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SyllabusF07

Course: SCI 190, Fall 2009
School: University of Dayton
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E. John Erdei INTEGRATED NATURAL SCIENCE SEQUENCE (INSS) SCI190 Fall 2007 Science Center 101B 92318 John.Erdei@notes.udayton.edu Mon Thrs 9:00 am 10:30 am 1:00 pm 2:30 pm Office of the Dean: O'Reilly Hall 104A 92604 Physics: Office Hours: Web Page: Text: http://www.udayton.edu/~physics/jee/jee.htm Hewitt, Conceptual Physics, 10th Ed. INTRODUCTION SCI190 it the first course in a sequence of three courses....

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E. John Erdei INTEGRATED NATURAL SCIENCE SEQUENCE (INSS) SCI190 Fall 2007 Science Center 101B 92318 John.Erdei@notes.udayton.edu Mon Thrs 9:00 am 10:30 am 1:00 pm 2:30 pm Office of the Dean: O'Reilly Hall 104A 92604 Physics: Office Hours: Web Page: Text: http://www.udayton.edu/~physics/jee/jee.htm Hewitt, Conceptual Physics, 10th Ed. INTRODUCTION SCI190 it the first course in a sequence of three courses. These courses are integrated, which allows information in from one course in the sequence to be used in another course. FOR FULL DETAILS ABOUT THE INSS CONSULT THE SCI190 LINK IN THE WEBPAGE LISTED ABOVE. Grading Exam Test 1 Test 2 Test 3 Points 50 50 50 Exam Test 4 Test 5 Test 6 Total Points 50 50 100 350 Grades will be computed on the basis of a possible 350 points on the tests. Points 325 315 Percentage of Total 93% 90% Grade A APoints 304 290 280 Percentage of Total 87% 83% 80% Grade B+ B BPoints 269 255 245 Percentage of Total 77% 73% 70% Grade C+ C CPoints 210 < 210 Percentage of Total 60% Grade D F ALL EXAMS ARE CLOSED BOOK, WITH NO FORMULA SHEETS OR CALCULATORS NOTE: ALL tests must be taken at the assigned time. A make-up exam will be given at the end of the term for those with a LEGITIMATE WRITTEN MEDICAL EXCUSE. Missed tests without such an excuse will be assigned a zero (going out of town and ride is not returning on time to take exam is not an acceptable excuse). Makeups are not given to replace a low score on one of the tests. The exams are not returned to the students. They can be examined at any time in the instructors office. MAKEUPS: A day is set aside at the end of the term for ALL makeup exams. Those with a valid excuse must obtain a REQUEST FOR MAKEUP EXAM form from the instructor of the course. The form must be filled out and signed by the instructor. Students who have not filled out a request form will not be allowed to take a makeup exam. Unless otherwise stated in class, ALL MAKEUP EXAMS ARE ON THE DATE LISTED ON THE CALENDAR AT 7:00 PM IN THE USUAL CLASSROOM. LAST EXAM: The last exam is administered during finals week. The time and date of the exam is listed on the calendar. All students registered for this course are required to take the last exam at the time specified. Students unable to take the last exam for a valid medical reason will be given an "I" and the exam will be made up at a later date. An exception is given to graduating seniors, who may have to take the exam early. This will be arranged by the instructor. COURSE WEBSITE: There is a website associated with this course that can be accessed through the website of Dr. Erdei at http://www.udayton.edu/~physics/jee/jee.htm. To