May 2006April 2004Belinda Wilkes A bit about me! Dr. Belinda Wilkes, Professional Astrophysicist (Astronomer) Smithsonian Astrophysical Observatory, Cambridge,

Slides:



Advertisements
Similar presentations
Life Cycle of Stars.
Advertisements

Chapter 4 – Stars, Galaxies, and the Universe.  The electromagnetic spectrum includes the entire range of radio waves, infrared radiation, visible light,
The Life Cycle of a Star.
Ch. 9 – The Lives of Stars from Birth through Middle Age Second part The evolution of stars on the main sequence.
Random Letter of Wisdom Dear Mr. Planisek’s HPSC classes: Before you begin today- 1.This is one of the best classes that you will ever take. Keep.
StarsStars. What is a star? The objects that heat and light the planets in a system A star is a ball of plasma held together by its own gravity –Nuclear.
DO NOW QUESTION What life stage is our Sun currently in? What do you think will happen to our Sun as it gets older?
Astronomy Picture of the Day. Recall: Luminosity - Intrinsic property of a star. Apparent Brightness – the brightness we perceive a star to be from Earth.
Place the following images in a sequence to represent the life cycle of a mid-sized star: 1, 2, 10, 14, 19, 21, – Hubble Optical Image.
StarsStars. What is a star? The objects that heat and light the planets in a system A star is a ball of plasma held together by its own gravity –Nuclear.
Stars: 19.2 Life Cycle of Stars With help from: l
Life Cycles of Stars. Stars Stars are a large hot balls of plasma that shine The Sun is the Star in our solar system A group of stars that form a recognizable.
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?
The Life of a Star All stars begin their lives as nebula.
LET’S PLAY JEOPARDY!! Life cycle H-R Diagram characteri stics Mixed Q $100 Q $200 Q $300 Q $400 Q $500 Q $100 Q $200 Q $300 Q $400 Q $500 Final JeopardyJeopardy.
Copy everything in this colour into your notes!. Galaxies & Stars.
Fusion, Explosions, and the Search for Supernova Remnants Crystal Brogan (NRAO)
By Ryan and Mike. How stars are formed There are two main models of star formation. Gravitational collapse is a process when molecular clumps that are.
The Birth and Death of Stars. What are Stars? Stars are large balls of hot gas. Stars are large balls of hot gas. They look small because they are a long.
Star Formation Star = large balls of gas that produce energy and shine…. unless old. Nuclear Fusion = combines light elements to create heavy ones….
Birth and Life of a Star What is a star? A star is a really hot ball of gas, with hydrogen fusing into helium at its core. Stars spend the majority of.
THE LIFE CYCLE OF STARS Stars are born in nebulae. Huge clouds of dust and gas collapse under gravitational forces, forming protostars. These young stars.
The Life Cycles of Stars RVCC Planetarium - Last updated 7/23/03.
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 Life Cycle of a Star The Horsehead Nebula – one of the most famous pictures in astronomy.
The Universe… …is space and everything in it.
Life Cycle of a star HR Diagram Review. The HR (Hertzsprung-Russel) Diagram.
Astronomy (cont.) Cosmic Measurements Astronomical Unit (AU) - distance from earth to the sun ~150 million kilometers - used to express distances to other.
The life cycle of Stars. Where do stars come from  Stars form in clouds of gas (a nebula)  These are called diffuse nebula or star forming nebula. 
ETA CARINAE – NATURE’S OWN HADRON COLLIDER We still do not know one thousandth of one percent of what nature has revealed to us. - Albert Einstein -
Unit 1 Lesson 3 The Life Cycle of Stars
- HW Ch. 10, EXTENDED Mon. Nov. 8 - HW Ch. 11 & 12, due Mon. Nov HW Ch. 13 & 14 due Mon. Nov. 22 Exam 3 on Tuesday Nov. 23.
STARS.
STARS.
STARS & their life cycles Like us, stars are born, grow older, become middle aged and eventually die!!! Unlike us, stars take billions of years to complete.
BEYOND OUR SOLAR SYSTEM CHAPTER 25 Part II. INTERSTELLAR MATTER NEBULA BRIGHT NEBULAE EMISSION NEBULA REFLECTION NEBULA SUPERNOVA REMANTS DARK NEBULAE.
STARS Earth and Space. INTRODUCTION When you look at the sky on a clear night, you can see dozens, perhaps even hundreds, of tiny points of light. Almost.
Stars and Galaxies Traveling Beyond the Earth Chapter 21.
And a Star is Born xY.
May 2006April 2004Belinda Wilkes Astronomers learn by looking.
Life Cycle of Stars 1st Step: Stars form from nebulas
Stage 1: Nebula – Latin for “cloud”
Thank you for not chewing gum or anything else 
Complete the worksheet on differences between fusion and fission…
2009: A Big Year for Science! 200 years, Darwin’s birth: 12 Feb 1809
A bit about me! Dr. Belinda Wilkes, Professional Astrophysicist (Astronomer) Smithsonian Astrophysical Observatory, Cambridge, Mass., USA On contract to.
Life Cycle of Stars 1st Step: Stars form from nebulas
Life Cycle of Stars 1st Step: Stars form from nebulas
The Universe and Electromagnetic Spectrum
Life Cycle of Stars 1st Step: Stars form from nebulas
Outline of Ch 11: The H-R Diagram (cont.)
The Life Cycle of a Star.
Composition of Stars Classify stars by their color, size, and brightness. Other properties of stars are chemical composition and mass. Color and Temperature.
Life Cycle of Stars 2005 K.Corbett.
Life Cycle of Stars 1st Step: Stars form from nebulas
Life cycle of a star - foldable
Stars form from nebulas Regions of concentrated dust and gas
19.3 Stars.
Astronomers learn by looking
STARS.
Astronomy Star Notes.
You can often predict how a baby will look as an adult by looking at other family members. Astronomers observe stars of different ages to infer how stars.
Life Cycle of Stars 1st Step: Stars form from nebulas
Life Cycle of Stars 1st Step: Stars form from nebulas
How are stars born, and how do they die?
Unit 2: Stellar Evolution and Classification …The stars are a lot more than belonging to constellations! Unit 2 Miss Cohn.
STARS.
Life Cycle of a Star.
Life Cycle of Stars 1st Step: Stars form from nebulas
Presentation transcript:

