'Entire sky' presentation slideshows

Aristotle (384-322 BC) showed Earth is round, way before Columbus!

969 views • 81 slides

Dark Energy and Supernovae

Dark Energy and Supernovae. Wendy Freedman Carnegie Observatories, Pasadena CA Beyond Einstein, May 13, 2004. Type Ia Supernovae for Cosmology. Advantages: small dispersion single objects (simpler than galaxies) can be observed over wide z range . Challenges: dust (gray dust)

765 views • 64 slides

How Do We Predict Weather? General Weather Information Clouds, rain, thunderstorms, etc.

735 views • 57 slides

Clouds

Clouds. Earth & Space Science Grade 4 By: Ashlee Gray. Click on the arrow to begin!. Introduction.

675 views • 57 slides

Weather

836 views • 53 slides

Universal access to the sky: amateurs, professionals, and the virtual observatory

478 views • 38 slides

??? ???? ?????? ??????

??? ???? ?????? ??????. Introduction to the Sira of Our Habib PBOH Lesson Plan The Meccan Period Class Two Imam Ibrahim A. Rahim Sister Mariam N. Ismail TA. Week #2 The boy who was a shepherd. The man the merchant and the moral lessons in between. Group Presentation:

508 views • 38 slides

ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe

ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe. Prof. D.C. Richardson Sections 0101-0106. How can we know what the universe was like in the past?. Light travels at a finite speed ( c = 300,000 km/s). Thus, we see objects as they were in the past:

822 views • 37 slides

ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe

ASTR100 (Spring 2008) Introduction to Astronomy Discovering the Universe. Prof. D.C. Richardson Sections 0101-0106. How can we know what the universe was like in the past?. Light travels at a finite speed ( c = 300,000 km/s). Thus, we see objects as they were in the past:

605 views • 37 slides

The World of the Angels

659 views • 36 slides

Latitude and Longitude

A model of the celestial sphere shows the patterns of the stars, the borders of the 88 official constellations, the ecliptic, and the celestial equator and poles. Latitude and Longitude.

915 views • 30 slides

Using the Electromagnetic Spectrum

Using the Electromagnetic Spectrum. Objective: Students will explain the need for observing the universe using different wavelengths and will be able to relate wavelength, frequency, and energy. The Electromagnetic Spectrum. Why look at the Universe through different wavelengths?.

408 views • 28 slides

A Web service for Distributed Covariance Computation on Astronomy Catalogs

A Web service for Distributed Covariance Computation on Astronomy Catalogs. Presented by Haimonti Dutta CMSC 691D. ROADMAP Background Information Interesting Astronomy Data Mining Problems What has / not been done (Literature review) My project objectives

300 views • 20 slides

Clouds! By: Alexie Canik

Clouds! By: Alexie Canik. I Hope You Enjoy My Power Point! ?. Types of Clouds. Cirrus Cirrocumulus Cirrostratus Altocumulus Altostratus Stratus Stratocumulus Nimbostratus. Cumulus Cumulonimbus Lenticular Kelvin-Helmholtz Mammatus Contrails.

363 views • 17 slides

249 views • 15 slides

source: Alex Szalay

266 views • 12 slides

Weather and climate

Weather and climate. Rafaela Diaz 8E. Difference between weather and climate. The difference between weather and climate is a measure of time. Weather is what conditions of the atmosphere are over a short period of time. Climate is how the atmosphere "behaves" over long periods of time.

499 views • 11 slides

What's hiding in the night sky???

What's hiding in the night sky???. By Claumetria Jones. ED 498.

219 views • 11 slides

Climate vs. Weather

Climate vs. Weather. Climate: Average weather conditions for an area over a long period of time. Weather: condition of the atmosphere at any given time. What effects Climate? . Solar Energy/Intensity Global Wind Patterns Ocean Currents Topography.

223 views • 9 slides

Clouds

423 views • 9 slides