Brochure
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- Introduction
- V1.1 Introduction: The Expanding Universe
- V1.2 Distances in Astrophysics: Using apparent sizes
- V1.3 Distances from Brightnesses
- V1.4 Spectra
- V1.5 Doppler Effect
- V1.6 Hubble Law
- V1.7 Exploding Egg model
- V1.8 Expanding Space
- V1.9 Steady State vs Big Bang
- V1.10 Blueshifted Galaxies
- V1.11 Conclusion
- What Now?
- Reference Notes
- WE1.1 Big Numbers and Strange Units
Greatest Unsolved Mysteries In The Universe
Quick Facts
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Medium of instructions
English
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Mode of learning
Self study
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Mode of Delivery
Video and Text Based
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Course overview
Planets, stars, galaxies, and all other forms of matter and energy comprise the universe. The Big Bang theory is the predominant cosmological explanation of the universe's evolution. According to this theory, space and time emerged simultaneously 13.7870.020 billion years ago, and since the big bang, the universe has been expanding. While the size of the entire universe is unknown, the observable universe has a diameter of approximately 93 billion light-years at the present time. Ancient greek and indian philosophers created geocentric models of the universe that placed the Earth at the center. Greatest Unsolved Mysteries In The Universe certification is made available by Udemy to candidates who want to know what’s happening in the universe
Greatest Unsolved Mysteries In The Universe online training comprises 10.5 hours of video, eight articles, and 13 downloadable resources. and a digital certificate for course completers.
New Trends in Outer Space Development online classes consist of the expanding universe, the big bang, dark energy, giant black holes, the first light in the universe, dark matter, solar system formation, and life in space.
The highlights
- Full Lifetime Access
- 10.5 Hours of Video
- 13 Downloadable Resources
- Access on Mobile and TV
- Certificate of Completion
Program offerings
- Online course
- Learning resources
- 30-day money-back guarantee
- Unlimited access
- 8 articles
Course and certificate fees
Fees information
₹ 649 ₹2,799
certificate availability
Yes
certificate providing authority
Udemy
Who it is for
What you will learn
Greatest Unsolved Mysteries In The Universe certification course, the applicant will learn about how to understand the unsolved mysteries in the universe., to find areas in the universe where life could exist. The candidate will learn distances from brightnesses, doppler Effect, hubble Law, and exploding egg model. The participant will get to know about the big bang, antimatter, density and energy evolution of the universe, how old is universe, and the dark energy. The aspirant will master the giant black holes, first light in the universe, gamma-ray bursts, dark matter as well as solar system formation, and life in space.
The syllabus
Introduction
Section 2: Big Bang
- V2.1 Introduction - the Big Bang
- V2.2 Scale Factors and Redshifts
- V2.3 Density evolution of the universe
- V2.4 Energy evolution of the Universe
- V2.4b Energy Conservation
- V2.5 The Cosmic Microwave Background
- V2.6 Primordial Nucleosynthesis
- V2.7 Structure Formation
- V2.8 Matter/Antimatter
- V2.9 Conclusion
- Worked Example - scale factor, energies and densities
Section 3: Dark Energy
- V3.1 Introduction: How old is the universe?
- V3.2 The Fate of the Universe
- V3.3 First Clues to Dark Energy
- V3.4 Type 1a Supernova and the expansion of space
- V3.5 A surprising result
- V3.6 Conclusion: Dark Energy
- Reference Notes 3: Dark Energy
- Estimating the age of the universe
- Using supernovae to measure expansion rate
- A conversation at morning tea
Section 4: Giant Black Holes
- V4.1 The Discovery of Quasars
- V4.2 Quasar Luminosity
- V4.3 Effect of a Quasar
- V4.4 Clues - what are quasars?
- V4.5 Fusion power for quasars?
- V4.6 Gravity power for quasars
- V4.7 What does a quasar look like?
- V4.8 Feeding black holes
- V4.9 Conclusion
- Worked Example: Energy from Fusion
- Energy from Gravity Worked Example
- V4.2 Quasar Luminosity
- Mystery Part 4: High Resolution Bubble Spectra
Section 5: First Light In The Universe
- V5.1 Introduction
- V5.2 Stellar Nucleosynthesis
- V5.3 How much Iron?
- V5.4 n-body simulations
- V5.5 Reionisation
- V5.6 Quasar Reionisation
- V5.7 The First Galaxies
- V5.8 21 centimetre radiation and the first stars
- V5.9 EDGES Anomaly
- V5.10 Conclusions
- WE5.1 n-body step worked example
- WE5.2 Galactic Archeology
- Mystery Clues 5: Other Wavelengths
Section 6: Gamma-Ray Bursts
- V6.1 The Discovery of Gamma-Ray Bursts
- V6.2 Possible Energy Sources?
- V6.3 Black Hole and Neutron Star energies
- V6.4 Three Clues
- V6.5 Number CountsV6.5 Number Counts
- V6.6 Optical Counterparts
- V6.7 Counterpart Energy
- V6.8 Further out
- V6.9 Beaming
- V6.10 Short Hard Bursts
- V6.11 GW170817
- V6.12 Fast Radio Bursts
- 6.13 Conclusion
- Number Counts: Worked Example
- Survey prediction worked example
- Mystery Clue 6: Parallax and Motions
Section 7: Dark Matter
- V7.1 Introduction
- V7.2 Mass of the stars in a galaxy
- V7.3 Using acceleration to find mass
- V7.4 Predicting rotation curves
- V7.5 Observed galaxy rotation curves
- V7.6 Mass of M33
- V7.7 More evidence for Dark Matter and MOND
- V7.8 What is dark matter?
- V7.9 WIMP dark matter
- V7.10 WIMPS Disproved?
- Dark Matter Worked Example
- Mystery Part 7
Section 8: Solar System Formation
- V8.1 Clues to the formation of our solar system
- V8.2 Angular momentum and giant molecular cloud collapse
- V8.3 Simulations of Giant Molecular Cloud collapse
- V8.4 Protoplanetary disks
- V8.5 From dust to planets
- V8.6 Collisions
- Angular Momentum Worked Example
- Mystery Part 8
Section 9: Life in Space
- V9.1 Space is really big
- V9.2 Habitable zone
- V9.3 ...but life is really complicated!
- V9.4 How long will intelligence stay around?
- V9.5 The Fermi Paradox
- V9.6 Charley Lineweaver Interview
- V9.7 Conclusions
Instructors
Mr Paul R Francis
Astrophysics Researcher
Freelancer
Ph.D
Mr Brian Schmidt
Professor
Australian National ...
Ph.D
Articles
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