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m02a02
m02a02

... the summer sky, the heating of the Earth’s surface is more direct plane of the ecliptic (whereas the low winter Sun‘s heating is more diffuse). ...
HomeWork #2
HomeWork #2

... for the observed motions of the planets, and so was considered more reliable than the geocentric theory. j 2. the heliocentric theory accounted for the same observed motions of the planets as the k l m n geocentric theory, but did so in a much simpler way. j 3. the heliocentric theory accounted for ...
February 2010 - Newbury Astronomical Society
February 2010 - Newbury Astronomical Society

... The dates for the next 6 months are shown along the bottom of the chart and the time up the sides. The areas shown light blue at the top and bottom indicate daylight. The lower thick curved line shows the start of dusk and the upper shows the end of dawn (full daylight). The conical curved black lin ...
SDO | solar dynamics observatory
SDO | solar dynamics observatory

... Earth revolves around the Sun once per year. The seasons on Earth are caused by the tilt of Earth on its rotation axis, which is approximately 23.5 degrees with respect to it’s plane of orbit. As Earth revolves around the Sun its axis is continually tilted in the same direction. If you extended the ...
PLANETARY MOTIONS
PLANETARY MOTIONS

... device, the orrery to represent planetary motions in an accelerated fashion. An orrery is a mechanical model of the Solar System. The model Sun is at the center and the model planets are driven around by a system of gears. Sometimes, on more elaborate orreries, some of the many satellites (moons) ar ...
Navigation
Navigation

... system using radio signals transmissions @ 100 KHz from 3 or more transmitters, linked in a chain. It gives a latitude and longitude readout position to marine, aero and land receivers. ...
Mercury`s MESSENGER mission comes to a crashing climax
Mercury`s MESSENGER mission comes to a crashing climax

... It also allowed measurement of the effects of solar in November 2012, NASA announced, evidence of wind and Mercury's magnetic field at varying water ice and carbon-containing tar-like organic distances, as well as capturing close-up compounds molecules at both of Mercury's poles. measurements and p ...
The cosmological distance ladder
The cosmological distance ladder

... The Cosmological Distance Ladder ...
Jupiter
Jupiter

... Seen here is a full-scale model of one of the twin Voyager spacecraft, which was sent to explore the giant outer planets in our solar system. ...
Gravitation
Gravitation

... The planet Saturn has 100 times the mass of the Earth and is 10 times more distant from the Sun than the Earth is. Compared to the Earth’s acceleration as it orbits the Sun, the acceleration of Saturn as it orbits the Sun is 1. 100 times greater ...
Astronomy and Space Science
Astronomy and Space Science

... • Aristotle’s (384-322 BCE) model placed the superior planets in right order using their speed on the celestial sphere. • It explains simple phenomena such as daily rise and set of celestial objects, but not the details in longer time scales. • In this model, the Earth is at the center the universe, ...
Gravity
Gravity

... CTGravity-6. A rock is released from rest at a point in space far from Earth, beyond the orbit of the Moon. The rock falls toward the Earth and crosses the orbit of the Moon. When the rock is the same distance from the Earth as the Moon, the magnitude of the acceleration of the rock is .. (Ignore th ...
The Seasons (PowerPoint)
The Seasons (PowerPoint)

... Does the Earth itself really move, orbiting around a static Sun? (Wouldn’t we feel that motion?) Or does the Sun move around the static Earth, as the ancient Greeks thought? We will return to this question later. Whichever is correct, the result is the same! We will ...
EarthScience-Astronomy-TheSolarSystem
EarthScience-Astronomy-TheSolarSystem

... fall.) There are 12 hours of daylight and 12 hours of darkness. The Sun is directly overhead at the equator (0°N) at noon. k. Fall (Autumnal) Equinox- September 22 or 23. This is the first day of fall in the Northern Hemisphere (in the Southern Hemisphere this is the first day of spring.) There are ...
Unit I – The Seasons
Unit I – The Seasons

... Does the Earth itself really move, orbiting around a static Sun? (Wouldn’t we feel that motion?) Or does the Sun move around the static Earth, as the ancient Greeks thought? We will return to this question later. Whichever is correct, the result is the same! We will ...
Daynightseasonsstars-1
Daynightseasonsstars-1

... generated inside the sun about 100,000 years ago ...
NATS1311_090908_bw
NATS1311_090908_bw

... than the usual three - the third is the Blue Moon - found only in February, May, August, and November, one month before the next equinox or solstice. The result of following rules laid down as part of the Gregorian calendar reform in 1582. The ecclesiastical vernal (spring) equinox always falls on M ...
Here
Here

... • In modern times, it was discovered that the human eye has a nonlinear response to light: if one source of light has twice the light as a second source, then the first source would not appear by eye to be twice as bright. • The response of the eye is logarithmic, so that differences of magnitudes c ...
Condensation of the Solar Nebula
Condensation of the Solar Nebula

... during the early stage of the solar system formation process, when there were still many planetesimals floating around. Evidences of Impact • Comet Shoemaker’s collision with Jupiter • Surface of the Moon and Mercury, • More in Chapter 7… Effects of Impact • Tilt of the rotation axis of planets (Ven ...
Teacher`s Guide - Discovery Education
Teacher`s Guide - Discovery Education

... Find out how the solar system formed and observe a model illustrating its vast distances. The Planets Discover the differences between the inner and outer planets. Listen to scientists debate Pluto’s status as a planet, and observe photographs of Jupiter from spacecraft. Comets and Asteroid Check ou ...
Ch9CTa
Ch9CTa

... Also, the work-energy theorem saysWnet = KE. The work must be positive, since by Kepler's second law, the planet moves faster (has higher KE) when it is nearer the Sun, so KE>0. ...
Other Bodies in the Solar System
Other Bodies in the Solar System

... • In 1800 astronomer Franz Xaver von Zach assembled the Celestial Police • Searching for “the missing planet” between mars and Jupiter • Based off Predictions by Johann Daniel Titius vonWittenburg • In 1801 Giuseppe Piazzi discovered the planet “Ceres” • William Herschel categorized Ceres and the ot ...
Lecture 7 Phys 1810
Lecture 7 Phys 1810

... • Tidal forces: cause distortion of an object by pull of another object. • Can occur when – Objects close (e.g. Earth & Moon) – 1 object is very massive (e.g. Jupiter & Io; Sun & Earth.) ...
Physics Today
Physics Today

... The nature of our Moon The natural first step in understanding our Moon is to consider its composition. We’ve all heard the amusing myth that the Moon is made of green cheese, a theory that, astonishingly, has been tested (see box 1). The six Apollo Moon missions, conducted between 1969 and 1972, no ...
Introduction to Earth Science - The Federation of Galaxy Explorers
Introduction to Earth Science - The Federation of Galaxy Explorers

... vital to our survival. That is atmospheric pressure. Without atmospheric pressure, we would literally explode and we wouldn’t want that to happen. We are most comfortable with a pressure of 10 to 15 pounds per square inch. Thus we can live at sea level or in the mountains. Let’s tell the engineers t ...
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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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