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Astronomy from the ancients to the Renaissance
Astronomy from the ancients to the Renaissance

... Astronomy of the ancients Many ancient cultures took note of celestial objects and celestial phenomena. They noted certain patterns in the heavens and were able to construct calendars. The Chinese, Egyptians, Britons, Mayans, and others have left us evidence of their interest in astronomy. ...
Jun - Wadhurst Astronomical Society
Jun - Wadhurst Astronomical Society

... was a mathematician and predicted a transit of Vulcan across the face of the Sun in 1843. But it didn’t happen. Eventually Le Verrier said that it wasn’t possible to give an explanation although at the time he was using Newton’s laws of planetary motion. But as Brian said, he was well respected beca ...
Chapter 6 Physics
Chapter 6 Physics

... 1. If a rocket is given a great enough speed to escape from Earth, could it also escape from the Sun and, hence, the solar system? What happens to the artificial Earth satellites that are sent to explore the space around distant planets, such as Neptune? 2. Assuming that a rocket is aimed above the ...
oceanworlds1
oceanworlds1

... The Earth is not the only planet in the solar system with an ocean. Scattered throughout the outer reaches are icy asteroids, moons, and dwarf planets; any of which could contain a large buried body of water. This intriguing possibility suggests we should refocus our exploration efforts if we want t ...
Announcements Ancient astronomers: Why did they do it? Why did
Announcements Ancient astronomers: Why did they do it? Why did

... Used experiments to show that objects in motion tend to remain in motion Many observations (with the new-fangled invention called the telescope showed that the heavens are far from perfect (e.g., spots on the Sun, jagged mountains and valleys on the Moon) The Milky Way indicated that stars are far m ...
The length of an Earth day is determined by the time required for
The length of an Earth day is determined by the time required for

... the number of sunspots increases the Sun gives off more energy Earth’s northern axis is tilted toward the Sun A lunar eclipse does not occur every month because sometimes the Moon is closer to the Earth. the Moon always keeps the same side toward the Earth. the Moon's orbit is inclined with respect ...
Topic IV: Motions of the Earth, Moon and Sun
Topic IV: Motions of the Earth, Moon and Sun

... 1) Didn’t explain retrograde motion 2) Didn’t explain Coriolis or Foucault 3) Models should be simple (epicycles) ...
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... • The earth was too big to rotate once a day. It would fly apart. • Stars did not show parallaxes during the year, which they must if the earth goes around the sun. This argument was conclusive for most people. The only way out: the stars must be very far away! ...
Moons of the planets
Moons of the planets

... Saturn was 19 arcseconds (remember what an arcsecond is). At that time, the angular diameter of the moon Titan (the star off to the left that night) was 0.84 arcseconds, smaller than the “seeing disk” due to the Earth’s atmosphere. ...
Chapter 17 Packet Pages
Chapter 17 Packet Pages

... 10. Complete the chart to tell about lunar eclipse and solar eclipse ...
Name____________________________________________________________________ Astronomy Packet 4
Name____________________________________________________________________ Astronomy Packet 4

... actually comes down as _____________ but it never reaches the ground due to the high temperature. The surface of Venus is covered in _____________ and ____________. The largest of which is _______________. In fact it is the high amount of ________________________ that maintains the thick atmosphere. ...
Unit 5
Unit 5

... Earth revolves around the Sun in and year and rotates on its axis in a 24-hour day. They have related this rotation of Earth to day and night while recognizing that the movements of the sun, moon, and stars are connected. SC.5.E.5.1: (DOK 1) Recognize that a galaxy consists of gas, dust, and many st ...
Night Sky Checklist Year-Round Unaided Eye Astronomy
Night Sky Checklist Year-Round Unaided Eye Astronomy

... are actually caused by small bits of rock and metal called meteoroids entering Earth’s atmosphere from space. They can be bright or dim, and last only seconds. Airplanes are easily distinguished from satellites because airplanes have flashing lights. Satellites may change their brightness slowly or ...
Categorizing Solar System Objects
Categorizing Solar System Objects

