'Planetary' presentation slideshows

Pictures for life death of solar system

Pictures for life death of solar system. Nebulas. Nebula. A cloud of dust and gas Mostly hydrogen and helium gas, 2% heavier particles Dark (dust) and light (gas) Irregularly shaped, dust and gas moving around

834 views • 68 slides

NEW DEVELOPMENTSIN AGRICULTURAL EQUIPMENT TRACTORS

NEW DEVELOPMENTSIN AGRICULTURAL EQUIPMENT TRACTORS. R. T. Schuler National AgrAbility Project University of Wisconsin - Madison. November 14 , 2006. Tractors. Guidance and Auto-Steer Global Positioning System Guidance Auto-Steer Autonomous Transmissions Number of gears/speeds

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545 views • 33 slides

Automatic Transmission Fundamentals

Automatic Transmission Fundamentals. Chapter 73. Objectives. Identify the basic parts of an automatic transmission Describe the operation of the major sections of an automatic transmission Explain how automatic transmissions shift gears

1.13k views • 32 slides

Stellar Death

Stellar Death. Core. He. H burning shell. The Sun in Five Billion Years. Main Sequence Evolution. Hydrogen is depleted in the last fusion zone Reaction rate falls Core can no longer support its weight core shrinks Temperature in the core increases Extra energy produced to -

398 views • 29 slides

Synoptic-Scale Weather Systems of the Intermountain West

Synoptic-Scale Weather Systems of the Intermountain West. Dr. David Schultz NOAA/National Severe Storms Laboratory Norman, Oklahoma schultz@nssl.noaa.gov http://www.nssl.noaa.gov/~schultz. What Might Be the Forecasting Challenges in February 2002?.

462 views • 28 slides

14a. Uranus & Neptune

14a. Uranus & Neptune. The discovery of Uranus & Neptune Uranus is oddly tilted & nearly featureless Neptune is cold & blue Uranus & Neptune are like yet dislike Jupiter The magnetic fields of Uranus & Neptune The dark rings of Uranus & Neptune Ancient tidal heating in some Uranian moons

500 views • 28 slides

Planetary Imaging

Webcam. Planetary Imaging. Agenda. Why Planetary Imaging ? Planetary Webcams Webcam Modification Taking a Planetary Image Taking Planetary Video Processing The Video Animations. Why Planetary Imaging?. It can be done from every location It can be done almost all month

606 views • 26 slides

One World Centre educating for a just and sustainable world

One World Centre educating for a just and sustainable world. Rockstrom, Sachs, Ohman & Schmit-Traub (2013) Sustainable Development & Planetary Boundaries.

410 views • 25 slides

Life of a star

Nicholas Kellogg & Annessa strickland . Life of a star. Life of a star. We can see the stages of a star. Even though are life's are much shorter than that of a human. At the end of a stars life it will most likely resolve in an explosion. Life of a star. Life of a star.

445 views • 20 slides

What do you think of when you look at the night sky?

What do you think of when you look at the night sky?. http://www.astro.ufl.edu/~lada/ast3018/lectures/ast3018lecturestarform.pdf. What is Space?. Not really empty Stars, planets, etc. Interstellar medium Dust and Gas Nebulas. Orion Nebula

292 views • 20 slides

Manual Transmission Fundamentals

Manual Transmission Fundamentals. Chapter 71. Objectives. Describe the relationship between gears and torque Understand the basic types of gears Calculate gear ratios Trace the power flow through three-, four-, and five-speed transmissions Name all of the transmission parts. Introduction.

649 views • 20 slides

Lifecycle of Stars

Lifecycle of Stars. By: Mark and Jacob . Nebula. A nebula is a cloud of gas and dust in space. Nebulae are the birthplaces of stars. There are different types of nebula.

307 views • 19 slides

Toward an Exoplanet Roadmap.

Toward an Exoplanet Roadmap. ExoPAG 8 Meeting Denver, CO October 5+6, 2012 Scott Gaudi. Goal. To develop a holistic, broad, unified, and coherent exoplanet roadmap for the next 5-10 years, with community consensus, focusing on areas where NASA can contribute. Why?.

226 views • 14 slides

492 views • 13 slides

J ovian E xtinction E vents JPL Confirmation of JEE Data.

220 views • 13 slides

Wind and the Coriolis Effect

Wind and the Coriolis Effect. Air pressure differences cause the movement of air Air moving parallel to the ground is called wind Air moving up or down is called a current. Air generally moves from the poles to the equator, this is because air flows from high pressure to low pressure

363 views • 11 slides

Atmospheric Physics at UMBC physics.umbc.edu (mcmillan@umbc.edu)

Offering M.S. and Ph.D. degrees Research areas: remote sensing of aerosols, gases, clouds, and transport modeling 4 core faculty, 20 research faculty, 2 Joint Centers with NASA Goddard (100+ researchers), and 15 graduate students.

278 views • 9 slides

prompt6b

Planetary Formation based on http://people.highline.edu/iglozman/classes/astronotes/solsys_form.htm .

183 views • 7 slides

Timing of Convection Initiation During the WETANC-LBA

145 views • 1 slides