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NASA – The Rumor Mill

Posted by drdave on December 18, 2009

Following on the Tuesday meeting at NASA headquarters concerning revamping the governance structure, and Wednesday’s meeting between NASA administrator Charles Bolden and President Barack Obama, the rumor mill has been if full fury.

Wayne Hale offered this tweet: “Wondering if reports on Obama-Bolden meeting are accurate or just blather. No hard news has appeared.” To which Bob Jacobs, NASA’s deputy assistant administrator of Public Affairs responded: “Inaccurate. The meeting was informational, not decisional…”. Of course, that’s NASA’s spokesperson. Amy Klamper at Spacenews.com thinks “New Direction for NASA Could Wait Until February.”

Now comes Science magazine’s (AAAS) Insider report concerning the outcome of the meeting:

President Barack Obama will ask Congress next year to fund a new heavy-lift launcher to take humans to the moon, asteroids, and the moons of Mars, ScienceInsider has learned. The president chose the new direction for the U.S. human space flight program Wednesday at a White House meeting with NASA Administrator Charles Bolden, according to officials familiar with the discussion. NASA would receive an additional $1 billion in 2011 both to get the new launcher on track and to bolster the agency’s fleet of robotic Earth-monitoring spacecraft.

The major elements include:

  • Elimination of the Ares I rocket
  • Recommend Commercial development of Low Earth Orbit (LEO) launch capability for cargo and then crew.
  • Development of a smaller heavy lift rocket along the lines proposed by the old NLS (National Launch System) NASA investigated in the early 1990’s and revived by the Direct Team between 2005 and today.
  • Addition of $1 Billion to the Budget for NASA
  • European countries, Japan, and Canada would be asked to work on a lunar lander and modules for a moon base.
  • Focus on being able to perform a variety of missions including Near Earth Objects, Lagrange points, the Moon, the moons of Mars (Phobos and Deimos). See Option “5D”
  • Additional probes to the Moon, Mars and and the moons of Mars.

Immediate blow back is expected from Senator Richard Shelby, who has asked the Inspector General at NASA to investigate “corruption” within the Augustine Commission. Shelby stated that several Augustine panel members were registered lobbyists who took “direct advantage of their temporary roles on the Commission to further their personal business.” This has been interpreted as a shot across the bow in the fight over Ares I and the jobs it creates at the Marshall Space Flight Center in Shelby’s state of Alabama. Whose bow it was aimed at is in question, and it looks like an act of desperation.

However, as noted in our Wrap Up report on the Augustine Commission, time is of the essence with regard to jobs and the retention of skills associated with building the 8.4 meter External Tank used by the space shuttle and the proposed heavy launch vehicle derived from the shuttle. If the politicians resist the change that’s coming to NASA, they may lose everything.

Denials to the Science Insider article came immediately from NASA and the White House. NASA spokesman Morrie Goodman said the article was “speculation.” White House spokesman Nicholas Shapiro echoed that characterization.

Posted in Astronauts, Augustine Commission, Commercial Spaceflight, Direct, European Space Agency, Human Exploration, International Space Station, Moon, Mars and beyond, NASA, Robotic Exploration, Space, Space Exploration | Tagged: , , , , , , , , , , , , , , , , , , | Leave a Comment »

100 Best Open Science Courses on the Web

Posted by drdave on December 9, 2009

NSS member Neal Rudin offers us his selection of the 100 Best Open Science Courses on the Web.

It’s never too late or too early to start expanding your knowledge of science. With the wealth of free courses available on the web, that goal is easier than ever to achieve and can often be done without even leaving the house. The courses listed here will help you get started, offering resources on a wide variety of scientific fields from those that delve into the laws of the universe to those that explain the chemical reactions taking place in your own kitchen.

Physics
Use these courses to learn about both the basics and some of the more advanced topics in physics.

