And his Atomic Theory. Niels Bohr was born on October 7, 1885 and he died on November 18, 1962. He was born in Copenhagen, Denmark and he died in the.

Slides:



Advertisements
Similar presentations
AQA Science © Nelson Thornes Ltd C2 1.1 True or false? How to play: Put your hand up for true, leave your hand down for false. Keep track of your.
Advertisements

The Sun – Describe characteristics of the Sun (S6C3PO2 high school)
Atomic Theories.
Ernest Rutherford By Lauren Kintzley and Brynn Reese.
The Sun - Our Star Sun’s diameter 100 times the Earth’s
Review Vocabulary magnetic field: the portion of space near a magnetic or current-carrying body where magnetic forces can be detected The Sun contains.
The Sun Chapter 28. Basic Properties Composition of sun 0.8% 70% 28% 0.3% 0.2%
What can happen when an atom absorbs energy?
Niels Bohr -Niels Henrik David Bohr was bored in Copenhagen, Denmark on October 7, 1885 and died in Copenhagen on November 18, 1962.
Niels Bohr By: Britany, Lynn, Tom, Rick, Kevin. Joke of the Day What happens when electrons lose their energy? They get Bohr'ed.
Sarah Keesee Lauren LeGardye Karli Weiand Born Copenhagen, Denmark October entered Copenhagen University won gold medal and earned.
By: Linden and Aleah Chemistry Bio Niels Henrik David Bohr was born in Copenhagen on October 7, He was the oldest son of Christian Bohr.
NIELS BOHR Chloe Listman and Margaux Benoit. Biography Niels Henrik David Bohr Born: 7 October 1885, Copenhagen, Denmark Most known for his theory on.
The History of the Atom.
Discovery of the Electron, Models & Theories Jeffrey Thorin Daniel.
ERNEST RUTHERFORD AND THE ATOMIC MODEL
THE SUN AND STARS And anything I want to put in here.
I Life Cycle of the Sun: A. Stars are born in nebulas. B. Nebula- A rapidly condensing cloud of gas and dust. C. Star “Pre-life Steps” 1. Gases rapidly.
Structure & Function. Our Nearest Star  Core  Comprises about 25% of sun’s interior  site of nuclear fusion  Radiative Zone  Energy produced in.
Modern Atomic Theory Group III: Libbi, Mazee, Taran, Elsie, Lane, Analise, Tyler, and Trey.
Section 1: Structure of the Sun
Chapter 4 The Bohr Model of the Atom Part 1. Visible Light.
NOTES – Introduction to Atomic Theory ( )
The Atomic Nature of Matter
Bohr's Model of the Atom.
Lauren Simonton Mary Heim Krystal Reese Hope Dubbs
BOHR’S LIFE AND HIS WORKS WHEN AND WHERE WAS OUR SCIENTIST BORN? WHAT EXPERIMENTS DID OUR SCIENTIST DO? HOW DID SUCH EXPERIMENTS HELP IMPROVEMENT OF ATOMC.
Chapter 29 The Sun 29.1 Structure of the Sun
History of Atomic Theory
OUR SUN THE CLOSEST STAR. Composition of the Sun The Sun is composed of at least 80 of the elements found on Earth. Sun is mostly composed of 91.2% Hydrogen,
Section 1: Structure of the Sun
The Sun’s Size, Heat and Temperature After completing this section, students will explain nuclear fusion, and describe the sun and compare it to other.
Unit 2 Lesson 3 The Sun Copyright © Houghton Mifflin Harcourt Publishing Company.
The Bohr Model and the Quantum Mechanical Model of the Atom
Sam Williams and Corey Taylor.  Niels Bohr was born on October 7, 1885 and died on November 18, 1962  Niels Bohr’s full name was Niels Henrik David.
By: Jessica Ferguson and Whitney Mann.  Niels Bohr in his younger days.
Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. Shown here is a life-sized model of a skier, but not all models are physical.
Atomic Structure A level at The Sixth Form College Colchester Adapted from: An example of How Science Works: Development of the Model of Atomic Structure.
Born on: October 7, 1885 Born at: Copenhagen, Denmark Died on: November 18, 1962 Died at: Copenhagen, Denmark.
5.1 Revising the Atomic Model > 1 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. Chapter 5 Electrons In Atoms 5.1 Revising.
The Story of the Atom Have your books open to page 73 Chapter 3.
Jackson and Kayla, Ernest Rutherford considered the father of nuclear physics Won the 1908 Nobel Prize in Chemistry Wanted to see if Thomson's.
Niels Bohr By: Leann Coffer, Zachariah Maskell, & Dylan Silva.
Niels Bohr A Brief History By: Dusty, Garrett, Jason & Timmay!
Atomic Theories Chapter 4.1 How do we know about atoms when no one has ever seen inside an atom?
Electrons in Atoms Light is a kind of electromagnetic radiation. All forms of electromagnetic radiation move at 3.00 x 10 8 m/s. The origin is the baseline.
Interesting quotes from Niels Bohr “Anyone who is not shocked by quantum theory has not understood it” “An expert is a man who has made all the mistakes.
NIELS BOHR COLE TODD AND ZACH SHEEHAN. WHAT, WHERE, WHY Niels Bohr announced the theory of electron placement in 1913, while studying at Cambridge.
History of Atomic Structure. Aristotle Democritus.
The Sun By: JGilliam The Sun’s CompositionIdentifying Stars Composition ▪ Hydrogen and Helium together make up 99% of the sun’s mass. ▪ 75% of the sun’s.
Unit 8 Chapter 29 The Sun. We used to think that our sun was a ball of fire in the sky. Looking at our sun unaided will cause blindness. The Sun’s Energy.
Models of the Atom Particle model of matter: All matter is composed of tiny particles called atoms. The combination of the types of particles in a substance.
Start of Class 1. Pick up your work from the front table. 2. Get a blank piece of paper and draw something like this 2/24/2016describe how the planets.
CHAPTER ONE The big picture – the periodic table.
Most of the sunlight we see from earth comes from continuous photosphere emissions. These emissions make up the “quiet sun”.
By Steven Scott and Bryan Denin.  Born October 7, 1885  Died November 18, 1962  Received Nobel Prize in 1922  Developed Bohr Model of the atom  Attended.
The Sun The SUN Chapter 29 Chapter 29.
5.1 Revising the Atomic Model > 1 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. Chapter 5 Electrons In Atoms 5.1 Revising.
Ms. Mikus Tuesday, September 8, 2009 D ALTON B IOGRAPHICAL I NFORMATION John Dalton was born on September 6, 1766 and died on July 27,1844. He worked.
Chapter 29. Sec 1 Structure of the sun People believed the sun’s energy came from fire They believed the sun burned some type of fuel to produce energy.
Unit 2 Lesson 3 The Sun Copyright © Houghton Mifflin Harcourt Publishing Company.
NIELS BOHR By Maddie O’Connor
Niels Henrik David Bohr
Astronomy-Part 8 Notes Here Comes The Sun
Niels Bohr Interesting quotes from Niels Bohr
Do Now 12/9/09 What is the sun made of???
Niels Bohr In the Bohr Model (1913) the neutrons and protons occupy a dense central region called the nucleus, and the electrons orbit the nucleus much.
The Sun.
Presentation transcript:

And his Atomic Theory

Niels Bohr was born on October 7, 1885 and he died on November 18, He was born in Copenhagen, Denmark and he died in the same area. His parents were Christian Bohr and Ellen Adler, (Bohr). He had an older sister named Jenny, who was born in 1883, and a younger brother named Harald who was born in Harald and Niels were very close through out his childhood and he was often heard saying that Harald was his best friend all through his life. Niels entered the Grammelholms school in October of 1891, he attended this school for his complete secondary education. He did fairly well in school but could never lay claim to a brilliant mind, he usually came in forth or fifth in a class of twenty. In his last two years in school Niels specialized in mathematics and physics, he frightened his math teacher with his exceptional skills and would work ahead in the physics textbook often pointing out errors in the text. He was learned more about this subject than he did from his teachers. Bohr entered the University of Copenhagen in Physics was his major and he had minors in mathematics and chemistry.

When he was in University he wouldn’t have been able to carry out any experiments in physics because the University didn’t have a laboratory, so he used his father’s physiology lab. And his first paper describes some of the experiments he did in the lab, he dedicated this paper to his brother, Harald. Due to this paper, Bohr, won the Gold Medal for 1906 from the Royal Danish Academy of Sciences, this was for his analysis of water jets being used to determine surface tension. He got his masters degree from the University of Copenhagen in 1909, and his doctorate in 1911for his thesis, Studies on the electron theory of metals. This thesis was dedicated to his father, who had died earlier in the year from a heart attack Bohr was engaged to Margrethe Norlund, who, many say, placed a key role in his successfulness, at the time of his father’s death. In 1911 in the month of September Bohr went to England to study with J J Thompson at Cambridge, he had hoped to spend a long period of time with Thompson, but, unfortunately, they didn’t get along. Lucky for him, he had met Rutherford earlier in that year and went to study with him instead, this was right after Rutherford had published his theory, which states that the bulk of the mass of an atom can be found in the nucleus.

Bohr began developing his theory in June of 1912 He did his fundamental work on the hydrogen atom eventually he even did some work on some heavier atoms. Bohr returned to Copenhagen to continue working on his theory which he completed to his satisfaction in and around July of The University recommended his name for a chair in theoretical physics, he expected his position to be confirmed within a year. It wasn’t to be. He spent the next four years working with Rutherford and his group yet again, he enjoyed his time with the group immensely, participating in many break through activities. His completed theory of the atom gave us the clue as to where, exactly, electrons were found in an atom. He stated that electrons traveled on fixed energy levels. Sort of like a ladder, these electrons could change orbits but they would always be found in an orbit and there would always be a certain number of electrons in the orbital.

Changing Energy Levels The fact that there were certain orbits and energies in an atom was part of Bohr’s theory. When these energies change levels there is a different color given off.

Orbits were the key to Bohr’s theory

People a long time ago, believed that the northern lights were a sign from God. Nobody would believe someone if he were to tell them that it could be explained with science, and if it was a woman trying to tell them this they would often be placed in an asylum or they would be placed in the care of one distant relative or another. Now we know the truth they can be explained by science and Niels Bohr is just the scientist to do it.

To answer this, we start with the sun whose energy production is far from even and fluctuates on an 11 year cycle. Maximum production occurs at the same time as high sunspot activity, processes on the sun's surface throw particles far out in space. These particles are called the solar wind and cause the northern lights. The sun's surface temperature is approximately 6,000 0C, much cooler than the interior which is several million degrees. In the sun's atmosphere the temperature rises again to several million degrees. At such temperatures, collisions between gas particles can be so violent that atoms disintegrate into electrons and nuclei. What was once hydrogen becomes a gas of free electrons and protons called plasma. This plasma escapes from the sun's atmosphere through a hole in the sun's magnetic field. As they escape, they are thrown out by the rotation of the sun in an ever widening spiral - the so-called garden-hose effect. The name originates from the pattern of water droplets formed if we swing a garden hose around and around above out heads. -Bohr

What causes the northern lights? Cont. The 11-year sunspot cycle compared to northern lights activity. The garden hose effect.

Presentation done by Becca Prescott, Dane Huntley, Maria Davis and Samantha Stewert