... Titan, satellite of Saturn – Titan is Saturn’s largest moon. Its diameter is 3,200 miles, the size of the United States. Triton, satellite of Neptune – Triton is covered in ice and may have a weak atmosphere. Venus, planet – Vesta, asteroid – Vesta has an interesting surface with clear light and dar ...
2003-1
2003-1

... of Venus. During the month, these two planets move away from each other in the sky. By January 31, they rise more than an hour apart (Mars at 3:04, Venus at 4:11), and Venus is 16 degrees away from Mars. Venus is the brightest object in the sky, after the Sun and Moon. At a magnitude of -4.4, it's a ...
Week 5 File
Week 5 File

... centre  of  the  slit  at  distance  D/2  away.  The  difference  in  the  path  length  of  the  two  rays  is  given     by  D/2  sinθ,  where  θ  is  the  angle  between  the  opFcal  axis  and  line  joining  the  point   ...
Fall 2014 -- Astronomy 1010: Planetary Astronomy Exam 1
Fall 2014 -- Astronomy 1010: Planetary Astronomy Exam 1

... at the center of the Milky Way near the center of the Milky Way about halfway out from the center of the Milky Way at the farthest outskirts of the Milky Way outside the Milky Way, which is why we can see it as a band across the night sky ...
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... intelligence is favored by natural selection and closely linked to language. • Cultural evolution on Earth began around 10,000 years ago. ...
Cosmology questions (Introduction)
Cosmology questions (Introduction)

... A space tourist spends a day (Sunrise to Sunrise) on each planet in the Solar System, before travelling to the next planet aboard a futuristic spacecraft which can travel at 0.1% of the speed of light, c  2.998 108 ms-1 Ignoring relativistic effects and also differences in distances between the pl ...
Rotational Axis
Rotational Axis

... Each 4 years, one day is added to the month of February to make up for the 0.25 (1/4) rotation in each revolution around the sun. ...
Earth`s Rotation and Effects
Earth`s Rotation and Effects

... The side closer to the moon accelerates (tends to move) towards it faster than the farther side, which lags behind. Relative to the center, the earth is stretched in opposite directions The Moon does NOT “lift” the water up on one side of the Earth closest to it! High and low tides ~ 12hrs; alternat ...
Planetary Science - Columbia Falls Junior High
Planetary Science - Columbia Falls Junior High

... strength of decreases as the gravity) distance between the objects increase. ...
the solar system and the universe
the solar system and the universe

... four days (Jupiter’s orbit takes twelve years!) This illustrated that exoplanets are quite different to those in our Solar System, and prompted much more research into finding these strange worlds. ...
brock university answers
brock university answers

... (b) about the same temperature as its surface. (c) * much hotter than its surface. (d) [It’s impossible to tell from geological evidence.] 7. Significant atmospheric winds exist on (a) the Moon. (b) Mercury. (c) * Mars. (d) Pluto. 8. Impact craters are found on the surface of (a) Jupiter. (b) Saturn ...
study-notes-for-2016-2017-1st-qtr-exam
study-notes-for-2016-2017-1st-qtr-exam

... based on distance from the sun and common characteristics. The 4 inner planets are considered rocky planets and are smaller than the outer planets. The outer planets (Jupiter, Saturn, Uranus, and Neptune) are much larger in comparison and are considered “gas giants” because of their size and their p ...
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Comparative planetary science

Comparative planetary science or comparative planetology is a branch of space science and planetary science in which different natural processes and systems are studied by their effects and phenomena on and between multiple bodies. The planetary processes in question include geology, hydrology, atmospheric physics, and interactions such as impact cratering, space weathering, and magnetospheric physics in the solar wind, and possibly biology, via astrobiology.Comparison of multiple bodies assists the researcher, if for no other reason than the Earth is far more accessible than any other body. Those distant bodies may then be evaluated in the context of processes already characterized on Earth. Conversely, other bodies (including extrasolar ones) may provide additional examples, edge cases, and counterexamples to earthbound processes; without a greater context, studying these phenomena in relation to Earth alone may result in low sample sizes and observational biases.
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