1. Fundamentals of Physics: In this course Professor Ramamurti Shankar will teach you about the basic principles of physics. [Yale]
2. Physics for Humanists: If you’ve always had more of a fondness for the social sciences rather than the natural sciences, this physics course is for you, examining physics issues from a more philosophical viewpoint. [Tufts]
3. Classical Mechanics: Check out this course to learn about physics fundamentals from Newtonian Mechanics to Kinetic Gas Theory. [MIT]
4. Electricity and Magnetism: Those who have a fascination with these subjects will get a chance to learn about everything from lightning to pacemakers in this course. [MIT]
5. Vibrations and Waves: This course will teach you the basics of vibrations and waves with additional lessons in topics like musical instruments to keep things interesting. [MIT]
6. Relativity: Get a better idea of what Einstein was really talking about in this course on special relativity. [MIT]
7. Quantum Physics: Quantum mechanics may sounds daunting, but this course will attempt to explain everything in a way you can understand. [MIT]
8. Particle Physics: Take physics studies to the high energy level in this course that looks at the activities of some of the smallest known particles. [MIT]
9. String Theory for Undergraduates: This entry level course will attempt to break string theory down, though some background in relativity or quantum mechanics is helpful for understanding it all. [MIT]
10. Atomic and Optical Physics: Try out this course to learn some of the principles of light and optics central to modern research projects. [MIT]
11. Introduction to Plasma Physics: Many people don’t know that matter has a fourth state: plasma. In this course you can learn what that is and what it means in physics terms. [MIT]
12. Introduction to Applied Nuclear Physics: While many people around the world rely on nuclear facilities to get power into their homes, few actually know much about how radiation functions. This course will help solve that and offers a range of knowledge on nuclear topics. [MIT]

Chemistry
Give these chemistry courses a try to get a handle on many aspects of the subject.

13. Freshman Organic Chemistry: Use the lessons in this course to teach yourself about the theories and principles of organic chemistry. [Yale]
14. Principles of Inorganic Chemistry: Once you’ve learned about organic chemistry, why not give the inorganic stuff a try with this course? [MIT]
15. Advanced Organic Chemistry: Those who have taken a more basic course in organic chemistry may want to try out the more advanced lessons found here. [MIT]
16. Physical Chemistry: In this course, students will learn about everything from quantum mechanics to chemical bonding. [MIT]
17. Kinetics of Chemical Reactions: Take this course to get some insights into the finer points of the energy produced when substances react with one another. [MIT]
18. Kitchen Chemistry: Chemistry doesn’t just happen in this classroom, as this course on kitchen chemistry proves. [MIT]
19. Principles of Chemical Science: This course is a great introduction to the basic principles of chemistry in both organic, inorganic and biological molecules. [MIT]
20. Organometallic Chemistry: Those who are looking for a challenge can take this course on organometallic transitions. [MIT]
21. Chemistry Laboratory Techniques: If you want to learn how to stay safe and create your own experiments in the chemistry lab, give the helpful video lessons in this course a try. [MIT]
22. Organic Structure Determination: This course will explain how modern chemists unravel the structure of organic molecules. [MIT]
23. Thermodynamics & Kinetics: Check out this course to learn more about equilibrium in systems as well as the impact of chemical reactions. [MIT]

Biology
Study cells, systems, plants and more through these free courses.

24. Introductory Biology: Those who want a good overview of the basics of biology will be well served with the material presented in this course. [MIT]
25. Microbiology: Take your study of biology down to the microbial level with this course on infection-causing bacteria and germs. [Tufts]
26. Molecular and Cell Biology: In this course you can learn more about how organic molecules function and get all the info you need on cellular structure and organization. [Berkeley]
27. Developmental Biology: This course will give you the tools you need to learn about how organisms develop, covering both vertebrate and invertebrate systems. [MIT]
28. Photosynthesis: Life from Light: Take a closer look at the process that keeps plants going and keeps them supplying us with oxygen in this course. [MIT]
29. The Fountain of Life: From Dolly to Customized Embryonic Stem Cells: This course will introduce some of the more basic and advanced concepts of genetic engineering and cloning to you. [MIT]
30. Introduction to Bioengineering: Learn both the fundamentals and the research applications of bioengineering through this course. [MIT]
31. Systems Biology: In this course, students can get a more mathematical and analytical way of looking at some of the big questions in modern biology. [MIT]
32. Biological Chemistry: You can mix both chemistry and biology in this course that explains the chemical processes inherent in many forms of life. [MIT]
33. Cellular Neurobiology: Take this course to learn more about the structure and function of the nervous system. [MIT]
34. Topics in Experimental Biology: Learn how to design and evaluate your own biological experiments in this course. [MIT]
35. Sophisticated Survival Skills of Simple Microorganisms: Microorganisms may be small, but they can also be tough, as this course explains by examining their defense mechanisms for stressors in a variety of natural settings. [MIT]

Astronomy
Take a closer look at some of the things going on in the space outside of our planet through these courses.

