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The Origin of the Solar System

The Origin of the Solar System

The Origin of the Solar System. Lecture 13. Announcements. Homework 7 due now Homework 8 – Due Monday, March 26 Unit 32: RQ1, TY1, 3 Unit 33: RQ4, TY1, 2, 3 Unit 35: RQ4, TY1, 3 Unit 39: P3, TY1 Lab Wednesday will be off-campus for telescope observing.

By PamelaLan
(724 views)

Fundamental Physics at ESA

Fundamental Physics at ESA

Fundamental Physics at ESA. J. Clavel ESA Science Directorate. Overview. Two dedicated missions in the Science Directorate LISA Pathfinder LISA Missions with aspects of FP in the Science Directorate Gaia Planck Mission concepts under assessment Fundamental Physics Explorer

By betty_james
(261 views)

Elements of the Solar System, Exploring Extrosolar Planets and Evolution of Planetary Systems

Elements of the Solar System, Exploring Extrosolar Planets and Evolution of Planetary Systems

Elements of the Solar System, Exploring Extrosolar Planets and Evolution of Planetary Systems. FIZ466, İTÜ. The Astronomical Unit (AU). The appropriate length unit for studying the Solar System is AU AU is the average distance between the Sun and the Earth

By cissy
(287 views)

About Omics Group

About Omics Group

About Omics Group.

By kareem
(146 views)

Minor Members of the Solar System

Minor Members of the Solar System

Minor Members of the Solar System. Chapter 23, Section 4. Asteroids. Asteroid – small rocky bodies that have been likened to “flying mountains” Most asteroids lie between the orbits of Mars and Jupiter. They have orbital periods of 3 to 6 years.

By thurston
(2697 views)

The Origin of the Solar System

The Origin of the Solar System

The Origin of the Solar System. Lecture 13. Announcements. Homework 7 due now Homework 8 – Due Monday, March 26 Unit 32: RQ1, TY1, 3 Unit 33: RQ4, TY1, 2, 3 Unit 35: RQ4, TY1, 3 Unit 39: P3, TY1 Lab Wednesday will be off-campus for telescope observing.

By kaya
(175 views)

Lecture 13 Electromagnetic Waves Ch. 33

Lecture 13 Electromagnetic Waves Ch. 33

Lecture 13 Electromagnetic Waves Ch. 33. Cartoon Opening Demo Topics Electromagnetic waves Traveling E/M wave - Induced electric and induced magnetic amplitudes Plane waves and spherical waves Energy transport snd Intensity of a wave Poynting vector Radiation Pressure produced by E/M wave

By amara
(425 views)

GRB

GRB

GRB. Useful reviews: Waxman astro-ph/0103186 Ghisellini astro-ph/0111584 Piran astro-ph/0405503 Meszaros astro-ph/0605208 Useful links http://www-astro.physics.ox.ac.uk/~garret/teaching/ http://www.cv.nrao.edu/course/astr534/. Theory and observations.

By lou
(102 views)

Gravitational Waves Generating Phenomena and Detection

Gravitational Waves Generating Phenomena and Detection

Gravitational Waves Generating Phenomena and Detection. Marino Maiorino. Table of Contents. Basics of Gravitational Waves (GW) GW’s propagation GW’s generation Low Frequency Astrophysical Phenomena High Frequency Astrophysical Phenomena Basics of Gravitational Waves Detection

By wind
(213 views)

The Origin of the Solar System

The Origin of the Solar System

0. The Origin of the Solar System. Chapter 16:. 0. The Great Chain of Origins: Early Hypotheses. 1) Catastrophic hypotheses Example: passing star hypothesis: . Star passing the sun closely tore material out of the sun, from which planets could form (no longer considered).

By Jims
(248 views)

Hot Cores and High Mass star formation

Hot Cores and High Mass star formation

Hot Cores and High Mass star formation. Malcolm Walmsley (Arcetri Observatory). Orion in NH3 (Mid 70s). Al Barrett and collaborators at MIT noticed a blue shifted component in their NH3 line profiles towards Orion-KL It was most apparent in the highly excited transitions tracing hot gas.