get to the course website, click on the SCI190 link (in blue) at the bottom of the page. SPECIAL CONSIDERATIONS: Students with learning disabilities can be given extended time for exams or a private location for taking exams in accordance with state and federal law. ALL STUDENTS REQUESTING SPECIAL CONSIDERATION ON EXAMS MUST PRESENT DOCUMENTATION from the Office of Learning Assistance to the course instructor at the beginning of the semester. Any special considerations for the location of the administration for the exam must be arranged with the instructor in advance. Homework Hewitt, 10th Ed. NOTE: Some sections in a given chapter will not be covered in class and will not appear on exams. Review Questions are labeled by section in the book. Only those section that have Review Questions assigned from them will appear on exams. C1 Rev: One Step: 1,9,10,11,12,19 9 1,7,8,9,10,11 1,7,9,11,12,15,20,28,29 2,3,4,5,6,7,8,9,10,11,12,18,19,20,22,23,24,26 4,8,10,12,14,17,20,22 3,4,6,9,10,11,13,15,16,17,19,22,24,27,32 3,4,5,7 3,5,6,7 6,8,13,16,17,18 1,10,11,12,16,20,22,23,24,25,28,29,30,31,33 1,4 2,5,7,9 1,2,3,9,13,14,21,34,36,41,47 2,3,4,5,8 4,5,10,11,12,14 4,7,13,20,24 1 1,3,4,6,9,12,16,18 2,3,5,7 1,2,3,4,5,14,15,16,18,23,24,26,27,28,33,41,42, 43,53,54,55 7,8 3,4,5,7,8,10,11,14,24,25 2,4,8,10,11,12,13,14 1,2,11,13,19,28,29,32,33,36,46,60,62 4 1,2,7,8,9,13,15,16,17,19,20 5,7,8,24,25,28,32,39,44 2,3,6,7,9 1,3,5,6,7,14 6,9,15,42 3 3,4,13,21,22,26,27 5,6,17,26 13,14,15 1,2 C18 Rev: One Step: 7,8,9,10,11,16,26,27 2,5,6,9,10,16,21,23,25,37,42,44 1,2,3 6,8,9,10,11,12,13,26,18,19 13,15,16,17,18,19,21,23,24,25,26,27,31 3,5,6 5,8,20,21,23,24 5,6,8,16,17,19,20,24,29,30,32,33 1,2,3,4,7 2,3,4,7,10,18,19,25,26 1,9,10,11,12,14,18,21,24,25,32,44,53 1,10 4,5,17,19 Ex: Prob: C2 Rev: One Step: Ex: Prob: C19 Rev: One Step: Ex: Prob: C3 Rev: One Step: Ex: Prob: C20 Rev: One Step: Ex: Prob: C10 Rev: One Step: Ex: Prob: C22 Rev: One Step: Ex: Prob: C4 Rev: One Step: Ex: Prob: C23 Rev: One Step: Ex: Prob: C5 Rev: One Step: Ex: Prob: C24 Rev: One Step: 3,7,9,10,11,12,13,14,19,20 2,5,8,9,12,13,20,24,31,39 2,4,5,8,16,17,118,19 3,8,9.16,24,25,26,33 1,3,4 1,2,3,4,5,6,7,8,9,10,11,12,13 4,5,7,8,18,20,21 1,3,4,5,7 11,12 39 2,6,8 4,8,30 1 11,12,13 9,11,12 1,4,5,6,7,8,13,14,16,17,19 3,5,10,16,19,40,43,46,47 1 Ex: Prob: C6 Rev: One Step: Ex: Prob: C25 Rev: One Step: Ex: Prob: C7 Rev: One Step: Ex: Prob: C26 Rev: One Step: Ex: Prob: C15 Rev: One Step: Ex: Prob: C11 Rev: One Step: Ex: Prob: C16 Rev: One Step: Ex: Prob: C31 Rev: One Step: Ex: Prob: C17 Rev: One Step: Ex: Prob: C32 Rev: One Step: Ex: Prob: C14 Rev: One Step: Ex: Prob: C30 Rev: One Step: Ex: Prob: Ex: Prob: August Sunday 19 26 20 27 Monday Tuesday 21 Classes Begin C1 28 C3 29 22 Wednesday 23 C2 30 C3 31 Thursday 24 Friday 25 Saturday September 1 2 9 16 23 30 3 Holiday 10 Drop W/O Rec 17 24 4 Test 1 (1,2,3) 11 C5 18 C7 25 C15 26 19 C10 12 5 6 C4 13 C6 20 27 C16 Test 2 21 28 22 29 (10,4,5,6,7) C15 14Subm For Grad 15 7 8 October 1 7 14 8 15 2 9 C14 16 Grad Fair C18 21 28Parents Wkend 22 23 C19 29 30 C20 31 24 17 MidTerms Due 18 Test 4 (17,14,18) 25 C20 C19 26Parents Wkend 27Parents Wkend 19 20 Test 3 C17 10 3 4 C17 11MidTerm Break 12MidTerm Break 13 5 6 (15,16) November 1 4 11 18 25 5 ...

