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PowerPoint. - teachearthscience.org
PowerPoint. - teachearthscience.org

... The apparent wobble of stars due to the gravitational influence of planets is evidence of the presence of one or more planets orbiting distant stars. This has become a technique to permit us to infer the presence of planets around other stars. Planets outside our own solar system are known as exopl ...
A Solar System - Cloudfront.net
A Solar System - Cloudfront.net

... revolve around black holes. ...
Section 14.3 The Inner Planets
Section 14.3 The Inner Planets

... The Inner Planets Mercury, Venus, Earth, Mars ...
Astronomy 100 Homework #2 Solutions 1, Problem 3‐27 (2 pts
Astronomy 100 Homework #2 Solutions 1, Problem 3‐27 (2 pts

... 2.
Problem
3‐40
(2
pts).
The
recently
discovered
object
Sedna
orbits
our
sun
 beyond
Pluto,
at
an
average
distance
of
509
AU.
What
is
its
orbital
period?
 a=509
AU,
P2
=
a3.
 P
=
a3/2
=
5093/2
=
11,480
years
 3.
Problem
3‐41
(3
pts).

The
recently
discovered
Eris,
which
is
slightly
larger
than
 Plut ...
The development of science during the renaissance The
The development of science during the renaissance The

... Greeks. For example that the earth was the centre of the universe. The church liked to be correct and didn’t allowed any ideas which weren’t the same as theirs. People who had different ideas were arrested and put in jail or were killed. This was called the inquisition. Copernicus Copernicus was a G ...
Documents A, b, c page 10
Documents A, b, c page 10

... opposite to the planet's rotation (a retrograde orbit), which suggests that it may once have been an independent object that Neptune captured. The disruptive effect this would have had on other satellites could help to explain why Nereid has the most eccentric orbit of any known moon -- it's almost ...
2- Origin of the Universe
2- Origin of the Universe

keplers laws and newton - Fort Thomas Independent Schools
keplers laws and newton - Fort Thomas Independent Schools

... directly proportional to the cube of its semi-major axis. ...
The solar system
The solar system

... 17 times that of the Earth, its diameter is 4 times that of earth 8th planet in order from the Sun, it is about 4.5 billion kilometers from the Sun Makes one complete orbit around the Sun every 164.79 years Rotates on its axis about the same speed as Uranus, it completes one rotation in about 18 hou ...
Our Solar System Study Guide 4 grade standard to be tested: S4E2
Our Solar System Study Guide 4 grade standard to be tested: S4E2

... These changes are caused by the way sunlight strikes the Moon as it revolves around Earth. The different ways the Moon looks throughout the month are called the phases of the Moon. The diagram below shows the Moon’s position at each phase. ...
Document
Document

... • A Small World: Pluto is less than half the size of Mercury. • Reclassified: Since its discovery in 1930, Pluto has been called the ninth planet. However, in 2006, it was reclassified as a dwarf planet. ...
Astronomy Review
Astronomy Review

... b. The geocentric theory is flawed and was immediately rejected. c. The geocentric theory is flawed but was accepted for thousands of years. d. The geocentric theory is accepted today. 6. The figure shows the apparent motion of Mars as seen from Earth. What type of motion is occurring? _____________ ...
Mountain Skies March 7 2016
Mountain Skies March 7 2016

SES4U ~ The Formation of Our Solar Systemstudentcopy
SES4U ~ The Formation of Our Solar Systemstudentcopy

... • These grains will settle to the disk midplane since they are heavier than the H and He gas. What happens next is uncertain. – One possibility is that the thin disk of dust is gravitationally unstable, leading to the formation of roughly 1 kilometer size objects known as planetesimals. – Another po ...
Astronomy Book Test Study Guide
Astronomy Book Test Study Guide

... What is the difference between meteors and meteorites? ____  meteors: flash of light in the sky from a falling object burning up in the atmosphere  meteorite: a meteor that reaches the ground  don’t need to know this quesiton  ...
Merit - NZQA
Merit - NZQA

... 2, 500 – 5, 000 k. Their spectral types are G, K or M. White dwarfs are a type of star with a high temperature range, 7, 500 – 30, 000 K. They are not very bright as they are found on the bottom left of the H/ R diagram. Their luminosity is between 10- 10,000 K x dimmer than our sun. White dwarfs ha ...
astronomy - sfox4science
astronomy - sfox4science