36. Frontiers and Controversies in Astrophysics: Professor Charles Bailyn explains some intriguing areas of astrophysics including extra-solar planets, black holes and dark matter in this course. [Yale]
37. Elementary Astronomy: Start with the basics in this introductory astronomy course. [Eastern Utah]
38. Exploring Black Holes: General Relativity & Astrophysics: Ever wonder what a black hole looks like? This course will teach you this and more as you explore many of the mysteries and myths surrounding these phenomena. [MIT]
39. Introduction to Astronomy: In this course you’ll get a chance to learn about the physics of the solar system and the universe beyond. [MIT]
40. Modern Astrophysics: Gain a better understanding of why objects in space do what they do with this course on all aspects of astrophysics. [MIT]
41. The Early Universe: This course will begin with how the universe began–with the big bang theory–and continue explaining theories of cosmology up to the present day. [MIT]
42. Cosmology: From radiation to red shifts, this course will explain many phenomena of the known universe. [MIT]
43. Astrophysics: This course is a more advanced take on astrophysics, tackling topics like dark matter and star structures. [MIT]
44. Particle Physics of the Early Universe: If you’ve already taken the other course on the Early Universe, expand your knowledge further with this course on some of the ways that modern particle physics explains things. [MIT]
45. The Solar System: Stay close to home with this course that examines the planets and happenings of our own solar system. [MIT]
46. Extrasolar Planets: Physics and Detection Techniques: This course offers you the chance to learn about new methods of seeking out and identifying planets well beyond the reach of our own solar system. [MIT]

Computer Science
These courses will help you embrace your inner techie.

47. Introduction to Computer Science and Programming: Even if you’ve never been a big programming geek, you can learn some handy fundamentals in this course. [MIT]
48. Structure and Interpretation of Computer Programs: In this course you’ll learn some of the basics of how computers and programming work. [MIT]
49. Artificial Intelligence: Try out this course to learn how artificial intelligence is developed and some of the theories behind how it works. [MIT]
50. Mathematics for Computer Science: Like many other branches of science, computer science is largely based on mathematics, and this course will show you the ropes. [MIT]
51. Great Ideas in Theoretical Computer Science: Take a look at some of the more theoretical, though not always practical, ideas in computer science in this course. [MIT]
52. Micro/Nano Processing Technology: Technology is always getting smaller and smaller, and this course explains how it’s even being taken to the nano level. [MIT]
53. Dynamic Systems & Control: Learn how computer systems are built, managed and controlled in this course. [MIT]
54. Theory of Computation: This course will touch on issues in computability theory, language theory and more. [MIT]
55. Computer Graphics: Give this course a try to learn how computer graphics are developed, programmed and implemented. [MIT]
56. Game Theory and Mechanism Design: Here you can see how game theory can be applied to systems like wireless communications networks. [MIT]
57. Ultrafast Optics: Learn how optics are working at literally the speed of light in this course. [MIT]
58. Advanced Topics in Cryptography: Learn what it takes to keep a computer network secure through this course. [MIT]

Geology
In these courses you can learn about the processes that shape Earth’s surface.

