Lithosphere-The outer layer of Earth's structure made up of the crust and solid ... Asthenosphere-The layer below the lithosphere that is made up of the rest of the ...
Planetesimal: small body from which a planet originated in the development of the solar system. Some planetesimals fused together to form protoplanets. ...
The four protoplanets that became Mercury, Venus, Earth, and Mars were close to the sun. ... The next four protoplanets became Jupiter, Saturn, Uranus, and Neptune. ...
Planetesimals in the early solar system collide and accrete to form protoplanets. ... Planetesimal: small ~1km rocky asteroid-like objects in early solar system ...
Runaway growth in the Asteroid belt in the presence of Jupiter ... Giant impact phase. A few tens of mars-size protoplanets form after the runaway phase ...
Long term evolution of circumstellar discs: DM Tau and GM Aur Ricardo Hueso (*) & Tristan Guillot Laboratoire Cassini, Observatoire de la C te d Azur, Nice, France
Origin of Our Solar System TEK Objective 5: Earth in space and time. The student understands the solar nebular accretionary disk model. The student is expected to ...
Origin of Our Solar System TEK Objective 5: Earth in space and time. The student understands the solar nebular accretionary disk model. The student is expected to: a ...
Formation of the Solar System ... * The big bang spread matter throughout the expanding universe. Some of this matter gathered into clouds of dust and gas.
Structure of the Sun and Solar Activity Structure of the Sun and Solar Activity The Inner Zone a. Radiative zone. Energy moves to the outside by Electromagnetic ...
Extrasolar Planets The first planet detected ... Rules of chemistry Observations of rock ... Asteroids Some asteroids appear to be rubble piles of broken ...
The Origin of Earth Six facts must be considered when formulating a hypothesis about the origin of Earth: Planets revolve around the sun in the same direction.
... Planet Formation. Hilke Schlichting. Advisor: Re em Sari. Planet ... 2-body Problem. Conservation of Energy & Momentum. Integration over b. Fdf=2pSGM. b. M ...
The interaction of a giant planet with a disc with MHD turbulence II: The interaction of the planet with the disc Papaloizou & Nelson 2003, MNRAS 339 (4), 993
Three orders of magnitude in distance. Nine orders of magnitude in volume! ... orders of magnitude in distance. Nine orders of magnitude in volume! (Grundy ...
Refraction of seismic waves. Density of the entire planet. Gravity (mass) of entire planet ... Earth: The Unfinished Planet. Earth continues to lose heat ...
0 The Origin of the Solar System Planetary Orbits Neptune Uranus Saturn Jupiter Mars Earth Venus Mercury All planets in almost circular (elliptical) orbits around the ...
In a dense molecular cloud far, far away proposed originally by Kant, Laplace, and others in the 1700's solar system formed from a nebula (cloud of interstellar gas ...
The universe began as hot, dense matter that was concentrated into a ... English scientist Sir Isaac Newton explained why planets stay in orbit (17th century) ...
The Origin of Our Solar System Chapter Eight Introduction To Modern Astronomy I: Solar System Constrains of Models Any theoretical model must be able to explain the ...
Formation of the Solar System Solar System Formation of the Solar System preview of the big bang theory the interstellar medium nebular condensation theories what s ...
... that more massive Jupiter and Saturn attracted much of the gas ... of Saturn - NASA ... nasa.gov/photo_gallery/photogallery-saturn.html#satellites ...
Migration occurs by tidal interaction between planet and disk: ... Migration of a Jovian planet over 10 Myr. Note extent of gap opened by planet once inside dead zone. ...
* Moons Pandora and Prometheus ... 1994 Jupiter is orbited by four large moons and tens of small ones Io s surface is sculpted by volcanic activity Io s ...
Protoplanetary disks are thought to be the progenitors of planetary systems. ... If tidal torques dominate, a large annular gap in the disk opens up around the ...
Keynote speaker: Ann Grandfield, program manager for the Dawn spacecraft at ... Dawn's mission to investigate Ceres and Vesta, two of the largest and oldest asteroids. ...
What is the subject of the act 'Formation and evolution of OUR Jovian planets' ... Strong disequilibrium phases can be anyhow possible (Wuchterl, 1993), and shock ...
Planetas extrasolares e nuvens moleculares Horacio Dottori Dpto. Astronomia IF-UFRGS SETI (Vida vs. Vida Inteligente) Como podemos comprobar en la propia Tierra, hay ...
Hot near center, cooler further away. material can condensate if cool enough ... now mostly look for wobble of Star (Doppler shift) due to gravity of planets ...
To Guide the Habitable Planet Search (TPF, Darwin), we Need to Know: ... Most of Earth's water was accreted during formation from bodies past snow line ...
Accretion of Planets Bill Hartmann Star & Planet Formation Minicourse, U of T Astronomy Dept. Lecture 5 - Ed Thommes Overview Start with planetesimals: km-size bodies ...
What is a Planet? Physical Geology (1) A 'planet'1 is a celestial body that (a) is in orbit around the Sun, (b) has ... body forces so that it assumes a ...
To guide the Habitable Planet Search (TPF, Darwin), we need to know: ... Most of Earth's water was accreted during formation from bodies past snow line ...
Title: The Milky Way Author: Markus Boettcher Last modified by: roberts Created Date: 2/23/2003 4:28:17 AM Document presentation format: On-screen Show
Callisto wears the scars of a huge asteroid impact ... Titan is Saturn's largest moon ... Neptune's largest moon, Tritan, was probably captured by Neptune's gravity ...
Terdapat aktivitas vulkanisme (intrusi & ekstrusi) Merupakan daerah hiposentra gempa dangkal dan dalam Lempeng dasar samudera menujam ke bawah lempeng benua (zona ...
Universe. Eighth Edition. Roger A. Freedman William J. Kaufmann III. CHAPTER 8 ... Its believed that some of the heavier elements was once inside other stars. ...
Title: Building the Terrestrial Planets: Constraining Accretion in the Inner Solar System Author: MacP91 LASP Last modified by: Sean Raymond Created Date
What caused the orderly patterns of motion in our solar system? ... birth region of planets Dust is continuously replenished by disruptive collisions between ...
Chapter 1 Introduction to Planet Earth Essentials of Oceanography 7th Edition * * Geography of the oceans Earth s oceans: Cover 70.8% of Earth s surface Are ...