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University of Dayton - SCI - 190
Part 2, B: MOTION Newton's Laws Fnet2Net force is the vector sum of the individual forces7N2N5NPart 2, B: MOTION Newton's Laws2Part 2, B: MOTION Newton's Laws2Part 2, B: MOTION Newton's Laws2Example: An object sits at rest on
University of Dayton - SCI - 190
123456Destructive Interference Active Noise Reduction (ANR)Koss Noise Reduction Headphones7Destructive Interference Active Noise Reduction (ANR)Koss Noise Reduction HeadphonesThis revolutionary Active Noise Reduction (ANR) ste
University of Dayton - SCI - 190
University of Dayton - SCI - 190
1234Part 2, B: MOTION Newton's Laws Fnet2Net force is the vector sum of the individual forces7N2N5N5Part 2, B: MOTION Newton's Laws26Part 2, B: MOTION Newton's Laws27Part 2, B: MOTION Newton's Laws2Example: An ob
University of Dayton - SCI - 190
Part 2, B: MOTION Derived Quantity - Acceleration An object is moving with a speed of 3 m/sec and accelerates at 4 m/sec . What is its speed after 1 sec, 2 sec, etc?Part 2, B: MOTION Derived Quantity - Acceleration An object is moving with a speed
University of Dayton - SCI - 190
15 Part 2, A: THERMODYNAMICS 6 WORK Definition (Young): Energy is the capacity to do work.16 Part 2, A: THERMODYNAMICS 56 WORK Definition (Young): Energy is the capacity to do work. W = Fd W F d is the work done (Joules) is the applied force (Newto
University of Dayton - SCI - 190
MotionInertiaPart 2, B: MOTION Newton's Vis Viva - Momentum Momentum: p = mv So what?2Part 2, B: MOTION Newton's Vis Viva - Momentum Recall: av=at ma v = ma t ap=Ft2Part 2, B: MOTION Newton's Vis Viva - Momentum Definition: a p is called
University of Dayton - SCI - 190
Part 3(e): Atomic Physics Bohr Model of the Atom Important point: * Each atom has a unique set of orbits * Each atom produces a unique set of wavelengths when it produces em wavesPart 3(e): Atomic Physics Bohr Model of the Atom Important point: * E
University of Dayton - SCI - 190
Astrophysics and CosmologyHow do we know what we know about the universe around us?Astrophysics and CosmologyHow do we know what we know about the universe around us? The farthest from the Earth we have been to return direct evidence has been Mar
University of Dayton - SCI - 190
Part 2, A: THERMODYNAMICS Ideal Gas Relationships - Equation of State3An equation of state is a relationship between the pressure, volume, and temperature of a system. In thermodynamics, pressure, volume, and temperature define the state of the s
University of Dayton - SCI - 190
E = F/q
University of Dayton - SCI - 190
Motion Newton's Laws1. Every body continues in its state of rest or uniform motion unless it is acted upon by a net external force. 2. The acceleration of a body is equal to the net force acting on the body divided by the mass of the body.NETa=F
University of Dayton - SCI - 190
1Motion* Why do all objects &quot;seem&quot; to fall at the same rate? * What is the relationship between force and motion? * Why do like really big slow moving ships run into like really big stationary continents?2MotionVis Insita Power of Resting3
University of Dayton - SCI - 190
1Fundamental Quantities and UnitsFundamental Quantity MKS Unit2Fundamental Quantities and UnitsFundamental Quantity * Length MKS Unit (Meters)3Fundamental Quantities and UnitsFundamental Quantity * Length * Mass MKS Unit (Meters) (Kilogr
University of Dayton - SCI - 190
Part 2, A: THERMODYNAMICS 2 Conservation of Energy Heat WorkKinetic EnergyChemical Energy1Part 2, A: THERMODYNAMICS Kinetic Theory Kinetic Energy3TemperatureHeat2Part 2, A: THERMODYNAMICS Kinetic Theory Kinetic Energy4Temperature
University of Dayton - SCI - 190
E = F/q
University of Dayton - SCI - 190
Line SpectraLine Spectrum of Hydrogen Gas
University of Dayton - SCI - 190
15 Part 2, A: THERMODYNAMICS 6 WORK Definition (Young): Energy is the capacity to do work.16 Part 2, A: THERMODYNAMICS 56 WORK Definition (Young): Energy is the capacity to do work. W = Fd W F d is the work done (Joules) is the applied force (Newto
