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Solutions
Solutions

... as we define them. Consider a planet at 1 AU orbiting in a circle. If the sun were more massive, that would mean greater gravitational force on a planet at a given distance, and therefore greater acceleration. Greater acceleration means that the velocity is changing faster. If you have a circlar orb ...
Solar System
Solar System

... -It is the largest planet in the solar system and the 4th BIGGEST object in the sky! -Since prehistoric times it has been known at a bright “wandering star”. ...
Slide 1
Slide 1

... • When the sun and moon moved 180 degrees to the other side of the earth in winter, the moon may now appear near Arcturus that night in the handle of the Big dipper pointing straight up at midnight. • And earth flow out of the reverse orbit of the sun. • The constellation T'ien-t'ing is the polar ...
Matariki-Maori New Year
Matariki-Maori New Year

... • If the stars were clear and bright, it was a sign of a favourable and productive season ahead, and planting would begin in September. • If the stars appeared hazy and closely bunched together, a cold winter was in store and planting was put off until October. ...
January 14 - Astronomy
January 14 - Astronomy

... Florida is closer to the equator and a space shuttle just sitting on the launch pad is moving about 1,550 km/hr. If we moved the launch pad to Maine, the space shuttle sitting on the launch pad is only moving 1,275 km/hr or about 275 km/hr less than in Florida. To launch the space shuttle in Maine ...
lecture 1 - University of Florida Astronomy
lecture 1 - University of Florida Astronomy

... Coordinate system on Earth ...
Document
Document

... b) slow motion of the Earth's rotation axis on the celestial sphere. c) apparent backward motion of planets on the celestial sphere. e) daily eastward motion of the Sun around the celestial sphere. ...
Unit 2 - Astronomy
Unit 2 - Astronomy

... • Autumnal Equinox - first day of fall (September 21) in the N. Hemisphere when there are equal amounts of day and night ...
celestial equator
celestial equator

... is magnificent. Roughly 2000 stars are visible to the unaided eye. If you know where to look, you can see Mercury, Venus, Mars, Jupiter, Saturn, and even Uranus. Occasionally, a bright comet is visible. On certain nights of the year there are many meteors (shooting stars) to be seen. Sometimes man-m ...
Key Stage 2: Teacher`s Pack
Key Stage 2: Teacher`s Pack

... 8. The rotational period of a star is the time it takes to spin around once. The Crab pulsar spins on its axis 30 times a second. What is its rotational period? Period = 1 / frequency = 1/30 = 0.033 seconds 9. This shows one way of finding exoplanets. The amount of light from the star is being measu ...
instructor notes: week 2
instructor notes: week 2

... distance from the true horizon upwards. Ecliptic. The great circle in the sky along which the Sun appears to move because of Earth’s orbit about it. Right Ascension. A celestial co-ordinate like longitude on Earth, increasing eastwards. Declination. A celestial co-ordinate like latitude on Earth, me ...
Chapter 9
Chapter 9

... Tides are caused by the difference in gravity between the moon & earth on opposite sides of the earth (different distances)  The force is stronger wherever the moon is closer to the earth and weaker wherever the moon is farther, and water can move easily!  The high tide bulge follows the moon arou ...
astrofe –astronomy ofe
astrofe –astronomy ofe

... Please describe the parts of a rocket below. What are some parts of a basic rocket and how do they work? ...
TAKS Study Guide - Northwest ISD Moodle
TAKS Study Guide - Northwest ISD Moodle

... 11. What processes does it take to form a metamorphic rock? 12. Give 2 examples for how catastrophic events can change the Earth’s surface. a. b. 13. What is the theory for how dinosaurs became extinct? 14. What are the 2 main factors that affect climate? ...
Notes for Unit 5
Notes for Unit 5

... -note that a few ancient Greeks had proposed a sun-centered universe, but their arguments didn’t hold up to Ptolemy’s. -in 1543, Nicholas Copernicus’ On the Revolutions of the Heavenly Bodies was published. He proposed a sun-centered universe. Note that although this was a radical change, he used ma ...
ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy
ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy

... Why did the asteroid belt between Mars and Jupiter not form into a planet? Do we have the technology to change the path of an asteroid? What is the difference between asteroids, comets, and meteors? Why is it believed that comets are derived from the Oort cloud? How often do Near Earth Objects enter ...
ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy
ASTRONOMY CURRICULUM Unit 1: Introduction to Astronomy

... Why did the asteroid belt between Mars and Jupiter not form into a planet? Do we have the technology to change the path of an asteroid? What is the difference between asteroids, comets, and meteors? Why is it believed that comets are derived from the Oort cloud? How often do Near Earth Objects enter ...
Second Lecture - University of Maryland Astronomy
Second Lecture - University of Maryland Astronomy

... Let R be the radius of that circle and T the time it takes the Moon to go around once, about one month (720hours). In that time the Moon covers a distance of 2πR An eclipse of the Moon occurs when the Moon passes through the shadow of the Earth, on the opposite side from the Sun (therefore, it must ...
Solar System.3rd.Mark Vega
Solar System.3rd.Mark Vega

... out circle) counterclockwise direction. The inner planets orbit much faster then the outer planets. Venus is the one inner planet that has a different rotation – it rotates in a clockwise rotation while all the other inner planets rotate in a counter-clockwise direction. The outer planets all rotate ...
Ice Giant Neptune Frontlines Potentially Hazardous Asteroid
Ice Giant Neptune Frontlines Potentially Hazardous Asteroid

... Earth on its closest approach. The asteroid, which we nicknamed “Dodgeball” because of its  frequent returns to Earth’s vicinity, was originally listed on the Sentry Risk Table with a Torino  Scale rating of 1 ­ at which time the asteroid was calculated to have a 1 in 9,300 chance of  impacting Eart ...
Cycles: Earth, Sun, Moon by MTDavis
Cycles: Earth, Sun, Moon by MTDavis

... ONE ROTATION of the earth on it’s axis = ONE DAY ONE MOON CYCLE =about 29.5 DAYS, which should be ONE MONTH. 12 X 29.5 = 354 days, 11 days short of the real SOLAR CALENDAR, so Julius Caesar, with the help of Greek science, changed our months to 30 or 31 day months which no longer match the moon cyc ...
Lecture 3a
Lecture 3a

... besides Earth could be at the center of motion) •  There were many more stars •  Venus had definite phases and was clearly orbiting the •  Observed Saturn’s rings, but didn’t understand what they were •  Observed sunspots on the sun, that the sun revolved on its own axis – wasn’t “perfect” and chang ...
ISP 205: Visions of the Universe
ISP 205: Visions of the Universe

... The rotation of the earth about its axis causes how many of the following? -The rising and setting of the sun -The rising and setting of the moon -The rising and setting of stars -The rising and setting of distant galaxies Answer: 0, 1, 2, 3, or 4? ...
Samenvatting ANW SPU set 3 Chapter 2: The Earth What are
Samenvatting ANW SPU set 3 Chapter 2: The Earth What are

... What are the differences between a star and a planet? The basic difference between a star and a planet is that a star emits light produced by a nuclear reaction in its core, whereas a planet only shines by reflected light. Not all objects in the universe that don't produce their own light are planet ...
B. protostar - University of Maryland Astronomy
B. protostar - University of Maryland Astronomy

... 6. Cepheid variable stars could be used to determine distance after Henrietta Leavitt established a correlation between_____________________________ using a sample of these stars found in the Magellanic Clouds. A. luminosity and absolute magnitude B. apparent and absolute magnitudes C. red shift an ...
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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.
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