planets Homework Solution 1.
... So, while Neptune is located about 3.5 meters away from the center of our model, your Proxima Centauri handball must be placed 31’400 km away! The Earth only ...
... So, while Neptune is located about 3.5 meters away from the center of our model, your Proxima Centauri handball must be placed 31’400 km away! The Earth only ...
AN INTRODUCTION TO ASTRONOMY Dr. Uri Griv Department of Physics, Ben-Gurion University
... to planet Uranus, imaged here in near-infrared light by the Antu telescope at the ESO Paranal Observatory in Chile. Since gas giant Uranus’ methane-laced atmosphere absorbs sunlight at near-infrared wavelengths the planet appears substantially darkened, improving the contrast between the otherwise r ...
... to planet Uranus, imaged here in near-infrared light by the Antu telescope at the ESO Paranal Observatory in Chile. Since gas giant Uranus’ methane-laced atmosphere absorbs sunlight at near-infrared wavelengths the planet appears substantially darkened, improving the contrast between the otherwise r ...
Chapter 2 - El Camino College
... At Earth’s North Pole, we would see half of the celestial sphere. The north celestial pole would be at the zenith, the ...
... At Earth’s North Pole, we would see half of the celestial sphere. The north celestial pole would be at the zenith, the ...
SNC 1D1 Space Unit Review Answers How long does it take the
... 365.256 days (365 days is an acceptable answer) 3. At what angle does the Earth rotate at, relative to its orbit of the Sun? 23.5o 4. How long does it take our Moon to make 1 full revolution of the Earth? 27.322 days (27 or 28 days is an acceptable answer) 5. Explain the difference between rotation ...
... 365.256 days (365 days is an acceptable answer) 3. At what angle does the Earth rotate at, relative to its orbit of the Sun? 23.5o 4. How long does it take our Moon to make 1 full revolution of the Earth? 27.322 days (27 or 28 days is an acceptable answer) 5. Explain the difference between rotation ...
File
... • Has a small rocky core covered with liquid gas • Has many moons surrounding it • The rings are made up of millions of ice crystals, some as big as houses and others as small as specks of dust • Very light as it is made up of more hydrogen than helium so it is less dense ...
... • Has a small rocky core covered with liquid gas • Has many moons surrounding it • The rings are made up of millions of ice crystals, some as big as houses and others as small as specks of dust • Very light as it is made up of more hydrogen than helium so it is less dense ...
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. ...
Gravitation and Orbital Motion
... better to weigh yourself when this heavenly body is directly overhead! If you have a mass of 85.0 kg, how much less do you weigh if you factor in the force exerted by the Moon when it is directly overhead (compared to when it is just rising or setting)? Use the values 7.35×1022 kg for the mass of th ...
... better to weigh yourself when this heavenly body is directly overhead! If you have a mass of 85.0 kg, how much less do you weigh if you factor in the force exerted by the Moon when it is directly overhead (compared to when it is just rising or setting)? Use the values 7.35×1022 kg for the mass of th ...
Our Solar System
... remnants left over from the formation of the planets. Most asteroids are found in the asteroid belt between the orbits of Mars and Jupiter, and most trans-Neptunian objects lie in the Kuiper belt outside the orbit of Neptune. Pluto is one of the largest members of the Kuiper belt. ...
... remnants left over from the formation of the planets. Most asteroids are found in the asteroid belt between the orbits of Mars and Jupiter, and most trans-Neptunian objects lie in the Kuiper belt outside the orbit of Neptune. Pluto is one of the largest members of the Kuiper belt. ...
The Sun . . .
... according to their luminosity/absolute magnitude, and spectral class based on color and surface temperature. Luminosity: The brightness of a star compared to the Sun. Absolute Magnitude: Compares the brightness of stars from a standard distance from Earth. ...
... according to their luminosity/absolute magnitude, and spectral class based on color and surface temperature. Luminosity: The brightness of a star compared to the Sun. Absolute Magnitude: Compares the brightness of stars from a standard distance from Earth. ...
Extraterrestrial skies
In astronomy, the term extraterrestrial sky refers to a view of outer space from the surface of a world other than Earth.The sky of the Moon has been directly observed or photographed by astronauts, while those of Titan, Mars, and Venus have been observed indirectly by space probes designed to land on the surface and transmit images back to Earth.Characteristics of extraterrestrial skies appear to vary substantially due to a number of factors. An extraterrestrial atmosphere, if present, has a large bearing on visible characteristics. The atmosphere's density and chemical composition can contribute to differences in colour, opacity (including haze) and the presence of clouds. Astronomical objects may also be visible and can include natural satellites, rings, star systems and nebulas and other planetary system bodies.For skies that have not been directly or indirectly observed, their appearance can be simulated based on known parameters such as the position of astronomical objects relative to the surface and atmospheric composition.