“false-color image” of infrared emission from interstellar cloud of gas and dust (made from space) with magnetic field map from South Pole.

Slides:



Advertisements
Similar presentations
Thermal (blackbody) spectra. Recap No HW this week Project due 11/22 Light /electromagnetic energy –Wavelength, frequency, energy –Electromagnetic spectrum:
Advertisements

The Life Cycle of Stars.
The Birth of Solar Systems A solar system The disk condenses and dissipates Collapse of and interstellar cloud Formation of a protostar and disk.
The Interstellar Medium Astronomy 315 Professor Lee Carkner Lecture 19.
The Birthplace of Stars The space between the stars is not completely empty. Thin clouds of hydrogen and helium, seeded with the “dust” from dying stars,
Imaging Science FundamentalsChester F. Carlson Center for Imaging Science The LASP* at RIT’s Center for Imaging Science *Laboratory for Astronomy in Strange.
Recycling in the Universe
The Milky Way. The Milky Way: Our Home Galaxy What are the different components of the Milky Way? How do we see those components? What does a map of each.
The Use of Infrared Color-Color Plots to Identify Rare Objects in the Galactic Mid-Plane Jessica Fuselier Dr. Robert Benjamin, advisor.
Nebulae Space clouds. What is a Nebula? A nebula is an interstellar cloud of 90% hydrogen, 10% helium, & trace amounts of heavier elements Nebulae are.
Life Cycle of a Star. Stars are born, live, and die. Just like people!
Stellar Evolution: from star birth to star death and back again Prof. David Cohen Dept. of Physics and Astronomy.
Formation of the Solar System  This is a picture of the Eagle Nebula taken by the Hubble Telescope in  A nebula is a cloud of gas and dust in space.
Interstellar Medium (ISM) Read Your Textbook: Foundations of Astronomy –Chapter 11, 12 Homework Problems Chapter 11 –Review Questions: 1, 2, 5, 6 –Review.
 Celestial Sphere  Imagine a sphere that surrounds our planet in which all the stars are attached. This sphere is allowed to rotate freely around the.
Nebular Astrophysics.
CHAPTER 3 (p ) Light. Only a very small range of wavelengths, 400nm to 700nm, are visible to humans. Wavelengths are very small so astronomers use.
Beyond our Solar System. The Milky Way Our solar system is part of a galaxy called the Milky Way Our solar system is part of a galaxy called the Milky.
The Interstellar Medium Chapter 14. Is There Anything Between the Stars? The answer is yes! And that “stuff” forms some of the most beautiful objects.
R2 APODs #3. SN 1006 Supernova remnant A new star, likely the brightest supernova in recorded human history, lit up earth’s sky in the year 1006 AD. The.
Stars are born from a large collection of dusts and gasses that compress under the pressure of gravity, and eventually these dusts and gasses clump in.
Happy Birthday Jodrell Bank! From West Mon School’s Astronomy Club and GCSE Astronomy Classes.
Multiwavelength Astronomy What do different wavelength regimes allow astronomers to “see”?
Nov 27th 2008Southwold and Reydon Society FROM SOUTHWOLD SKIES TO THE UNIVERSE - a journey through space astronomy Michael Rowan-Robinson.
Galaxies of Stars.  By far the nearest star to earth.  A star is a large self-luminous body in space that creates its own radiant energy.  It gets.
By Chloe O.. Nebula The nebula is an interstellar cloud of dust, hydrogen gas, helium gas and plasma. Many nebulae form from the gravitational collapse.
Galaxies Astronomy 115. First, which of the following is a galaxy? Open cluster Globular cluster Nebula Interstellar medium (gas and dust) Supernova remnant.
Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display 1 Announcements: -Extra Credit opportunity this Friday Evergreen.
The Interstellar Medium
Astronomy Chapter Nineteen: Galaxies and the Universe 19.1 Tools of Astronomers 19.2 Stars 19.3 Galaxies and the Universe.
The Milky Way By Maddy Inside The Milky Way might look like this.