59. Introduction to Geology: Get an introduction to studying the physical features of the earth in this course. [Eastern Utah]
60. Atmosphere, Ocean and Climate Dynamics: Learn about the physics that determine how the oceans and atmosphere circulate in this course. [MIT]
61. Applications of Continuum Mechanics to Earth, Atmospheric, and Planetary Sciences: This course will give you some practical, real-life situations in which the continuum theory can be applied. [MIT]
62. The Environment of the Earth’s Surface: In this class, you’ll learn about the basic processes that govern changes in Earth’s surface. [MIT]
63. An Introduction to Fluid Motions, Sediment Transport, and Current-generated Sedimentary Structures: Take this course to learn more about fluid dynamics and how those principles can be applied to erosion, sedimentation and more. [MIT]
64. Basics of Impact Cratering & Geological, Geophysical, Geochemical, Environmental Studies of Some Impact Craters of the Earth: It might not seem like it, but Earth has been bombarded by objects from space and has the impact craters to prove it. This course will take a closer look at those craters. [MIT]
65. Structure of Earth Materials: Diamonds may be beautiful, but have you ever considered where they come from? This course will examine crystal structure and theory more closely. [MIT]
66. Sedimentary Geology: Learn about the process of sedimentation and what can be learned from it in this course. [MIT]
67. Essentials of Geophysics: This course will cover topics like gravity, geomagnetism, seismology, and geodynamics among others to give a more complete picture of geophysics. [MIT]
68. Past and Present Climate: Here you’ll find an introductory course on climate studies, offering a look back in time to see how climates have changed over the centuries as well. [MIT]
69. Surface Processes and Landscape Evolution: Get a better idea of how climate, tectonics and processes like erosion have shaped Earth’s surface in this course. [MIT]
70. Introduction to Seismology: Take this class to find out more about earthquakes and how seismic waves can tell us more about Earth’s interior. [MIT]

Environmental Science
Take one of these courses to learn about the science behind ecology, sustainability and other environmentally focused topics.

71. Fundamentals of Ecology: Learn how an ecosystem functions as a single unit and as individual entities in this course. [MIT]
72. Seminar in Environmental Science: Through this course you can become more knowledgeable about recent research in environmental science. [MIT]
73. Modeling Environmental Complexity: Here you’ll see how some of the more complex phenomena on earth are modeled and understood. [MIT]
74. Environmental Earth Science: Take this course to learn how the environment changes alongside some of the big changes that have happened with Earth’s surface. [MIT]
75. Complexity in Ecology: Here you can learn about issues in the complexity of ecology, looking at past models and coming up with new ways of organizing and obtaining data. [MIT]
76. Ecological Theory: This course requires some intense reading on both past and present theories of ecology. [MIT]
77. Chemicals in the Environment: Toxicology and Public Health: Learn how chemicals released into the environment can have a pretty negative impact on human health from this course. [MIT]
78. Water Quality Control: Here, you’ll learn how to model the distribution of substances into a water supply and the importance of maintaining quality water. [MIT]
79. Planning for Sustainable Development: Through this course you can see new ways that more sustainable communities are being developed. [MIT]
80. Environmental Microbiology: Microorganisms may be small but this course will show you what a big role they play in natural ecosystems. [MIT]
81. Strange Bedfellows: Science and Environmental Policy: Learn how scientific discoveries have pushed environmental policy making forward in this course. [MIT]

Health Science
In these courses you can learn about a wide range of medical issues.

82. Histology: Try out this course to learn about the structures and functions of human tissues and cells. [Tufts]
83. Genetics: Learn how genetic diseases are diagnosed and treated in this course. [Tufts]
84. Nutrition and Medicine: Here you can learn more about the big impact proper nutrition has on the health and well being of individuals. [Tufts]
85. Human Growth and Development: In this course you can learn how humans go from embryo to adult. [Tufts]
86. Principles of Human Disease: From contagious diseases to genetic ones, this course explains the modern understanding of diseases. [MIT]
87. Cancer Biology: From Basic Research to the Clinic: Learn what progress has been made in the fight against cancer in this course. [MIT]
88. Human Reproductive Biology: This course will teach you more than just how babies are made, focusing on the structure, function and even diseases of the reproductive system. [MIT]
89. Gastroenterology: Learn about the chemistry and biology of the digestive system in this course. [MIT]
90. Principles of Pharmacology: Most of us take medicines that are prescribed without giving much thought to how they came to be. This course will teach you how pharmacological agents are developed. [MIT]
91. Introduction to Neuroscience: Take this course to learn about some of the amazing and sometimes surprising ways the brain works. [MIT]
92. http://ocw.mit.edu/OcwWeb/Health-Sciences-and-Technology/HST-947Spring-2005/CourseHome/index.htm
: Learn how artificial intelligence is being used in medical care and diagnosis here. [MIT]
93. Brain Mechanisms for Hearing and Speech: In this course you can learn how your brain takes in information from auditory sources and formulates its own responses through vocal utterances. [MIT]

Miscellaneous
This assortment of courses covers things like evolution, meteorology and science writing.