May 2006April 2004Belinda Wilkes A bit about me! Dr. Belinda Wilkes, Professional Astrophysicist (Astronomer) Smithsonian Astrophysical Observatory, Cambridge, Mass., USA On contract to NASA to run Chandra X-ray Observatory (Hubble’s X-ray sister) English, BSc St. Andrews, PhD Cambridge In USA since 1982

May 2006April 2004Belinda Wilkes Astronomers learn by looking

May 2006April 2004Belinda Wilkes Life Cycle of a Star The Sun: our nearest star

May 2006April 2004Belinda Wilkes Stars have different colors B: blue – hottest A: green – warm C: red - cool What can we measure?

May 2006April 2004Belinda Wilkes Color, Brightness + Count them

May 2006April 2004Belinda Wilkes What makes the Sun Shine?

May 2006April 2004Belinda Wilkes Where are Stars Born? Clusters: Pleiades

May 2006April 2004Belinda Wilkes Stellar Nurseries Infrared: 30 Doradus in LMC Optical

May 2006April 2004Belinda Wilkes

May 2006April 2004Belinda Wilkes Circumstellar Disks First image of dust disk, around 18 th brightest star 25 light years away Disk thought to be debris left from planet formation Infrared

May 2006April 2004Belinda Wilkes

May 2006April 2004Belinda Wilkes Stellar Life Star burns fuel in its core (fusion: H→Helium) Initially fuel is H, star is on Main Sequence “Adult” (e.g. The Sun) When H runs out, core heats up and He, burns: “Middle Age” (Giant star) then He runs out, it burns heavier elements, e.g. Fe

May 2006April 2004Belinda Wilkes HR Diagram shows age and mass

May 2006April 2004Belinda Wilkes Death of a Star When all fuel runs out, the core collapses Outer regions of star explode outwards: Supernova SN shine more brightly than a galaxy for a few hours/days

May 2006April 2004Belinda Wilkes

May 2006April 2004Belinda Wilkes We are made of stardust!

May 2006April 2004Belinda Wilkes Cassiopeia A: X-rays

May 2006April 2004Belinda Wilkes The Crab Nebula Hubble Space T/p: OpticalChandra X-ray Observatory: X-ray

May 2006April 2004Belinda Wilkes Chandra X-ray Observatory

May 2006April 2004Belinda Wilkes What are X-rays?

May 2006April 2004Belinda Wilkes Focusing X-rays

May 2006April 2004Belinda Wilkes Launch: 23 July 1999 Space Shuttle Columbia

May 2006April 2004Belinda Wilkes STS-93 Shuttle Crew Commander: Eileen Collins Mission Spclst: Cady Coleman Astronomer: Steve Hawley

May 2006April 2004Belinda Wilkes Supernovae by Chandra