Supernova Remnant Reveals Magnesium in Abundance Instrument ACISACIS Reference S. Park et al, 2003 Astrophys. J. 592, L41 Distance Estimate 160,000 light.

Slides:

Advertisements

Similar presentations

Life Cycle of Stars. Omega / Swan Nebula (M17) Stars are born from great clouds of gas and dust called Stars are born from great clouds of gas and dust.

Advertisements

Chapter 4 – Stars, Galaxies, and the Universe.  The electromagnetic spectrum includes the entire range of radio waves, infrared radiation, visible light,

The suitability of optical instruments

Introduction to Astrophysics Ronald L. Westra Department Mathematics Maastricht University.

Presented by: Jorge A Campos. Description part of NASA's ﬂeet of "Great Observatories" including: the Hubble Space Telescope the Spitizer Space Telescope.

Spectroscopy. Spectroscopy is complex - but it can be very useful in helping understand how an object like a Star or active galaxy is producing light,

X-ray Properties of Five Galactic SNRs arXiv: Thomas G. Pannuti et al.

A Galaxy Revealed in Multiple Wavelengths 0 Topic: Multiwavelength observations Concepts: Infrared observations, X-ray observations, Optical observations,

Tycho’s SNR – Obs ID 115 ds9 analysis by Matt P. & Leah S. PURPOSE: To use ds9 software to analyze the X-ray spectrum of the Tycho Supernova Remnant, determine.

Matter Unit Learning Goal #1: Recognize the origin and distribution of elements in the universe.

X Ray Astronomy Presented by:- Mohit Shashwat Ankit.

Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 11 The Interstellar Medium.

Intro X-rays From the Sky Chandra X-ray Observatory November, 2003.

X-ray Data Analysis Workshop Group 2 (NCU). Homework Contents Download Chandra data, extract the lightcurve and spectrum. Identify spectral lines. Make.

Light and Telescopes Chapter 5. Radio Interferometry The Very Large Array (VLA): 27 dishes are combined to simulate a large dish of 36 km in diameter.

March 11-13, 2002 Astro-E2 SWG 1 John P. Hughes Rutgers University Some Possible Astro-E2 Studies of Supernova Remnants.

Stellar Explosion has Many Layers Department of Physics National Tsing Hua University G.T. Chen 2006/11/06 Oct. 26, 2006

An X-ray Study of the Bright Supernova Remnant G with XMM-Newton SNRs and PWNe in the Chandra Era Boston, MA – July 8 th, 2009 Daniel Castro,

Intro NASA's Chandra X-ray Observatory Exploring the X-ray Universe 2006.

By Adam and Jack 10 YEARS OF MESMERIZING PHOTOS FROM NASA’S SPITZER SPACE TELESCOPE.

Electromagnetic Spectrum. Different forms of radiation arranged in order according to their wavelength. – Travels through space at 300,000 km/s or 186,000.

Chapter 3 Astronomy TEST REVIEW. WHAT ARE ALL THE FORMS OF ENERGY THAT COME FROM THE SUN? Radio waves Microwaves Infrared Rays (Heat) Visible light Ultraviolet.

Stars, Galaxies, and the Universe.  To understand how telescopes work, its useful to understand the nature of the electromagnetic radiation. Light is.

Key Ideas How are stars formed?

Tycho’s SNR SNR G "To make an apple pie from scratch, you must first invent the universe." ~Carl Sagan.

What We Know About Stars So Far

Ds9 analysis software. Images taken by telescopes that observe at the "invisible" wavelengths are sometimes called "false color images." That is because.

Earth Science Final December 2014 Mrs. Sagala-Riddle.

X-ray Surveys with Space Observatory Khyung Hee University Kim MinBae Park Jisook.

Nov 27th 2008Southwold and Reydon Society FROM SOUTHWOLD SKIES TO THE UNIVERSE - a journey through space astronomy Michael Rowan-Robinson.

The UniverseSection 1 Question of the Day: Jackie used a portable electric drill to remove screws from a broken wooden table. He noticed that the screws.

What are stars? Glencoe: Chapter 26-2 Outline. Astronomy The study of objects and matter outside the Earth’s atmosphere and of their physical and chemical.

The UniverseSection 1 Section 1: The Life and Death of Stars Preview Key Ideas Bellringer What Are Stars? Studying Stars The Life Cycle of Stars.

TeV gamma-ray observation of RCW86 with the CANGAROO-II telescope WATANABE Shio (Kyoto university) for the CANGAROO Collaboration Contents The CANGAROO.

Tour of the Invisible Universe From the Moon to Beyond.

This composite X-ray (blue)/radio (pink) image of the galaxy cluster Abell 400 shows radio jets immersed in a vast cloud of multimillion degree X-ray emitting.

