'Red dwarf' diaporamas de présentation

EARTH SCIENCE FINAL

1.85k views • 170 slides

INTO The DARK: the FAR FUTURE of OUR universe

INTO The DARK: the FAR FUTURE of OUR universe. Fred C. Adams University of Michigan. The Copernican Time Principle. The current cosmological epoch has no special significance. Interesting physics processes will continue to take place in the future, despite decreasingly energy levels.

749 views • 58 slides

Discovering the Universe

Discovering the Universe. Table of Contents. A Multimedia Project by Dennis Culver. Credits. Table of Contents. Planets. Stars. Galaxies. Moons. Other. Planets. Mercury. Venus. Earth. Mars. Jupiter. Saturn. Uranus. Neptune. Pluto. Comparison Graph. Mercury.

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The Life Cycle of Stars

The Life Cycle of Stars. From birth, to death , to live, once again. Life Cycle. Very Small Sized Star. Nebula Protostar Brown dwarf. Life Cycle. Eagle Nebula. Protostar. Brown dwarf. Small Sized Star. Nebula Protostar Red Dwarf White Dwarf. Life Cycle. Omega Nebula. Protostar.

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Calculate the net force acting on a particle

Mass transfer in a binary system. Calculate the net force acting on a particle . Gravitational potential in the corotating frame. Mass Transfer in Binary Stars. In a binary system, each star controls a finite region of space, bounded by the Roche Lobes (or Roche surfaces ).

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Light Curves of the Dwarf Nova U Gem: A Diagnostic of Accretion Disk Evolution

Light Curves of the Dwarf Nova U Gem: A Diagnostic of Accretion Disk Evolution. Larry Molnar Calvin College Grand Rapids, Michigan. Outline. Calvin-Rehoboth Twin Telescopes Project Dwarf Novae U Gem Preliminary Light Curves. Calvin-Rehoboth Twin Telescope Project. NSF-CCLI funding

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Astronomy 12 Stars, Stellar Evolution, and High Energy Astrophysics

Astronomy 12 Stars, Stellar Evolution, and High Energy Astrophysics - Stan Woosley The Nature of Astronomy The study of objects beyond earth (here with emphasis on stars and physics)

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U2: Astronomy - Measuring Space Distances

U2: Astronomy - Measuring Space Distances . FLIP LESSON. On the Move.

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Lives of Stars Section 3

Lives of Stars Section 3. Nebula. Large cloud of gas and dust spread out in an immense volume All stars are born in a nebula , large cloud of gas and dust. . Protostar. Gas and dust begin to collect due to gravity . Once enough material has formed together, a protostar is created.

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Goal: To understand the lifetime of a star and how the mass of a star determines its lifetime

Goal: To understand the lifetime of a star and how the mass of a star determines its lifetime. Objectives: To learn what defines a Main sequence star To understand why Energy is important for a star To examine the Cores or stars To understand what determines the Lifetime of a star

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The Lives of Stars

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Stars and Galaxies

Stars and Galaxies. By Jake Koch-Gallup, Matthew Yorro, Aidan McCaul, Brigitte Bazie, and Laura Lill. Galaxies and stars.

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Quantum levitation anyone?

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Sun and other Stars

Sun and other Stars. By: Kennedy Howard Presley Wilson Tyra Gilbert. What is the sun?.

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YTV

YTV. Beginning. YTV was launched on September 1, 1988 with a preview special hosted by John Candy It was one of the major cable networks on Canadian TV. Programming Back Then.

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Miss Plascak

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The Stars

The Stars. S4E1 . Students will compare and contrast the physical attributes of stars & star patterns a. Recognize the physical attributes of stars in the night sky such as number, size, color and patterns.

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