PDF-(BOOK)-Astroquizzical: Solving the Cosmic Puzzles of Our Planets, Stars, and Galaxies:

Author : GabrielaLivingston | Published Date : 2022-09-07

Exploring the family tree of the cosmos from humans on Earth to stars and galaxies to the first atoms of the Big Bang with striking color illustrationsLooking up

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(BOOK)-Astroquizzical: Solving the Cosmic Puzzles of Our Planets, Stars, and Galaxies:: Transcript


Exploring the family tree of the cosmos from humans on Earth to stars and galaxies to the first atoms of the Big Bang with striking color illustrationsLooking up at the night sky we see not only stars twinkling in their constellations and planets caught midorbit but our cosmic family tree We are here on Earth because billions of years ago the Big Bang created the atoms that over unimaginable periods of time formed the stars and galaxies Generations of stars that burned exploded or collided long before our planet was formed created the carbon of our bodies and the iron in our blood In Astroquizzical astrophysicist Jillian Scudder takes readers on a curiositydriven journey through outer space traveling back in time from Earth to the stars and galaxies to the cosmic explosions of the Big BangScudder proceedsastroquizzicallyquestion by question answering and explaining such queries as What color is the universe Do all planets spin the same way and How many galaxies are there Along the way she proposes a series of thought experiments including What would happen if we split the sun in half and What happens to time dilation at the speed of light She covers meteors the aurora and the Moon Earths cosmic companion Jupiters stripes and Plutos mountains red dwarfs brown dwarfs and white dwarfs the deaths of stars and the abundance of galaxies and much more Striking color images illustrate astrophysical marvels. Recap. Canvas homework: due on Wednesday. Lab this week: Galaxy Morphology. Campus Observatory. Milky Way galaxy. Stars: . brightnesses. , masses, sizes, compositions, evolution. Interstellar matter: gas, dust. H.-W. Rix IMPRS Galaxies Course March 11, 2011. Goal:. Determine . n. *. (M. *. ,. t. age. ,[Fe. /H],. R. ). . for a population of galaxies. How many stars of what mass and metallicity . formed when and where in galaxies?. 2. The Universe. Th. 3. The Universe is . everything. t. hat exists in space. 4. Galaxies. 5. Galaxies and Shapes (…Cont.). Spiral galaxies:. can be broken down in two categories. Circular spiral - round center. The Cosmic Vision is the paraphrasing name given to the roadmap for scientific space based missions of the European Space Agency (ESA) in the time frame between 2015 and 2025. . Experts are developing this rapidly-growing industry known as "geo-information".. Ms. Cordaro . SMHS . Earth Science. Review/Warm up – Write this in your journal. (Do not fill in the blanks yet!!). A light year = How far _ _ _ _ _ travels in _ _ _ year.. The electromagnetic spectrum is made up of different size _ _ _ _ _ that produce _ _ _ _ _ _ in the form of radiation.. Let’s look back at the rotational velocity equation:. v = (M. interior. G/r). 0.5. The rotational velocity is constant at big r values.. What must we conclude?. The mass interior to the orbit is still increasing. Even after the radius r has gone beyond the last of the stars. It must be increasing in order to hold v constant.. .. 1. First spiral nebula found in 1845 by the Earl of . Rosse. . Speculated it was beyond our Galaxy.. 1920 - "Great Debate" between Shapley and Curtis on whether spiral nebulae were galaxies beyond our own. Settled in 1924 when Edwin . 4.f. Describe the hierarchical structure (stars, cluster, galaxies, galactic clusters) of the universe & examine the expanding universe to include its age & history & the modern techniques (e.g. radio, infrared, ultraviolet & x-ray astronomy) used to measure objects & distances in the universe. (DOK 2). Chapter 2. Stars. Section 1 Vocabulary. Spectrum. Apparent Magnitude. Absolute Magnitude. Light-Year. Parallax. Color of Stars. Red and Yellow. Cool. Blue . Warm. Blue flame hotter than yellow flame. Here’s the Story We’ll Unfold for You…. Hubble’s galaxy classifications: Spirals, . ellipticals. , irregulars. . Structural parts of galaxies: disk, halo, nucleus, bulge. Spiral arms – tracers of star formation. Most single-player games include puzzles. But non-cooperative multiplayer games often do not. Both single-player games and puzzles rely on the game system to provide challenge to the player. Multiplayer games often rely on other players. The “. Cosmic Distance Ladder. ”. Visual. “. Parallax. ”. “. Binocular. Vision”…. Let’s us “see” 3D images . (depth). …but, how to do this to get . Astronomical Distances. ?. “. Stephen Hawking - The Birth of Stars - YouTube. Life Cycle of Stars. Nebula – large cloud of gas and dust spread out in an immense volume. Life Cycle of Stars. Gravity pulls gas and dust together in the densest part of the nebula. Gravity . and Light. Black Holes. What is Dark Matter?. Recap. Midterm . Friday . 11/. 1: summary review sheet posted. Canvas homework : . due Wednesday. Lab this week. Using . gravity to measure . masses.

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