OUR UNIVERSE : AN EXPANDING MYSTERY

Slides:



Advertisements
Similar presentations
Chapter 18: Cosmology For a humorous approach to quarks, check out the Jefferson Lab’s game.  In Looking for the Top Quark, each player receives six quarks.
Advertisements

UNIVERSE CHAPTER BIG BANG The big bang theory is the main cosmological model for the earliest known time of the Universe. It shows us how the universe.
The Electromagnetic Spectrum
Objectives Distinguish the different models of the universe.
Astronomy Ch 20 The Universe What is the universe? What is the universe? Sum of all space, matter, and energy past, present, future
THE BIG BANG THEORY A video on the Big Bang theory click here.
Multiwavelength Astronomy What do different wavelength regimes allow astronomers to “see”?
Tools and Technology Space Objects By: Brittany D. Alexander.
Astronomy Chapter Nineteen: Galaxies and the Universe 19.1 Tools of Astronomers 19.2 Stars 19.3 Galaxies and the Universe.
The theory of the universe. Expanding of our universe In the 1920s, astronomers had the technology to see more Celestial bodies with advance telescope.
OUR UNIVERSE : AN EXPANDING MYSTERY Supratik Pal Indian Statistical Institute, Kolkata.
Radio Waves Interaction With Interstellar Matter
S4E1 Students will compare and contrast the physical attributes of stars, star patterns, and planets. d. Identify how technology is used to observe distant.
To View Slide Show Click on “Slide Show” above –Click on “From Current Slide”
Catalyst Pick up a note sheet. Pick up 1 piece of colored paper. Put “Unit 1 Astronomy” on the front of the colored paper. SIT SILENTLY IN YOUR SEAT.
Wilkinson Microwave Anisotropy Probe (WMAP) By Susan Creager April 20, 2006.
AIM: How was the Universe Created? Do Now: Which planet has the shortest day? Which planet rotates on its side? Which planet has the longest rotation?
Astronomy 2 Overview of the Universe Spring Lectures on External Galaxies. Joe Miller.
Using the GAVRT Radio Telescope: The SETI Project
GCSE Astronomy.
Aim: How did the universe form?
Evidence for The Big Bang
Key Areas covered The temperature of stellar objects is related to the distribution of emitted radiation over a wide range of wavelengths. The wavelength.
Observing and exploring space
STARS AND GALAXIES.
Lesson 1 Observing the Universe
Interesting Stuff in Space
Question of the Day What determines the path of the life cycle for a star? WWBAT: Describe the three types of galaxies Size.
Daily Routine Sit in your appropriate seat quietly
Ch.1, Sec.2 - Telescopes Optical Telescopes
Earth in Space & Time.
8 Space physics Topic overview
Solar system Orbital motions AQA SPACE PHYSICS PHYSICS ONLY Red shift
The Universe everything we can touch, feel, sense, measure or detect.
The Universe Visual Vocabulary.
BIG BANG THEORY.
Using Telescopes to Observe Electromagnetic Radiation in Space
Stars Notes Ch. 28.
Cosmology: SNC 1D.
The Formation of the.
FORMATION OF THE UNIVERSE
Big Bang.
Understand the electromagnetic spectrum and how it is organized.
Galaxies and the Universe
Contemporary science issues
How Did the Universe Begin?
Introduction to Astronomy
Using Technology to See Beyond the Visible
Using Technology to See Beyond the Visible
Optical Telescopes, Radio Telescopes and Other Technologies Advance Our Understanding of Space Unit E: Topic Three.
Absorption lines of a galaxy shift toward the blue end of the spectrum when it moves toward Earth. The lines shift to the red end of the spectrum when.
Absorption lines of a galaxy shift toward the blue end of the spectrum when it moves toward Earth. The lines shift to the red end of the spectrum when.
Integrated Science.
Formation of the Universe
The Universe everything we can touch, feel, sense, measure or detect.
Key Areas covered The temperature of stellar objects is related to the distribution of emitted radiation over a wide range of wavelengths. The wavelength.
How Technology is Used to Observe Objects in Outer Space
Understand the electromagnetic spectrum and how it is organized.
Section 5 – pg 622 The Expanding Universe
Evidence for the Big Bang Theory
Absorption lines of a galaxy shift toward the blue end of the spectrum when it moves toward Earth. The lines shift to the red end of the spectrum when.
12-3,4 Evolution of Stars.
The Universe.
Chapter 15 – Stars, Galaxies and the Universe
BIG BANG THEORY.
Understand the electromagnetic spectrum and how it is organized.
Scientific Theory on Origin of Universe
FORMATION OF THE UNIVERSE
Solar system Orbital motions AQA SPACE PHYSICS PHYSICS ONLY Red shift
Galaxies and the Universe
Presentation transcript:

OUR UNIVERSE : AN EXPANDING MYSTERY Supratik Pal Indian Statistical Institute, Kolkata

Meeeeeee…..

Night Sky From New York

Beyond Naked Eye: Telescopes

Eye in the Sky: Hubble Space Telescope

Supernova Probe Wilkinson Microwave Anisotropy Probe

ASTROSAT: A purely Indian Initiative Launched successfully on Sept 28, 2015

South Pole Telescope

Giant Meterwave Radio Telescope: Indian initiative

Square Kilometer Array in the making…. 11 core members countries, including India 1

Interesting facts about SKA SKA will use enough optical fibre to wrap twice around the earth. The data collected by SKA in a single day would take nearly two million years to playback in an iPod. The SKA central computer will have processing power of about one hundred million PCs. The SKA will be so sensitive that it will be able to detect an airport radar on a planet tens of light years away. The dishes of SKA will produce 10 times the global internet traffic. The aperture arrays of SKA could produce more than 100 times the global internet traffic.

Happy Birthday to our Universe: 13800000000 Years Ago

The First Sky

A Star is Born

Brighter than Stars : Nebulae

Our Galaxy Milky Way

Cloud made of Hydrogen in our Galaxy

~80% of visible matter is Neutral Hydrogen Neutral Hydrogen has singlet and triplet states Spin flip (Hyperfine splitting) Emits radiation with frequency 1420 MHz / wavelength 21 cm

Even what we do not see also exists: Dark Matter

Our Galaxy is one among Millions

= (300000 km/sec) X (2.5X1000000X365X24X60X60 sec) How far are They ? Nearest Galaxy: Andro- meda Our Galaxy: Milky way 2.5 million Light Years = (300000 km/sec) X (2.5X1000000X365X24X60X60 sec) = 20000000000000000000 kilo-meters !!!

To See the Unseen: Lens in the Sky

To See the Unseen: Collision in the Sky

Death of a Star: Supernova Explosion

What do they tell us ? Why are they so important ? Age of the Universe = 13800000000 Years Size of our Universe = 13800000000 Light Years = 100000000000000000000000 kilo-meters !!! Why are they so important ?

Universe is expanding at accelerated rate

Huge Energy Still Unknown

The Cosmic Constituents: As of Now

Scientific Queries What? Why? How?

And miles to go Dark energy or cosmological constant? What is dark energy? Why is cosmological constant so small? What is dark matter? Who governs fast expansion at the beginning? How were stars, galaxies etc formed? Gravitational waves: yes or no? How to match precise observational data? How to discriminate a model from others? Many more…..

Want to make it a career? Basic level ….. Mathematical Methods Classical Mechanics Quantum Mechanics Electrodynamics Advanced level ….. General Relativity Quantum Field Theory Particle Physics Computer Programming