Day 11: The Big Bang Theory. Astronomy Intro Grade 9 Science The Expanding Universe The Visible Spectrum –____________________________________ ____________________________________.
Chapter 15: Star Formation and the Interstellar Medium.
Review for Quiz 2. Outline of Part 2 Properties of Stars  Distances, luminosities, spectral types, temperatures, sizes  Binary stars, methods of estimating.
The INTERSTELLAR MEDIUM
Lecture 30: The Milky Way. topics: structure of our Galaxy structure of our Galaxy components of our Galaxy (stars and gas) components of our Galaxy (stars.
The Science behind the Eagle Nebula Image
Radio Waves Interaction With Interstellar Matter
Galaxies GALAXIES Stars are not randomly sprinkled throughout the universe. Most astronomers agree that there are about 100 billion galaxies in the universe,
Harry Kroto image at:
Thessaloniki, Oct 3rd 2009 Cool dusty galaxies: the impact of the Herschel mission Michael Rowan-Robinson Imperial College London.
A Solar System is Born 4/25/14 IN: What do you think the planets are made of? 19-1a pgs
Universe The universe is all existing matter and space considered as a whole. The universe is all existing matter and space considered as a whole.
Basics of Astronomy Casey McNamara.
Stellar Birth By: Scott M & Jeremy B By: Scott M & Jeremy B.
Stars are formed from _______ ___ and ____ coming together due to _______. All stars begin with the _______ ______. What happens then depends on the ____.
Mission Description Well-designed spacecraft and instruments using high energy launches and gravity assists to escape quickly Could be accomplished by.
ASTR Fall Semester Joel E. Tohline, Alumni Professor Office: 247 Nicholson Hall [Slides from Lecture18]
Session 9: Galaxies. The Main Concepts… 1.A galaxy is a large collection of stars, gas and dust. 2.We live in a galaxy called the Milky Way. 3.Our Sun.
Astronomy!!!!. Astronomical Unit kilometers This is the average distance between the earth and the sun.
Universe Tenth Edition
Spiral Galaxy - Canis Venitici We can only see about 1/6 (ca 6000ly) of the way to the Galctic Centre due to scattering by gas and dust in the disk.
Nebula Images. Nebula.
“Twinkle, Twinkle Little Star” The Life Cycle of a Star: Nursery to Neverland Courtney Mutschler Geospace 355
MAY 9, 2016 Daily Question: How do you think scientists classify stars? Materials: Agenda Pencil Notebook/Folder Daily Objective: Today we will learn about.
Space Nebulae & Black Holes. Nebula Derived from the Latin word for "clouds". Nebulae are the basic building blocks of the universe They contain the elements.
The Life Cycle Of Stars.
Star Formation The stuff between the stars Nebulae Giant molecular clouds Collapse of clouds Protostars Reading
“Globular” Clusters: M15: A globular cluster containing about 1 million (old) stars. distance = 10,000 pc radius  25 pc “turn-off age”  12 billion years.
Chapter 25 Beyond Our Solar System
 A nebula is a cloud of gas and dust in space.  Some nebulas are regions where new stars are being formed, while others are the remains of dead or dying.
Galaxies.
Universe Galaxies & Stars Electromagnetic Spectrum
Star Formation & Main-sequence Stars
Multiwavelength Images
Our Place in Space Essential Questions
The Formation and Structure of Stars
Spiral Arms.
Title: 30.1 Galaxies and The Universe
Presentation transcript:

“false-color image” of infrared emission from interstellar cloud of gas and dust (made from space) with magnetic field map from South Pole “false-color image” of infrared emission from interstellar cloud of gas and dust (made from space) with magnetic field map from South Pole the Carina Nebula is an example of a “stellar nursery”: an interstellar cloud where new stars are being formed P med = 2.0 % Dec. offset (degrees)

The Balloon-borne Large Aperture Submillimeter Telescope (BLAST)

The Universe at 300,000 yrs old: (false-color image of microwaves emanating from the entire sky) nothing but gas – no dust; no stars; no life