94. Principles of Evolution, Ecology and Behavior: Professor Charles Bailyn explains some of the central issues to evolution and why we are the way we are in this course. [Yale]
95. Tropical Ecology and Conservation: This course focuses on methods that can be used to increase conservation efforts in the rainforests of the world. [Tufts]
96. Holographic Imaging: Holography might seem more science fiction than science, but this course will explain some of the fundamentals behind it and show you how it could be used. [MIT]
97. Geobiology: In this course you will investigate the way that life and the Earth itself have evolved side-by-side. [MIT]
98. Building Earth-like Planets: From Nebular Gas to Ocean Worlds: Do you know how planets are formed? This course will explains some of the best theories out there on how the planets came to be. [MIT]
99. Tropical Meteorology: Learn how weather works in some of the wettest places on Earth in this course. [MIT]
100. The Science Essay: Learn how best to write about science for the general public in this course touching on both English and science issues. [MIT]

Posted in Astronomy, Moon, Mars and beyond, Space, Technology | Tagged: , , , , , , , , , , | Leave a Comment »

International Space Station – Ralf Vandebergh – STS-129 Adds ELC2

Posted by drdave on December 2, 2009

ISS

ISS with Atlantis and ECL2.
Photograph used by permission of Ralf Vendebergh

Ralf Vandebergh continues to do his amazing work, even under adverse conditions. Here is a recent image of the International Space Station before and after Atlantis (STS-129) delivered the ExPRESS Logistics Carrier (ELC2). The module was mounted on the S3 truss. You can see Atlantis docked below the Space Station.

Ralf uses a 10 inch Newtonian telescope with a videocam eyepiece. He manually tracks the ISS and other objects across the sky. Due to atmospheric turbulence (its why stars twinkle), a portion of one image may be clear and another blurry. By judicious combination of various images from the video and that good old standby Photoshop, you can create a nice image.

Other recent events at the ISS are given below. Comparing the HTV-1 approach to ISS below with the recent ECL2 image (left), you can see the effects that weather play on the quality of the photographs.

You can follow Ralf on Twitter

ISS

Progress 34 (M-67) Resupply ship docked to ISS.
Photograph used by permission of Ralf Vendebergh

ISS

Japanese H-II Transfer Vehicle (HTV-1) approaches ISS.
Photograph used by permission of Ralf Vendebergh

Posted in Eye Candy, International Space Station, Space, Space Exploration, Space Settlement | Tagged: , , , | Leave a Comment »

Galaxy Zoo – Smashing Galaxies Together

Posted by drdave on November 29, 2009

Galaxy Zoo was started in July of 2007. NSS Phoenix first posted about Galaxy Zoo in June of 2008.

Hundreds of thousands of human eyeballs have yielded research results. One of the most recent peer-reviewed publications Galaxy Zoo Green Peas: Discovery of A Class of Compact Extremely Star-Forming Galaxies was published 7 September 2009 in Monthly Notices of the Royal Astronomical Society (Mon. Not. R. Astron. Soc.), and the Abstract was published on the Galaxy Zoo Forum. The Abstract begins: “We investigate a class of rapidly growing emission line galaxies, known as “Green Peas,” first noted by volunteers in the Galaxy Zoo project because of their peculiar bright green colour and small size, unresolved in SDSS imaging.”

The newest project is the dynamics of Galaxy Mergers. Once you register and login, you are presented with the Current Target of merging galaxies.Your task is to watch sample mergers played out dynamically and select one if it appears similar to the target. As the website makes clear:

This one takes a lot of patience. However, if you look at enough states, eventually you will get solutions that are close.

So click on “Take Me There” and get started.

Merger Target

Credit: Galaxy Zoo (Creative Commons License).

Select Similar Mergers

Credit: Galaxy Zoo (Creative Commons License).

In the center of the screen is your target merger. When you click on “More”, eight new simulations will be run, one at a time in each box. The “Animate” check box in the upper right shows the actual collision, rather than just the end result. If none of the collisions look like the target, then skip them and click on “More” again.