By tryphena
(132 views)

Lecture 23

Lecture 23

Physics 2102 Jonathan Dowling. Lecture 23. AC Circuits: Power Electromagnetic waves. Driven RLC Circuits: Summary. E = E m sin(  d t); I = I m sin(  d t -  ). X C =1/( w d C), X L = w d L . At resonance: X L =X C ; w d 2 =1/LC; f =0; Z =R (minimum), E m =E m /R (maximum) .

By bowen
(128 views)

The world is not coming to an end in 2012.

The world is not coming to an end in 2012.

The world is not coming to an end in 2012.

By adamma
(61 views)

Single Molecule Studies of DNA Mechanics with Optical Tweezers

Single Molecule Studies of DNA Mechanics with Optical Tweezers

Single Molecule Studies of DNA Mechanics with Optical Tweezers. Mustafa Yorulmaz Koç University , Material Science and Engineering. Outline. Motivation Methods Models Aims Basics of optical tweezers Physics beyond optical trapping Experimental part Force-extension curves Results

By bradford
(253 views)

Lives and Deaths of Stars

Lives and Deaths of Stars

Lives and Deaths of Stars. Milky Way Galaxy. 28,000 light years. 200 billion stars. 100 billion galaxies in the observable Universe. 10 day exposure photo!. Over 1500 galaxies in a spot 1/30 the diameter of the Moon. Farthest and oldest objects are 12-13 billion light years away!.

By elmer
(1 views)

Hydrogen burning under extreme conditions

Hydrogen burning under extreme conditions

Hydrogen burning under extreme conditions. Scenarios:. Hot bottom burning in massive AGB stars (> 4 solar masses) . (T 9 ~ 0.08). Nova explosions on accreting white dwarfs. (T 9 ~ 0.4). X-ray bursts on accreting neutron stars. (T 9 ~ 2). accretion disks around low mass black holes ?

By lester
(144 views)

Precise Orbit Determination of the GIOVE Satellites

Precise Orbit Determination of the GIOVE Satellites

Precise Orbit Determination of the GIOVE Satellites. Peter Steigenberger, Urs Hugentobler Technische Universität München. Oliver Montenbruck, André Hauschild , Deutsches Zentrum für Luft- und Raumfahrt, Oberpfaffenhofen. Introduction. G alileo I n O rbit V alidation E lement.

By rudolph
(124 views)

Rendezvous with a Comet

Rendezvous with a Comet

Rendezvous with a Comet. Courtesy: Pat Rawlings - Deep Impact -NASA & JPL. Introduction. The history of comet watching dates back to 1000 BC from the Chinese records and Chaldea, a place in present Iraq. Comets have been regarded as omen, even as recently as 1986. Battle of Hastings - 1066

By jayme
(119 views)

The Threat of Parametric Instabilities in Advanced Laser Interferometer Gravitational Wave Detectors

The Threat of Parametric Instabilities in Advanced Laser Interferometer Gravitational Wave Detectors

AIGO. The Threat of Parametric Instabilities in Advanced Laser Interferometer Gravitational Wave Detectors. Li Ju Chunnong Zhao Jerome Degallaix Slavomir Gras Pablo Barriga David Blair. Contents. Parametric instabilities Minefield for Advanced Detectors Suppression of instabilities

By asis
(96 views)

Thermal & Radiometric Forces

Thermal & Radiometric Forces

. Hot. Cold. d p. T 1 , c 1. T 2 , c 2. Thermal & Radiometric Forces. Reading: Chap. 8. http://aerosol.ees.ufl.edu/Thermophoresis/section01.html. Thermophoresis: Particle motion in a temperature gradient, from a hotter to a colder region. Molecular impacts on a particle

By grant
(119 views)

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