University of Dayton - SCI - 190
123Standing Waves What determines the &quot;standing wave patterns&quot; that can be achieved in a system?4Standing Waves What determines the &quot;standing wave patterns&quot; that can be achieved in a system? * The length of the system5Standing Waves Wha
University of Dayton - SCI - 190
Motion Newton's LawsI'd rather be a hammer than a nail.- Simon and Garfunkel1Motion Newton's Laws1. Every body continues in its state of rest or uniform motion unless it is acted upon by a net external force. 2. The acceleration of a body i
University of Dayton - SCI - 190
12345MotionVectorsQuantity Distance Speed Acceleration Symbol d v a d/t v/t Definition Units m m/s m/s2 Quantity Symbol Definition UnitThe symbol &quot; means &quot;Change in&quot;6MotionVectorsQuantity Distance Speed Acceleration Symbol d v a d/
University of Dayton - SCI - 190
Part 2, A: THERMODYNAMICS2Anaximander: Two sets of opposites - wet and dry, hot and cold. Empedocles: First to detail the theory of the four elements - earth, wind, water, and fire.1Fundamental Quantities and UnitsFundamental Quantity * Lengt
University of Dayton - SCI - 190
How do we know what we know about the universe around us?How do we know what we know about the universe around us?Moving one step closer to finding the fingerprints of life in a habitable planet beyond the solar system, astronomers have for the f
University of Dayton - PHY - 206
Chapter 2 Motionin One Dimension2008 by W.H. Freeman and Company2-1 DisplacementThere is a distinction between distance and displacement.Displacement (blue line) is how far the object is from its starting point, regardless of how it got there.
University of Dayton - PHY - 206
Chapter 3 Motion in Two and Three Dimensions; VectorsVectors and ScalarsA vector has magnitude as well as direction. Some vector quantities: displacement, velocity, force, momentum A scalar has only a magnitude. Some scalar quantities: mass, time,
University of Dayton - PHY - 202
Chapter 27 Early Quantum Theory and Models of the Atom27.2 Plancks Quantum Hypothesis; Blackbody RadiationAll objects emit radiation whose total intensity is proportional to the fourth power of their temperature. This is called thermal radiation;
University of Dayton - PHY - 202
Wave Nature of LightRefraction Interference Young's double slit experiment Diffraction Single slit diffraction Diffraction grating24. Wave Nature of Light24.1 Waves Versus Particles; Huygens' Principle and DiffractionHuygens' principle: Every
University of Dayton - PHY - 202
PHYSICS 202, WINTER 2007 Please note that this syllabus is subject to change!Instructor: Dr. Mo Ahoujja Office: SC013 Phone: 229-2735 Email: Mo.ahoujja@notes.udayton.edu Homepage: http:/campus.udayton.edu/~physics/ma/ma.htm Office Hours: MWF: 1:00-2
University of Dayton - PHY - 202
Practice Test #3- Chapters 23, 24 and 27 from Giancoli 5ed1. A real object is placed 10 cm from a converging lens that has a focal length of 6 cm. Which statement is most accurate? a. b. c. d. The The The The image image image image is is is is rea
University of Dayton - PHY - 202
Practice Test #3- Chapters 23, 24 and 27 from Giancoli 5ed1. A real object is placed 10 cm from a converging lens that has a focal length of 6 cm. Which statement is most accurate? a. b. c. d. The The The The image image image image is is is is rea
University of Dayton - PHY - 202
PHY202Practice-Test 1Winter, 20031. What is the magnitude and direction of the electric field at a point midway between a 8 C and a +6.0 C charge 4.0 cm apart? a. b. c. d. 3.2x108 N/C, toward the negative charge 3.2x108 N/C, toward the positive
University of Dayton - PHY - 202
Practice Test 2 (chapters 20, 21, 22, and 23 from Giancoli).Mar3, 031. What is the strength of a magnetic field 4.0 cm from a long straight wire carrying 3.0 A of current? 2. Two long parallel wires carry currents of 5.0 A and 8.0 A in the same d
University of Dayton - PHY - 207