If you find a collision that resembles the target, click on the simulation and it will be added to the “Selected Sims” panel on the right. Remember, not selecting a simulation is just as important as selecting one. It lets the Galaxy Zoo researchers know that a particular set of conditions will not produce the target merger.

Once you have found a candidate, you can refine the simulation. Click on the “Enhance” tab.

To the left is an image of the Enhance screen for mergers. First, select the simulation from the right hand panel (double click). Then, you can “Add More Stars” and watch the simulation at greater detailNow the fun begins. You can adjust the orientation of the simulation by click and hold on the image and drag. Although the target merger can only be seen from the orientation shown, the sim can be rotated in three dimensions.

There are a lot of variables to play with: Mass, Velocity, Depth, Size, Angles 1 and Angles 2. You can flip the galaxies. For a detailed description of these variables, see the instructions. Once you have the collision as close as possible, click on “Save Sim”.

Adjustments are tricky and even slight variations in a variable can produce wildly divergent results.

Enhance and Adjust

Credit: Galaxy Zoo (Creative Commons License).

Happy Mergers.

Posted in Astronomy, Space | Tagged: , | 1 Comment »

Holiday Gifts – A Membership in The National Space Society

Posted by drdave on November 25, 2009

Rather than buying space books, we suggest our chapter members and friends give an NSS MEMBERSHIP as a holiday gifts instead. In fact, give three:

  • One regular “Adult” for a good friend
  • One “Student” for your child or grandchild
  • One “Senior Citizen” for a friend who remembers watching the Apollo lunar landings

Besides being a relatively low-cost gift that keeps on giving for an entire year (or at least every other month) to the lucky recipient(s), you’ll help expand the Phoenix chapter as well as the NSS as a whole.

Be sure to check the appropriate box with our chapter registration number (Phoenix = 504)

“Ad Astra”

NSS

Posted in National Space Society, Phoenix Chapter, Space | Tagged: , | Leave a Comment »

Proton Launches Eutelsat W7

Posted by drdave on November 25, 2009

A Russian Proton / Breeze M launch vehicle lifted off from Baikonur at 7:19 AM Phoenix time 24 November. 9 hours and 12 minutes later, the Breeze M released the Eutelsat W7 communications satellite in a Geo Stationary Orbit. International Launch Services (ILS) was responsible for the mission. The 5,627 kg W7 satellite was built by Thales Alenia Space and has a 15 year life expectancy.

Ignition

 

Ignition. Credit: www.zenite.nu

Liftoff

 

Liftoff. Credit: www.zenite.nu

Posted in Commercial Spaceflight, Rocket, Satellites, Space | Tagged: , , , , , , , | Leave a Comment »

The Augustine Commission – Final Report – Hits and Misses – Wrapped Up

Posted by drdave on November 23, 2009


“The Augustine Commission for Dummies”

(Part 1. Part 2. Part 3. Part 4. Part 5. Wrap Up.)

Given the intent of the politicians to fight for the funding their districts currently receive from the Constellation Program (CxP – the current program developing the Ares I and Ares V rockets) as well as go begging for more, and given the budget constraints the NASA faces, it is instructive to see where this course will end up. In the Senate, Richard Shelby has announced his intention to fight for Constellation and will try to increase funding to the Marshall Space Flight Center in Alabama. Senator Bill Nelson of Florida is fighting for Kennedy Space Center and all the jobs and funding there. In the House, Gabrielle Giffords of Arizona and Pete Olson of Texas have dug in their heels and reiterated their backing of the Constellation program (See Space News, 21 November 2009).

All this is taking place against the backdrop of the Augustine Commission’s Final Report, which has made it clear that Ares I is over budget and underpowered. As Jeff Greason said at the Committee deliberations, if Santa Clause gave us Ares I and Ares V tomorrow, we would have to scrap them immediately because they would be too expensive to operate.

The Forum at NasaSpaceFlight has been for many years the authoritative site for information on all things NASA. It has been home to the rebel alliance of NASA and industry engineers that have advocated the in-line shuttle derived launch vehicle for the past four years.