Leaning objectives: Explain that: Elements as heavy as iron are formed inside stars by nuclear fusion. Heavier elements are formed in supernovas. Exploding.

A101 Slide Set: From Supernovae to Planets Drafted by Manning for the SOFIA Team 0 Topic: Supernovase. Concepts: Supernovae, planet formation, infrared.

Astronomy Big Idea: The sun is one of billions of stars in one of billions of galaxies in the universe.

Starter activity Name 5 elements. Name 5 compounds. Name 5 mixtures. Starter activity Name 5 elements. Name 5 compounds. Name 5 mixtures.

2005 K.Corbett Life Cycle of Stars K.Corbett 3 categories of stars  Sun-sized stars  (up to 6 times the size of the sun)  Huge stars  (

The UniverseSection 1 Key Ideas 〉 How are stars formed? 〉 How can we learn about stars if they are so far away? 〉 What natural cycles do stars go through?

Nucleosynthesis and formation of the elements. Cosmic abundance of the elements Mass number.

Intro Exploring the X-ray Universe 2006

Black Holes in Other Galaxies. The giant elliptical galaxy M87 is located 50 million light-years away in the constellation Virgo. By measuring the rotational.

Earth & Space Science March 2015

C. Y. Hui & W. Becker X-Ray Studies of the Central Compact Objects in Puppis-A & RX J Max Planck Institute for Extraterrestrial Physics, Giessenbachstrasse.

PWV LIGHT §Radio Waves §Microwaves §Infrared Light §Visible Light §Ultraviolet Waves §X-Ray Waves §Gamma Waves.

Birth and Death of Stars. Astronomers learn about stars by observing the electromagnetic radiation the stars emit. The most common type of telescope collects.

Part 6:The Sun Photo from

Life of a Star. Nebula A cloud of dust and gas in which new stars form.

Learning target: I can describe black holes Vocabulary: black hole, Agenda: Blackhole notes Blackhole math Stellar evolution activity Learning target DEC.

Astro 101 Slide Set: “Inside-Out” Star Clusters Developed by the Chandra Team 0 Topic: Star clusters Concepts: Stellar evolution, star formation, cluster.

Deep Space and Solar System New Test/New Quiz. Universe Biggest Oldest Galaxy Milky Way Solar System Star Sun PlanetMoon Smallest Youngest.

Aim: Tools of Astronomy Do Now: List 4 tools that a chief may use DO NOW: What is this picture showing you? Notepack 21.

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.

© 2017 Pearson Education, Inc.

Chandra Science Highlight

Multiwavelength Images

A Galaxy Revealed in Multiple Wavelengths

Birth of stars: Clouds of gas collect And form stars.

Using Telescopes to Observe Electromagnetic Radiation in Space

Stars Notes Ch. 28.

STARS Visual Vocabulary.

Life Cycle of Stars 2005 K.Corbett.

Intrinsic in⋅trin⋅sic

1. People have studied the stars for centuries

Chandra Science Highlight

Presentation transcript:

Supernova Remnant Reveals Magnesium in Abundance Instrument ACISACIS Reference S. Park et al, 2003 Astrophys. J. 592, L41 Distance Estimate 160,000 light years (distance to Large Magellanic Cloud) Also Known As SNR Release Date March 24, 2004 Credit NASA/CXC/Penn State/S.Park et al.Scale Each panel is 3.25 arcmin per side Category Supernovas and Supernova RemnantsCoordinates (J2000) RA 05h 25m 26.04s | Dec -65º 59' 06.90“Supernovas and Supernova Remnants Constellation DoradoObservation Date September 15, 2001Dorado Observation Time 8.3 hoursObs. ID 1041 Color Code Energy (Left panel: Red keV, Green keV, Blue keV; Right panel: Pink keV; Cyan/Blue = Mg)

Chandra Inside Glowing Ring “Oxygen and neon are the most abundant elements in the remnant, evidence that the star that exploded was at least ten times as massive as the Sun.” Color Code Energy (Red keV, Green keV, Blue keV) What do you think the red in the image represents?

Celestial Illumination: The X-Ray Glow From An Exploded Star A Chandra “blue blob” Color Code Intensity: X-ray (blue), Optical (green), Radio (red) Inverted Chandra Image of N63A “The fluffy crescent-shaped X-ray features that appear around the edge of the remnant are thought to be fragments of high-speed matter shot out from the star when it exploded, like shrapnel from a bomb. “

Color Code Energy: Red keV, Cyan keV, Blue keV Color Code Energy: Red keV, Green keV, Blue keV

Load Chandra data into ds9 and use “energy cut” to show photons within a certain energy range. Save each energy cut as a separate.tiff file.

Load.tiff files made with ds9 showing “soft”, “medium” and “hard” x-rays into Image J to make final 3-color composite.

ds9 Image J