B due to a moving point charge Biot-Savart law: B due to a current element B on the axis of a current loop B inside a solenoid B due to an infinite long straight wire Ampere's Law: Note: Ampere's law is valid only if currents are continuous with a hi
University of Dayton - SCI - 190
SCI190,Fall of 2005Instructor: Dr. Mo Ahoujja Office: Sherman SC013 Phone: 92735 (229 2735 off campus) E-mail: mo.ahoujja@notes.udayton.edu Homepage: http:/www.udayton.edu/~physics/ma/ma.htm Office Hours: Mon. 3-4, Wed. 11-12, Tue. 11:45-12:45, or b
University of Dayton - PHY - 206
PHYSICS 206, WINTER of 2006 Please note that this syllabus is subject to change!Instructor: Dr. Mo Ahoujja Office: SC013 Phone: 229-2735 Email: mo.ahoujja@notes.udayton.edu Homepage: http:/www.udayton.edu/~physics/ma/ma.htm Office Hours: MWF: 11:00-
University of Dayton - SCI - 190
Review for test4 Chapter 22chapters 22, 24, 25, and 26Like charges repel and unlike charges attract. Electric force between two charges is proportional to the product of the charges divided by the square of the distance between the two charges. G
University of Dayton - SCI - 190
SCI190,Fall of 2008 Note that this syllabus is subject to change!Instructor: Dr. Mo Ahoujja Office: Sherman SC013 Phone: 92735 (229 2735 off campus) E-mail: mo.ahoujja@notes.udayton.edu Homepage: http:/campus.udayton.edu/~physics/ma/ma.htm Office Ho
University of Dayton - PHY - 207
PHY20702 3010827 2863680 3006583 3018016 3079352 3035215 3005433 3006612 3033386 2979889 3060505 3040192 3009359 2823718 3060463 3053660 3006555 3044152 3014471 3018910 3006547 3036672 3060426 3025514 3030896 2774642 2974179 3006526 3227976 3014200 2
University of Dayton - PHY - 207
PHYSICS 207, FALL 2006Instructor: Dr. Mo Ahoujja Office: SC013 Phone: 229-2735 Email: mo.ahoujja@notes.udayton.edu Homepage: http:/www.udayton.edu/~physics/ma/ma.htm Office Hours: MWF: 1-2, or by appointment. Note that this syllabus is subject to ch
University of Dayton - PHY - 403
Intermediate Mechanics IIExam2 Take-HomeNovember 14, 2006The following problems are due at the beginning of class on Monday, 4 December 2006. Problem 1. (25 pts.) A massless rigid rod of length l is attached at one end to an electric motor and
University of Dayton - SCI - 190
Chapter 6Momentum = mass times Momentum = m v velocityWhich has a greater momentum, a heavy truck at rest or a moving skateboard? What is the magnitude of the momentum of a 100 kg bike moving at 14 m/s? What is the magnitude of the momentum of a 0
University of Dayton - PHY - 206
PHYSICS 206, Fall of 2008 Please note that this syllabus is subject to change!Instructor: Dr. Mo Ahoujja Office: Sherman SC013 Phone: 92735 (229 2735 off campus) E-mail: mo.ahoujja@notes.udayton.edu Homepage: http:/campus.udayton.edu/~physics/ma/ma.
University of Dayton - PHY - 206
Practice Test#3 (Chapters 8,9, and 10 From Tipler) 1.The center of mass of the system of particles shown in the diagram is at point A) 1 B) 2 C) 3 D) 4 E) 52. A boy and girl on ice skates face each other. The girl has a mass of 20 kg and the boy
University of Dayton - PHY - 206
Practice Test 2 1. A mass m is traveling at an initial speed v0 = 25.0 m/s. It is brought to rest in a distance of 62.5 m by a force of 15.0 N. What is the mass m?2.Which of the following free-body diagrams represents the block sliding down a fri
University of Dayton - PHY - 201
PHY 201 Summer 1st Session, 2008Instructor: Dr. Mo Ahoujja Office: SC 013 Phone: 229-2735 e-mail: mo.ahoujja@notes.udayton.edu Webpage : http:/campus.udayton.edu/~physics/ma/ma.htmTEXT: Giancoli, Physics, 6th Ed. 2005 Course Description and Object
University of Dayton - PHY - 207
Practice Test 3 1. (a) An AC voltage source has an output given by = 200 sin t. This source is connected to a 100 resistor. Find the peak (maximum) and rms current in the circuit. (2 A, 1.41A)(b) An inductor L = 25 mH is connected to a source whos
University of Dayton - PHY - 206
