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RP 4E1 Earth in the Universe - NC Science Wiki
RP 4E1 Earth in the Universe - NC Science Wiki

... shown to be different from stars in two essential ways—their appearance and their motion. When a modest telescope or pair of binoculars is used instead of the naked eyes, stars only look brighter— and more of them can be seen. The brighter planets, however, clearly are disks. (Not very large disks e ...
Journey Through the Universe By Brian Fontaine
Journey Through the Universe By Brian Fontaine

... of gas (nebula) collapsed to form the sun, which began rotating. As time when on, the heavier dust fell toward the sun, creating the rocky inner planets, and the lighter stayed further away from the sun’s gravity, forming the outer gaseous planets. ...
2nd Planet from the Sun
2nd Planet from the Sun

... ◗ Much of the surface is covered with lava flows ...
AST 301 Introduction to Astronomy
AST 301 Introduction to Astronomy

... Apparent motion of Sun during the year The Earth orbits the Sun once a year. This makes the Sun appear to pass in front of different stars (the constellations of the zodiac) during a year. The zodiac does not lie on the celestial equator, but is on a circle tipped about 23o from the equator. This i ...
Life on Our Evolving Planet
Life on Our Evolving Planet

... us. Our Sun fuses hydrogen into helium in its core and generates energy (E=mc 2) which is radiated into the universe either as waste heat or life giving sunlight depending on your perspective. The Sun has fused hydrogen for over 4.5 billion years and will continue for five billion more years, but it ...
Solar system and eclipse
Solar system and eclipse

... 5. There's a recurring myth that pregnant women can't go outside during an eclipse. Astronomers from the Griffith Observatory in LA say they get dozens of calls about it when an eclipse happens, even though it seems irrational. But if one of your friends is pregnant, don't worry, you can invite them ...
Section 1
Section 1

... Earth and the other planets revolve around the sun. Since Galileo’s time, our knowledge of the solar system has increased dramatically. Galileo knew the same planets that the ancient Greeks had known—Mercury, Venus, Earth, Mars, Jupiter, and Saturn. Since Galileo’s time, astronomers have discovered ...
Unit 2 Section 1
Unit 2 Section 1

... Earth and the other planets revolve around the sun. Since Galileo’s time, our knowledge of the solar system has increased dramatically. Galileo knew the same planets that the ancient Greeks had known—Mercury, Venus, Earth, Mars, Jupiter, and Saturn. Since Galileo’s time, astronomers have discovered ...
Ch. 27 Notes
Ch. 27 Notes

... difficult – if lucky gravitational lensing can be used when a galaxy's image is being magnified by the gravity of a massive cluster of galaxies parked in front of it, making it appear 11 times brighter. ...
Orbit by Tega Jessa Everything in the universe circles or “orbits
Orbit by Tega Jessa Everything in the universe circles or “orbits

... Many children, and even adults, dream of visiting other planets and wonder what it would be like to stand on another planet. For one thing, your weight would be different on another planet, depending on a number of factors including the mass of the planet and how far you are away from the center of ...
Unit 5 -
Unit 5 -

... The equatorial bulge at Earth's equator is measured at 26.5 miles (42.72 km) and is caused by the planet's rotation and gravity  This means that instead of being of equal circumference in all areas, the poles are squished and a larger circumference and diameter at the equator. ...
Chapter 18 - "The Earth in Space"
Chapter 18 - "The Earth in Space"

... – Yearly time • The time required for the Earth to make one complete revolution around the Sun. • A tropical year is the time between two spring equinoxes • A sidereal year is the time required for the Earth to move around the Sun once. – A sidereal year is 365.25636 mean solar days. – This leaves ...
Student Text, pp. 139-144
Student Text, pp. 139-144

