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COORDINATES, TIME, AND THE SKY John Thorstensen
COORDINATES, TIME, AND THE SKY John Thorstensen

... equal to your latitude. Note that altitude is measured along a great-circle arc which passes through the object and the zenith. The existence of a pole implies the existence of a celestial equator, which is the set of all directions 90 degrees from (either) pole. If you stand on the north or south p ...
Celestial Motions
Celestial Motions

... © 2010 Pearson Education, Inc. ...
PLANETESIMALS TO BROWN DWARFS: What is a Planet?
PLANETESIMALS TO BROWN DWARFS: What is a Planet?

... A good definition has several desirable characteristics. It should be succinct and easily understood by the public, yet precise enough to be acceptable to scientists. An ideal definition would not depend on specific knowledge or examples that will change as we learn more, although the definition of plan ...
The Night Sky
The Night Sky

... The all-sky constellation chart in the center of the November Sky & Telescope will do just fine. ...
19.
19.

... acquired by the Mariner 10 spacecraft on February 5, 1974. The image shows the thick cloud coverage that prevents optical observation of the planet's surface. The surface of Venus remained hidden until 1978 when the Pioneer Venus 1 spacecraft arrived and went into orbit about the planet on December ...
Neptune & Uranus Notes
Neptune & Uranus Notes

... Moons of Neptune  Neptune has a total of 13 known moons  The largest moon, Triton, is the only large moon in our solar system to have a retrograde orbit  Part of its surface resembles the rind of a cantaloupe  Ice volcanoes spout what is probably a mixture of liquid nitrogen, methane, and dust, ...
Earth Science Units of Study - eLearning
Earth Science Units of Study - eLearning

... (a) It is made up of solar systems, which contain galaxies. (b) It is made up of a few galaxies and billions of stars. (c) It is made up of billions of galaxies, which contain billions stars. (d) It is made up of solar systems and billions of stars. ...
What CAN You See With a Telescope?
What CAN You See With a Telescope?

... Early astronomers had used their telescopes to measure the rotation rate of the Sun and some of the  planets. Since the asteroids were thought to be “minor planets,” it was assumed that they also rotated  on their own axes. In 1810, Schröeter 6  thought Juno had a 27­hour rotation rate. This is abou ...
Chapter 11
Chapter 11

... Jupiter is surrounded by belts of charged particles, much like the Van Allen belts but vastly larger Magnetosphere is 30 million km across ...
Reference PDF document
Reference PDF document

... From a visual point of view, the phenomenon of the transit of Venus is similar to Mercury’s: Venus is visible as a black circle moving slowly over the brilliant solar disk. The transit of Venus lasts a maximum of 8 hours. During the transit, Venus has a very small apparent diameter. However, it is c ...
PARAMOUNT SCHOOL OF EXCELLENCE TIME AND SPACE
PARAMOUNT SCHOOL OF EXCELLENCE TIME AND SPACE

... Explain that we can use these powers of 10 to represent decimal places, too: a. 3.4 can be written as 3.4 x 100. b. 99.1 can be written as 9.9 x 101. c. 4,526 can be written as 4.526 x 103. Review the properties of exponents to make scientific notation even more useful: d. When multiplying two numbe ...
Earth and Space Science Unit Outline Welcome to High School
Earth and Space Science Unit Outline Welcome to High School

... 13. Compare environmental conditions during the ice age to present. 14. Compare environmental conditions during the little ice age to present. Climate Change 15. Describe factors that contribute to global climate change. 16. Describe the movement of carbon through the different systems of the Earth ...
Example 13.1 Billiards, Anyone? Three 0.300
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... 5. Imagine that nitrogen and other atmospheric gases were more soluble in water so that the atmosphere of the Earth is entirely absorbed by the oceans. Atmospheric pressure would then be zero, and outer space would start at the planet’s surface. Would the Earth then have a gravitational field? (a) Y ...
The complex planetary synchronization structure of the solar system
The complex planetary synchronization structure of the solar system

... In 1543 the De revolutionibus orbium coelestium (On the Revolutions of the Heavenly Spheres) was published. As opposed to Ptolemy’s geocentric model that had been widely accepted since antiquity, Copernicus (1543) proposed a heliocentric model for the solar system: the planets, including the Earth, ...
Chapter 2 Text - UW Atmospheric Sciences
Chapter 2 Text - UW Atmospheric Sciences

... increased by about 30% during the lifetime of Earth, about 4.5 billion years. The cause of this increased energy output is the gradual increase in the density of the sun, as lighter elements convert to heavier ones. The solar system includes nine planets. They may be divided into the terrestrial, o ...
The Digital Carousel
The Digital Carousel

... What is needed for life - where all these exist and persist is where you look for life ...
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... A person on earth would be mostly looking at the unlit side of the moon, which is not visible. In the northern hemisphere a little bit on the right side would be lit: a crescent moon. ...
Astronomy: A Day-time Activity
Astronomy: A Day-time Activity

... stars, and all other natural objects in the solar system move around us from east to west. We say that the sun ―goes across the sky.‖ The astronaut’s view — An astronaut looking at the Earth from space sees the Earth rotating from west to east as it revolves around the sun. They say that, ―it is the ...
Comet Catalina 2016 - Fraser Heights Chess Club
Comet Catalina 2016 - Fraser Heights Chess Club

... at the end of the Big Dipper's handle • January 16 — Passes 2° southwest of the 8thmagnitude galaxy, M101 • January 17 — Passes 3.4° northeast of the double star Mizar in the bend of the Big Dipper's handle ...
Ancient Astronomy - Sierra College Astronomy Home Page
Ancient Astronomy - Sierra College Astronomy Home Page

... Three modern criteria of scientific models: – Model must fit the data – Model must make predictions that can be tested and be of such a nature that it would be possible to disprove it – Model should be aesthetically pleasing simple, neat, and elegant (Occam’s razor) ...
Science and the Universe
Science and the Universe

... Sun at its center and nine planets orbiting the Sun – The Earth is one of the nine planets • The Sun is a star – Its diameter is 1.5 million km • A planet is a body of significant size that orbits a star and does not produce its own light • A star is large body which (at some point during its life) ...
Understanding Precession of the Equinox
Understanding Precession of the Equinox

... would slowly change the seasons within the calendar. For example, in the Northern Hemisphere it would eventually become winter in July and August, and summer in January and February. This is because the seasons are indirectly caused by axial tilt (summer when that hemisphere leans closer to Earth, a ...
The Search for Extrasolar Earth-like Planets
The Search for Extrasolar Earth-like Planets

... calculations of the orbital stability of an Earth-mass planet at various semi-major axes for specific systems with known giant planets give a more concrete answer about which stars are dynamically able to harbor terrestrial planets at terrestrial-like semi -major axes. Transits as a Planet Detection ...
The Starry Messenger
The Starry Messenger

... Great indeed are the things which in this brief treatise I propose for observation and consideration by all students of nature. I say great, because of the excellence of the subject itself, the entirely unexpected and novel character of these things, and finally because of the instrument by means of ...
September 3, 2013
September 3, 2013

... appears 12th or 13th magnitude. If you succeed, could this be your record-farthest galaxy? The cluster is 300 million lightyears away. Use the finder charts and photo with Ken HewettWhite's "Going Deep" article in the September Sky & Telescope, page 60. Wednesday, September 4 • The big but dark-colo ...
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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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