• Study Resource
  • Explore
    • 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
Planet formation Abstract Megan K Pickett and Andrew J Lim
Planet formation Abstract Megan K Pickett and Andrew J Lim

... not entirely certain, it is on the order of or smaller than the timescale for core-accretion. Thus, by the time a core reaches the trigger mass, the nebular gas may have disappeared. There may be exposed cores of failed gas giants in the universe, but they are not among the extrasolar planets so far ...
FREE Sample Here
FREE Sample Here

... galaxies, then clusters and groups of galaxies, and then the roughly 100 billion individual galaxies, most of which are many thousands of light-years across. Each galaxy contains billions of stars and many or most stars may be orbited by planets. When we say that the universe is expanding, we mean t ...
AMOFMP3_3
AMOFMP3_3

... people have understood why and how bodies move in the cosmic space. Under the action of the Sun, planets move in roughly circular orbits while comets travels in elongated elliptical orbits or, sometimes, along parabolic trajectories. For a space vehicle to be launched to Mars, it is necessary that t ...
test - Scioly.org
test - Scioly.org

... a) Which type of stellar system is this object? b) Why does this object experience dynamic instability in luminosity and size? c) In what wavelength does this object emit most of its radiation? d) Which wavelength(s) is Image D shown in? Specify if you are describing left or right. 26) Which DSO is ...
High resolution spectroscopy: what`s next?
High resolution spectroscopy: what`s next?

... - ESPRESSO as a science generating machine: the goal is to provide scientific data as precise as possible in a short time after the end of an observation. ...
Society News - Bristol Astronomical Society
Society News - Bristol Astronomical Society

... Sitting along the length of Hydra are three small constellations, Corvus, Crater and Sextans. Corvus is the most easterly of the trio and is probably the easiest to identify, four of the brighter stars, beta (β), delta (δ), gamma (γ) and epsilon (ε) Corvi form an irregular quadrilateral which stands ...
Detection Technique for Artificially-Illuminated Objects in the Outer
Detection Technique for Artificially-Illuminated Objects in the Outer

... We first examine the feasibility of this new SETI technique within the Solar System, which offers the best prospects for detecting intrinsically faint sources of light. The flux reaching an observer from any self-luminous source varies according to the familiar inverse square law, but the flux from ...
Detectability of extrasolar moons as gravitational microlenses
Detectability of extrasolar moons as gravitational microlenses

... microlensing Bennett & Rhie (2002) mention the possibility of discovering extrasolar moons similar to our own Moon. Later that year, Han & Han (2002) performed a detailed feasibility study whether microlensing offers the potential to discover an Earth-Moon analogue, but concluded that finite source e ...
Daily Communication Skills
Daily Communication Skills

... answered all parts of the original question. It may also be helpful to have a friend read your work. Example #1: “I know you preferred we don't email you our homework's but my printer is out of ink. Sorry and thank you for excepting it.” (I think the student meant ‘accepting’ but she inadvertently t ...
The Solar System and Beyond
The Solar System and Beyond

... Solar Eclipse Have you ever tried to watch TV with someone standing between you and the screen? You can’t see a thing. The picture from the screen can’t reach your eyes because someone is blocking it. Sometimes the Moon is like that person standing in front of the TV. It moves directly between the S ...
allowed planetary orbits
allowed planetary orbits

... discoveries of other planetary systems occur, such a law could explain the distances of their planets. The ongoing search of extrasolar planets is one of the most attractive fields of research in astrophysics and astronomy. Up to February 11, 2012, 759 exoplanets in 609 extrasolar systems have been ...
Volcanoes and Igneous Activity Earth
Volcanoes and Igneous Activity Earth

... (Earth-centered) view of the universe • Seven heavenly bodies (planetai) • Changed position in sky • The seven wanderers included the • Sun • Moon • Mercury through Saturn (excluding Earth) © 2011 Pearson Education, Inc. ...
Spring 2012 - Union College
Spring 2012 - Union College

... considered plagiarized. In addition, if you take any material from of an internet source, cite the source. Failure to do so will also be considered plagiarism. Late Policy: Labs should be turned in by the deadline given at the time of the lab. There will be a 10% reduction in grade per day late. Not ...
Investigate Planets, Stars, Galaxies, and the Universe
Investigate Planets, Stars, Galaxies, and the Universe

... the city, state, country, and continent. Continue with Earth, the Solar System, the Milky Way Galaxy, the Virgo Supercluster, and the observable universe (the school’s “long address”). This will give students a sense of their place in space. Next, have them watch a video called “The Known Universe” ...
Document
Document

... Contraction of the core is stopped by electron degeneracy. The electrons repel each other as they are pressed closer together and a White Dwarf forms. White Dwarfs have a mass that is less than 1.4 Mo They will shine for a long time but no fusion is taking place. •One teaspoon weighs about 5 tons. ...
Core instability models of giant planet accretion – II. Forming
Core instability models of giant planet accretion – II. Forming

... form several cores in the same disc. Initially we start the simulation with a number N planets,0 of cores through the disc, separated by 10 rH . This could have important consequences on the final distribution of masses and semimajor axis of extrasolar planets, especially for the changes in the dyna ...
Article PDF - IOPscience
Article PDF - IOPscience

Slides - Geophysical Sciences
Slides - Geophysical Sciences

... terrestrial planets) that differ somewhat from those observed in the Solar System. Thus, although there is general confidence that the basic physics of terrestrial planet formation is understood, it is clear that current models do not include all of the ingredients needed to accurately match Solar S ...
ORIGIN AND EVOLUTION OF THE SOLAR SYSTEM: An overview
ORIGIN AND EVOLUTION OF THE SOLAR SYSTEM: An overview

... ∗ The observation of disks around stars ∗ The protoplanetary disk: physical features ∗ Accretion of grains into planetesimals and growth to planets ∗ Planet migration and scattering of residual planetesimals ∗ Some reflections about the discovered extrasolar systems ∗ Residual populations: comets, a ...
White Dwarfs
White Dwarfs

... 9. What unusual property do all higher-mass white dwarfs have? a. They are cooler than lower-mass white dwarfs. b. They are smaller than lower-mass white dwarfs. c. They are less dense than lower-mass white dwarfs. d. They are less luminous than lower-mass white dwarfs. e. All of the above. ...
Quark Presents: Holiday Tour of the Star System Sol
Quark Presents: Holiday Tour of the Star System Sol

... B. Nebula flattens, forms rotating disk, matter concentrates in center C. Disk cools, forms particles that grow into planetesimals - composition varies with temperature/distance from star ...
Jupiter`s Secrets Revealed
Jupiter`s Secrets Revealed

... At about 484 million miles (779 million km) from the Sun, Jupiter is five times farther from the Sun than Earth. Jupiter is the fifth planet from the Sun. (Earth is the third planet from the Sun.) Jupiter is so far away that it takes 12 Earth-years for it to orbit the Sun one time. Jupiter, the giant ...
Geometry of orbits - Harpursville Middle School
Geometry of orbits - Harpursville Middle School

... Any object that orbits another object in space is known as a satellite  Planets ...
Planet formation
Planet formation

... Snow line: 2.7 AU from the Sun, temperatures are low enough that molecules appear in the form of icy grains, and dust grains have sufficiently low temperatures to capture ice molecules in their mantles. The Snow line is crucial for the planet formation process, as ice-covered grains are suggested to ...
Starspots (AIP – Klaus G
Starspots (AIP – Klaus G

< 1 ... 27 28 29 30 31 32 33 34 35 ... 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 © 2025
  • DMCA
  • Privacy
  • Terms
  • Report