... The universe is estimated to be over 10 billion years old. The universe is composed of galaxies, stars, planets, asteroids, comets, and meteors, each having different properties. Our solar system exists within the Milky Way galaxy. The known components of our solar system are the Sun, four terrestri ...
Slide 1
Slide 1

... The Sun is 109 times brighter than Jupiter and 1010 times brighter than the Earth. Therefore, no hope to observe planets directly orbiting stars Well, we may use indirect methods ...
PTYS/ASTR 206 – Section 2 – Spring 2006 Practice Exam 1 Note
PTYS/ASTR 206 – Section 2 – Spring 2006 Practice Exam 1 Note

... A. its distance from the Sun B. its eccentricity C. its size D. the number of moons orbiting around it 20. Why do the planets orbit the Sun in the same direction? A. the Sun captured the planets from a passing star, so the rotation direction is just a consequence of the passing star's trajectory B. ...
here
here

... Start off the activity by making a list of Solar System objects. In most classrooms, students will have already learned the planet names; some students might know about asteroids and comets. Have them name different objects, until the list includes at least: - Sun - 8 planets (Mercury, Venus, Earth, ...
S E N S ` 2 0 0 6
S E N S ` 2 0 0 6

... basic questions arising when somebody think about the origin of Solar system and other planetary systems. But there is not yet any theory confirmed all circumstances. How one planet begins its life? Is it originate from the gas and dust between stars? Or it’s life begins from star’s pieces after som ...
Homework 4 1 Chapter 3 October 4, 2011
Homework 4 1 Chapter 3 October 4, 2011

... two types of planets. They are located closer to the sun and are composed primarily of rock and metal. They have fewer moons than jovian planets and no rings. They also have a solid surface. jovian planets are larger, more massive, and less dense than terrestrial planets. They are composed primarily ...
ASTR101 Unit 14 Assessment Answer Key 1. It is believed that the
ASTR101 Unit 14 Assessment Answer Key 1. It is believed that the

... paradox. If other technological civilizations exist, they would tend to spread out and colonize the galaxy. It is estimated that this would take about a million years, a negligible fraction of the age of the galaxy. Since the galaxy does not seem to be colonized, Fermi argued that other technologica ...
title of lesson plan - Discovery Education
title of lesson plan - Discovery Education

... - What are some of its geological traits? - How many moons does the planet have? - How long is the planet's “day”? How long is its “year”? - What is the surface gravity like on the planet? - How did scientists learn about the planet? - Who first discovered the planet? When? - Over the course of hist ...
Formation of the Solar System
Formation of the Solar System

... A passing star raised a great tide on the Sun and released the gas that later formed the planets due to forces of acceleration. Planetesimal Theory (1900, Forrest Moulton and Thomas Chamberlain) The tidal action of a passing star released matter from the Sun. This matter cooled and by forces of acce ...
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Definition of planet



The definition of planet, since the word was coined by the ancient Greeks, has included within its scope a wide range of celestial bodies. Greek astronomers employed the term asteres planetai (ἀστέρες πλανῆται), ""wandering stars"", for star-like objects which apparently moved over the sky. Over the millennia, the term has included a variety of different objects, from the Sun and the Moon to satellites and asteroids.By the end of the 19th century the word planet, though it had yet to be defined, had become a working term applied only to a small set of objects in the Solar System. After 1992, however, astronomers began to discover many additional objects beyond the orbit of Neptune, as well as hundreds of objects orbiting other stars. These discoveries not only increased the number of potential planets, but also expanded their variety and peculiarity. Some were nearly large enough to be stars, while others were smaller than Earth's moon. These discoveries challenged long-perceived notions of what a planet could be.The issue of a clear definition for planet came to a head in 2005 with the discovery of the trans-Neptunian object Eris, a body more massive than the smallest then-accepted planet, Pluto. In its 2006 response, the International Astronomical Union (IAU), recognised by astronomers as the world body responsible for resolving issues of nomenclature, released its decision on the matter. This definition, which applies only to the Solar System, states that a planet is a body that orbits the Sun, is massive enough for its own gravity to make it round, and has ""cleared its neighbourhood"" of smaller objects around its orbit. Under this new definition, Pluto and the other trans-Neptunian objects do not qualify as planets. The IAU's decision has not resolved all controversies, and while many scientists have accepted the definition, some in the astronomical community have rejected it outright.
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