• Study Resource
  • Explore Categories
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
Chapter 8 The Parts of the Solar System Section 8.1 The Sun
Chapter 8 The Parts of the Solar System Section 8.1 The Sun

... The sun does not have a solid surface, but the gases of the photosphere are thick enough to be visible. When you look at an image of the sun, you are looking at the photosphere. It is considered to be the sun’s surface layer. The Chromosphere During a total solar eclipse, the moon blocks light from ...
Lecture 4
Lecture 4

... • Sun plus 8 (or 9 with Pluto) planets many of which have moons • plus “debris”: comets, asteroids, meteors, etc • We’ll go over historical understanding of motion (which is “complicated” when viewed from the Earth) and later look at Solar System formation, planetary atmospheres, and planets discove ...
Slide 1
Slide 1

... pro = first ...
Chapter 3: Galileo, Newton, and Einstein
Chapter 3: Galileo, Newton, and Einstein

... 1. Stars are so far away that stellar parallax is too small to notice with the naked eye 2. Earth does not orbit Sun; it is at the bottom of the universe With rare exceptions such as Aristarchus, the Greeks rejected the correct explanation (1) because they did not think the stars could be that far a ...
Winter 2006 - Cornell Astronomy
Winter 2006 - Cornell Astronomy

... Ever since the discovery in 1992 of a massive belt of small bodies beyond Neptune (the Kuiper Belt or the trans-Neptunian region), the status of Pluto has been in serious question. With more than a thousand trans-Neptunian objects discovered to date, it has become increasingly clear that Pluto is no ...
Light and Telescopes - Otterbein University
Light and Telescopes - Otterbein University

... – Observed mountains on the Moon, suggesting that the Earth is not unique – Sunspots; suggests that celestial bodies are not perfect and can change – Observed four moons of Jupiter; showed that not all bodies orbit Earth – Observed phases of Venus (and correlation of apparent size and phase); eviden ...
planet research paper
planet research paper

... Rotation on its Axis: How long does it take for your planet to rotate on its own axis? (This is one day on your planet.) Size: How big is your planet? How does it rate in terms of the other planets in terms of size (is it the biggest, the smallest)? What is your planet's mass? Gravity: What is the f ...
Chapter 15 The Formation of Planetary Systems
Chapter 15 The Formation of Planetary Systems

... Current record holder, until last year. ...
The Planets Testify of the Creator
The Planets Testify of the Creator

... be thought of as an continuous repetition of days numbered from 1 to 7. These 9 "lords" may have originally referred to the Moon, Mercury,Venus, Sun, Mars, Jupiter, Saturn, Uranus, and Neptune, even as our seven­day week is associated with the first seven in that series.[4] Pluto, the other so­calle ...
Sky Study Guide_1
Sky Study Guide_1

... Category Distance from Sun (Millions of Km) Period of revolution Diameter (km) Atmosphere ...
PHASES OF THE MOON
PHASES OF THE MOON

... Category Distance from Sun (Millions of Km) Period of revolution Diameter (km) Atmosphere ...
leo 1. episode 1
leo 1. episode 1

... It would be easy to imagine that the same thing would happen with Antares and that said planet would be a satellite of the star Antares. And yet, such is not the case: Antares is a red giant star with a diameter 500 times bigger than our Sun. It has no habitable worlds. The target planet for Project ...
Phys 1830: Lecture 33 - University of Manitoba Physics Department
Phys 1830: Lecture 33 - University of Manitoba Physics Department

PHYS103 Hour Exam No. 2 Preview 2 Page: 1 1 According to
PHYS103 Hour Exam No. 2 Preview 2 Page: 1 1 According to

... 1 According to Newton’s Law of Gravity, the gravitational attraction of the Earth for other objects, such as the Moon, apples on trees and space shuttles in low earth orbit, a. is smaller for objects farther from the Earth but never vanishes entirely. b. is the same no matter where those objects are ...
Revolution: Earth`s orbit around the Sun
Revolution: Earth`s orbit around the Sun

... Earth rotates (southern hemisphere) The Moon Phases of the Moon – varying amounts of the moon’s surface that is seen from Earth  Caused by the Moon’s revolution around the Earth  Perigee – nearest (closest) point  Apogee – farthest point o Moon’s orbit is elliptical  5 degree difference in plane ...
study-notes-for-2016-2017-1st-qtr-exam
study-notes-for-2016-2017-1st-qtr-exam

... Motions within Our Solar System Cause of Day & Night Day and Night occur on Earth because of the rotation of the Earth on its axis. 1 Earth day lasts 24 hours. The length of daylight and dark vary depending on the season and a person’s location on Earth. Cause of Seasons Seasons on Earth are cause ...
File - IGS Intro Materials
File - IGS Intro Materials

... • A comet, is composed of dust and rock particles mixed with frozen water, methane, and ammonia. • As a comet approaches the Sun, it begins to vaporize. The vaporized dust and gases form a bright cloud called a coma around the nucleus. The solar wind pushes on the vaporized coma, forming a tail that ...
What Makes a Planet Habitable?
What Makes a Planet Habitable?

... problems in current habitability research. An atmosphere of the type suspected for the young Earth, and definitely the present-day atmosphere, would not have succeeded in keeping the average Earth’s surface temperature above the freezing point during the first 2.5 billion years of its life; the requ ...
The Jovian Planets
The Jovian Planets

... Giant storm – twice as wide as the Earth Somewhat like a hurricane – High pressure rather than low. ...
Origin of the Elements and the Earth
Origin of the Elements and the Earth

... cloud of gas probably blown to us by a group of super-giants. It is called the Local Interstellar Cloud(LIC) or the ...
Our Solar System
Our Solar System

... Pluto’s orbit, is about 40 times the diameter of Earth’s orbit around the Sun. • If we consider also the most distant Kuiper Belt objects discovered to date, up to 90 times Earth’s distance from the Sun, the diameter of our solar system would be increased accordingly. • However, the distance to the ...
Saturn Entry Probe Science Objectives
Saturn Entry Probe Science Objectives

... Giant Planet Comparative Planetology Data Set Needed for Meaningful Comparisons ...
Life on hot Jupiters
Life on hot Jupiters

... Information about Hot Jupiters • Hot Jupiters have some common characteristics: • They have a much greater chance of transiting their star as seen from Earth than planets of the same mass in larger orbits. • They are all thought to have migrated to their present positions because there would not ha ...
Educator Guide: Starlab (Grades 6-8)
Educator Guide: Starlab (Grades 6-8)

... students participating in the Starlab program to learn, though prior study of  these words is not required for student participation.   Asterism – a recognizable pattern of stars that is not an officially recognized  constellation, i.e. the Big and Little Dippers (as they are smaller parts of larger ...
brock university answers
brock university answers

... (d) * nuclear reactions that convert hydrogen into helium. 12. The distance from the Sun to Neptune, the farthest known planet, is about (a) * 30 AU. (b) 30 light years. (c) 30 parsecs. (d) 30 kWh. 13. The Sun is (a) significantly larger than average stars. (b) significantly smaller than average sta ...
< 1 ... 123 124 125 126 127 128 129 130 131 ... 338 >

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.
  • studyres.com © 2026
  • DMCA
  • Privacy
  • Terms
  • Report