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Earth Moon Sun System PPT
Earth Moon Sun System PPT

... away from Earth than the moon – this is what makes the two objects the same size in the sky. • Solar eclipses occur when the moon passes between the Sun and Earth. • Not everyone gets to see a solar eclipse b/c the moon’s shadow that falls on Earth is very small (only 167 miles wide) and moves quick ...
How we know the Earth moves - Michael Beeson
How we know the Earth moves - Michael Beeson

... to fire a rocket due north, over the pole for example, by the time it landed, the original target would have moved eastward due to the Earth’s rotation. You could see that you had aimed right, because your rocket would pass over the pole. The same effect can be seen in a shorter flight, and has to b ...
waves
waves

... objects that orbit the central star, known as the Sun; e.g. planets, moons, asteroids, comets, meteoroids a piece of rock, smaller than a planet, that orbits the Sun; many are found orbiting in a region between Mars and Jupiter a mass of frozen gases and rock particles that orbits the Sun a chunk of ...
Space and Technology
Space and Technology

... Jupiter - powerful lightning storms - ___________ Great Red Spot Saturn - thousands of rings of ice, rock and dust • ______ • ______ Uranus - spins on its side • _______ Neptune - huge circular storm (like Jupiter’s) ...
How the Hubble Telescope Will Look at the Moon to See Venus
How the Hubble Telescope Will Look at the Moon to See Venus

... · The waning gibbous Moon is up in the southeast by around 11 p.m., depending on where you live. Look about a fist-width to the Moon's right for fiery Antares. Around and upper right of Antares are other stars of Scorpius. Tuesday, May 8 · The brightest star very high in the east these evenings is A ...
A105 Stars and Galaxies
A105 Stars and Galaxies

... • Instead of a planet rotating around the center of the Sun, it actually rotates around the center of mass of the two bodies • Each body makes a small elliptical orbit, but the Sun's orbit is much much smaller than the Earth's because it is so much more massive ...
Document
Document

... • “Fast electrons” produced when the solar wind hits Jupiter’s magnetosphere • Lethal rays: density of particles is thousands of ...
Document
Document

... • “Fast electrons” produced when the solar wind hits Jupiter’s magnetosphere • Lethal rays: density of particles is thousands of ...
December 2007 Clear Skies Newsletter PDF
December 2007 Clear Skies Newsletter PDF

... Arizona. Astronomers discovered that active, supermassive black holes were ubiquitous in the early universe, though they are difficult to observe. Black holes are objects so dense that not even light can escape the grasp of their massive gravitational fists. They are detected by studying their effec ...
The Wizard Test Maker
The Wizard Test Maker

... Base your answers to questions 12 and 13 on the diagram below, which represents the position of the Sun with respect to Earth’s surface at solar noon on certain dates. The latitudes of six locations on the same line of longitude are shown. The observer is located at 42° N in New York State. The dat ...
Gravitational Forces
Gravitational Forces

... the Earth but with a radius that is 3.5 times less than the Earth’s . ___________________________________________________________________________________ ___________________________________________________________________________________ ______________________________________________________________ ...
The Earth-Moon-Sun System
The Earth-Moon-Sun System

... Stonehenge may also have provided a method of determining eclipses ...
If you wish to a copy of this months Night Sky News
If you wish to a copy of this months Night Sky News

... The Leonid meteor shower can be seen emanating over the eastern horizon at about 11:00 pm from the 15th to 20th November. Its maximum is on the 17th. With a ZHR ~ 15, the Leonids can provide very fast, magnificent displays, with persistent trains from its radiant around the neck of Leo. The rates ar ...
Sun - Midlandstech
Sun - Midlandstech

... preview only sets the stage for the drama to come. Now it is time to return to Earth and look closely at the sky. To understand what you are in the universe, you must know where you are. As you look at the sky, you can ...
The Solar System
The Solar System

... The Sun is our closest star. It is a member of the Milky Way galaxy. The Sun is a yellow dwarf star, which means it is a medium size star. It is believed to be over 4 billion years old. The Sun spins slowly on its axis as it moves around the galaxy. Because the Sun is so massive, it exerts a powerfu ...
Your Place in Space and Time
Your Place in Space and Time

... are microscopic on this scale. The portion of the universe that we can observe is limited by the age of the universe: Because our universe is about 14 billion years old, we can see no more than about 14 billion light-years in any direction. Measurements indicate that the observable universe contains ...
Habitability: Good, Bad and the Ugly
Habitability: Good, Bad and the Ugly

... Luminosity of the Sun • Definition of luminosity (watts/m2) • Sun’s luminosity has been changing: earlier in its evolution, luminosity was only 70% of what it is today (how could temperature be maintained over geological time) • Future for luminosity – Remember star sequence from lab and lecture – 2 ...
NAME: CLASS: 1 Solar System Formation: PowerPoint Notes Sheet
NAME: CLASS: 1 Solar System Formation: PowerPoint Notes Sheet

... Which planets rotate faster? gaseous Which type of planets have many moons? Gaseous Slide 4: What is special about Pluto? Inclined orbit (18 degrees) and oval shape - not circular Slide 5: List the planets in order of increasing tilt angle: Mercury, (0), Jupiter (3) Earth (23) Mars (25) Saturn (27), ...
Solar System
Solar System

... • These planets are named terrestrial because of their solid, rocky surfaces. • These planets are sometimes called the inner planets. ...
Digital Moon - Net Start Class
Digital Moon - Net Start Class

... A class is planning a trip to the beach. They would like to choose a day that will be the most sunny yet have a lower temperature for the daily high. Based on this five-day prediction, which day should they choose? ...
September 2015 - Hermanus Astronomy
September 2015 - Hermanus Astronomy

... supernovae. They are detected from Earth by the beams of radio waves that emanate from their magnetic poles and sweep across space as the pulsar rotates. Since they are phenomenally dense and massive, yet comparatively small - a mere 20–25 km across some pulsars are able to maintain their rate of sp ...
Asteroids
Asteroids

... sublimed from the solid nucleus. The coma and the nucleus form the head of a comet. Ion Tail: A tail of charged gases (ions) always faces away from the sun because the solar wind (ions streaming from the sun at high velocities) pushes it away (it is also called the plasma tail). When the comet is ap ...
Climbing the Cosmic Distance Ladder: How Astronomers Measure
Climbing the Cosmic Distance Ladder: How Astronomers Measure

... Distances to very distant stars  •  This gave a way to obtain the absolute brightness for  these stars, and hence observed distances.   •  Because Cepheids are so bright, this method works  up to 13,000,000 light years, well beyond the Milky  Way! Most galaxies are fortunate to have at least  one  ...
Gravity
Gravity

... the basic force in the universe. Every body (planet, moon, star, comet, asteroid, meteor, etc.) in the solar system has a force that pulls things to itself. That's gravity- the force of attraction between all objects in the universe. ...
The Chandler wobble and Solar day
The Chandler wobble and Solar day

... in the scope of national and international programs showed that all those studies have some common features: the star zenith distance variations were observed and interpreted (and are still being observed and interpreted) based on the “evidence”. However, even evident suggestions must be proved; unf ...
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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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