... the search for answers to questions related to the patterns and motions of those objects. Until the late 1700s, Jupiter and Saturn were the only outer planets identified in our solar system because they were visible to the naked eye. Combined with the inner planets (Mercury, Venus, Earth, and Mars), ...
PART A: MULTIPLE CHOICE (40 MARKS: 40 Minutes)
PART A: MULTIPLE CHOICE (40 MARKS: 40 Minutes)

... 13. A method used to charge an object without actually touching the object to any other charged object 14. A flow of electric charge 15. It occurs when the Moon passes between the Earth and the Sun blocking our view of the Sun. 16. Charging by contact 17. A process by which there is a net accumulati ...
Chap. 13 Gravitational Interactions
Chap. 13 Gravitational Interactions

... Ocean tides would be higher and so the tidal forces on the moon’s crust would be greater If the moon were too close, Earth’s tidal forces would tear the moon into a billion pieces, forming a ring around Earth similar to those around Saturn ...
Space (Part 1)
Space (Part 1)

... has cleared the area around its orbit of objects.” This photograph shows Pluto and its moon, Charon. Pluto’s orbit is surrounded by smaller objects which have not been cleared by its gravitational field. Pluto and the other ‘smaller’ planet-like objects such as Eris and Ceres have now been reclassif ...
Astronomy Final review key - Hicksville Public Schools
Astronomy Final review key - Hicksville Public Schools

... around the Sun. The length of daylight experienced at different latitudes on a given date is shown on the diagram. 21. Describe how the length of daylight changes from the Equator to the North Pole on the date shown. ...
16 October 2006
16 October 2006

... • Most are much closer to their stars than Jupiter. How is this possible? Our theory predicts that giant planets should be farther out! • But our detection method is inherently biased toward these cases, since they produce the greatest stellar wobble. ...
Document
Document

... surface of Mars. It has been analyzed and found to have a high iron content, so it has a rusty look. The surface of Mars is dry and rocky, and is covered with this reddish dust. The atmosphere is very thin and is composed mainly of carbon dioxide. Mars has about 1/3 of the gravity of Earth, so when ...
9/20/16 Tuesday CP class Earth to Mars article
9/20/16 Tuesday CP class Earth to Mars article

... bright red star of the sky; one of the brightest objects, rivalling the brightness of Venus or Jupiter. There’s no question Mars is bright and close, you can see it with your own eyes. Paragraph 6 And theoretically at this point, Mars and Earth will be only 54.6 million kilometers from each other. B ...
Document
Document

... • Nebular hypothesis: The solar system formed from a collapse of a giant molecular cloud • Due to some trigger (supernova?) a specific region of the cloud became denser • Due to gravity, that region started to attract more and more hydrogen • Eventually, in a specific region of the cloud the density ...
Homework 4 1 Chapter 3 October 4, 2011
Homework 4 1 Chapter 3 October 4, 2011

... helium only condense at colder temperatures. So, close to the sun where it is warmer only the rock and metal could condense and eventually form planets made of those materials. But, farther away the hydrogen and helium condensed as well, so planets in that region are composed of these elements as we ...
1. Base your answer to the following question on the
1. Base your answer to the following question on the

... 43. The planetary wind belts in the troposphere are primarily caused by the 1) Earth’s rotation and unequal heating of Earth’s surface 2) Earth’s revolution and unequal heating of Earth’s surface 3) Earth’s rotation and Sun’s gravitational attraction on Earth’s atmosphere 4) Earth’s revolution and S ...
Slide 1
Slide 1

... Recall our theory of solar system formation. Hydrogen planets would not form close to the central star, because the proto-planetary disk would have been so hot that hydrogen, helium, and hydrogen-rich compounds would have been in gas from. This is why we have terrestrial planets close to the Sun, an ...
Physics Today
Physics Today

... as that in ocean water. Because D/H ratios found in the universe vary considerably, the ocean's isotopic composition of hydrogen, along with the isotopic compositions of a large number of nonradiogenic elements in the Earth, strongly supports the meteorite mixture model for the chemical composition ...
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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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