Practice Test#4 (Chapters 11 and 14 From Tipler)1. The moon has a period of 27.3 d (days) and is an average distance from the earth of 3.84 105 km. A communications satellite is placed in an earth orbit at 4.23 104 km from the center of the earth
University of Dayton - PHY - 207
PHY207 Fall 2005Exam1Name(print)NOTE: For full credit, you must show your work! Some useful constants and information:Volume of a sphere of radius R : V = 4/3 R3 Area of a sphere of radius R : A = 4 R2e = 1.60x10-19 C, k = 8.99x109 N.m2/C2
University of Dayton - PHY - 206
Practice Test#3 ( Chapters 8,9, and 10 from Tipler) M r cm = mi ri ;i p = mv ; ;Fnet ,exttf dp = dt = t;1 K = mv 2 2; U = mghI = F dt = P ;tiF avIv2 f - v1 f = -(v2i - v1i );relative speed of particles in an elast
University of Dayton - PHY - 206
Practice Test#4 (Chapters 11 and 14 From Tipler)1. The moon has a period of 27.3 d (days) and is an average distance from the earth of 3.84 105 km. A communications satellite is placed in an earth orbit at 4.23 104 km from the center of the earth
University of Dayton - NEHI - 2006
Mary Beth Blegen Teacher/Consultant/Speaker 17114 Firtree Place Farmington, MN 55024 952-953-3955 Marybeth@marybethblegen.com Mary Beth Blegen has worked as a consultant in the Saint Paul High Schools since 2001. She works with schools on the develop
University of Dayton - NEHINSTITU - 2008
Institute Location: Vienna, AustriaDEAR COLLEAGUE LETTER1MOZART'S WORLDS June 16July 11, 2008Dear Colleague, Thank you for your inquiry about the NEH Institute &quot;Mozart's Worlds.&quot; Imagine yourself living in Vienna for four weeks, and studying th
University of Dayton - DAY - 3
DNAThe Secrets it tells us about Evolution!Remember: Gene Chromosome 1 molecule of DNA = 1 chromosome What are the building blocks of DNA? What are the building blocks of protein?How do genes code for genetic traits?Answer: 1 gene co
University of Dayton - PHY - 250
Black Hole in the Center of the Galaxy Compelling EvidenceBlack Hole in the Center of the Galaxy Compelling EvidenceNASA's COBE satellite scanned the heavens at infrared wavelengths in 1990 and produced this premier view of the central region of
University of Dayton - PHY - 6
Black Hole in the Center of the Galaxy Compelling EvidenceBlack Hole in the Center of the Galaxy Compelling EvidenceNASA's COBE satellite scanned the heavens at infrared wavelengths in 1990 and produced this premier view of the central region of
University of Dayton - PHY - 250
Supernova Type 2 SupernovaProduced during the death of a very massive star.SupernovaTWO VERY DIFFERENT TYPES OF SUPERNOVAESupernova Type Maximum Luminosity Type Ia* 3 x 109 Suns Type II83 x 10 Suns Spectrum Where found No hydrogen lines Lines
University of Dayton - PHY - 6
Supernova Type 2 SupernovaProduced during the death of a very massive star.SupernovaTWO VERY DIFFERENT TYPES OF SUPERNOVAESupernova Type Maximum Luminosity Type Ia* 3 x 109 Suns Type II83 x 10 Suns Spectrum Where found No hydrogen lines Lines
University of Dayton - PHY - 250
The Solar SystemTitan (Saturn)This is the first coloured view of Titan's surface, following processing to add reflection spectra data, gives a better indication of the actual colour of the surface. Initially thought to be rocks or ice blocks, the
University of Dayton - PHY - 6
The Solar SystemTitan (Saturn)This is the first coloured view of Titan's surface, following processing to add reflection spectra data, gives a better indication of the actual colour of the surface. Initially thought to be rocks or ice blocks, the
University of Dayton - PHY - 250
Gamma Ray Bursts (GRB)Compton Gamma Ray Observatory (CGRO)Gamma Ray Bursts (GRB)Gamma Rays the highest energy photons in the electromagnetic spectrum Gamma-ray bursts - short-lived bursts of gamma ray photons, the most energetic form of light.
University of Dayton - PHY - 6
Gamma Ray Bursts (GRB)Compton Gamma Ray Observatory (CGRO)Gamma Ray Bursts (GRB)Gamma Rays the highest energy photons in the electromagnetic spectrum Gamma-ray bursts - short-lived bursts of gamma ray photons, the most energetic form of light.