'10 million years' diaporamas de présentation

The Geologic Column

The Geologic Column. Sean D. Pitman, M.D. June 2006. www.DetectingDesign.com. Features of the Geologic Column. Made of layers of sedimentary rock Layers generally very flat/even relative to each other (may be tilted/warped now) Found generally all over the globe

1.76k views • 158 slides

The Geologic Column

The Geologic Column. Sean D. Pitman, M.D. May 2006. www.DetectingDesign.com. Features of the Geologic Column. Made of layers of sedimentary rock Layers generally very flat/even relative to each other Found generally all over the globe Some areas have missing layers

1.39k views • 120 slides

The Geologic Column

The Geologic Column. Sean D. Pitman, M.D. May 2006. www.DetectingDesign.com. Features of the Geologic Column. Made of layers of sedimentary rock Layers generally very flat/even relative to each other Found generally all over the globe Some areas have missing layers

1.21k views • 120 slides

From Earth we can observe two or three novae each year.

788 views • 65 slides

From Earth we can observe two or three novae each year.

656 views • 65 slides

Sustaining Biodiversity: The Species Approach

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Sustaining Biodiversity: The Species Approach

664 views • 53 slides

An Overview of the Creation/Evolution debate

635 views • 50 slides

Origin of the Solar System

Origin of the Solar System. Stars spew out 1/2 their mass as gas & dust as they die. In the interstellar medium, dust and gas coalesces into clouds. New generations of stars (and their planets, if any) form in these clouds. Nebular theory.

655 views • 50 slides

Origin of the Solar System

Origin of the Solar System. Stars spew out 1/2 their mass as gas & dust as they die. In the interstellar medium, dust and gas coalesces into clouds. New generations of stars (and their planets, if any) form in these clouds. Nebular theory.

562 views • 50 slides

427 views • 42 slides

II OM AMRITESHWARIYAI NAMAHA II

538 views • 35 slides

The Life Cycle of Stars

The Life Cycle of Stars. Do Now. Compare Aldebaran with Sirius B. Which star is hotter? Which is brighter? How do you know?. Agenda. Do Now Mrbrysonscience.wikispaces.com Life Cycle of Stars Simulation Exit Ticket. Stellar Variables. Heat Color Mass Life Cycle Size

425 views • 20 slides

Extinction: past, present, future

Extinction: past, present, future. Material: Gwen Raitt. BCB 341: Principles of Conservation Biology. What is Extinction?. Extinction is the process through which a species or higher taxonomic category ceases to exist.

351 views • 18 slides

Extinction: past, present, future

Extinction: past, present, future. Material: Gwen Raitt. BCB 341: Principles of Conservation Biology. What is Extinction?. Extinction is the process through which a species or higher taxonomic category ceases to exist.

185 views • 18 slides

Lecture 17

Lecture 17. Tectonic-scale Climate Change Text book: Ch. 4, p64-67, 71-80, 82-86. Four Main Processes: Land-ocean spatial configuration: control where ice sheets form

305 views • 15 slides

The Fermi Paradox

The Fermi Paradox. First articulated by Enrico Fermi in 1950. If there is a high possibility for ETL (extra terrestrial life) then where is everybody??? Given: -planets (proto=planetary disks) are common -life originated early on Earth, is easy to evolve

259 views • 10 slides