The source of this concern was former Administrator Michael Griffin’s decision in 2005 to replace the dual-launch, in-line shuttle derived architecture recommended by NASA engineers, with his personal choice of a small Ares I and a very large Ares V. Instead of building one rocket using existing shuttle components as Congress had directed, he would build two brand new rockets. This decision came just two weeks before the scheduled release of the NASA document on the Constellation program.

Now, four years later in 2009, when the in-line shuttle derived launch vehicle should have been making its first flight, we are five or six years away from Ares I making its first flight. The Shuttle is scheduled for retirement next year and America will have to buy seats on the Russian Soyuz to get to the International Space Station. And the International Space Station is scheduled for de-commissioning in 2015 and would be de-orbited into the Pacific Ocean.

This reality gave birth to the Augustine Commission and its Final Report. We have covered in detail the findings of the Committee. Now we look to consider the possible outcomes.

Philip Metschan (writing as ‘Phoegh’), a long time contributor to the Forum at NasaSpaceFlight, has produced a marvelous interactive series of graphics available at directlauncher.com that illustrate the options identified by the Augustine Commission.

The Budget and Time Line for these options are given in the following table. Included are destinations beyond low Earth orbit (LEO) and the impact of each option on the existing workforce.

Option Extra $ / Yr Through 2020 Through 2030 Moon NEO Depot Workforce
Option 1 $0 $99 B $205 B ? ? ? 50% Loss
Option 2 $0 $105 B $200 B ? ? ? 60% Loss
Option 3 $3 B $127 B $275 B 2025 ? ? 53% Loss
Option 4 $3 B $121 B $264 B 2030 ? ? 70% Loss
Option 4B $3 B $118 B $255 B 2029 ? 2026 25% Loss
Option 5A $3 B $128 B $272 B ? ? ? 75% Loss
Option 5B $3 B $123 B $268 B 2029 2026 2024 90% Loss
Option 5C $3 B $120 B $256 B 2030 2027 2025 30% Loss
Option 5D $1 B $116 B $239 B 2019 2022 2028 15% Loss

We can draw the following conclusions, which are illustrated in the Graphics mentioned earlier and shown below. We start with Option 1, the Program of Record (POR – Constellation) and the funding level provided in FY 2010:

  • Option 1 – Ares I crew vehicle is ready a year after the ISS is de-orbited (2015) and Ares V is completed in 2028 with no funds to conduct exploration. There is no Moon in the picture.
  • Option 2 – Scrap Ares I and substitute Commercial Crew Access to LEO. The money saved is used to keep the ISS operating until 2020. Ares V is completed in 2028 with no funds to conduct exploration. There is no Moon in the picture.
  • Option 3 – Add $3 Billion per year to the existing program. Ares I crew vehicle is ready a year after the ISS is de-orbited (2015) and Ares V is completed in 2019. The Moon is reached in 2025, but no other destinations beyond LEO can be funded.
  • Option 4 – Add $3 Billion per year to the existing program. Scrap Ares I and substitute Commercial Crew Access to LEO. The money saved is used to keep the ISS operating until 2020. Ares V is completed in 2023. The Moon is reached in 2030, but no other destinations beyond LEO can be funded.
  • Option 4B – Add $3 Billion per year to the existing program. Extend the Shuttle to 2015. Scrap Ares I and substitute Commercial Crew Access to LEO. The money saved is used to keep the ISS operating until 2020. Ares V is completed in 2023. Develop the Propellant Depot by 2026. The Moon is reached in 2030.
  • Option 5A – Add $3 Billion per year to the existing program. Scrap Ares I and substitute Commercial Crew Access to LEO. The money saved is used to keep the ISS operating until 2020. Scrap Ares V in favor of a smaller Ares V Lite, which is completed in 2023. Visit EML-1 or EML-2 in 2026. Visit a Near Earth Object (NEO) Sometime in the Future.
  • Option 5B – Add $3 Billion per year to the existing program. Scrap Ares I and substitute Commercial Crew Access to LEO. The money saved is used to keep the ISS operating until 2020. Scrap Ares V in favor of a commercial heavy launch capability, which is completed in 2021. Develop the Propellant Depot by 2024. Visit a Near Earth Object (NEO) in 2026 and Phobos in 2028. Return to the Moon in 2029.
  • Option 5C – Add $3 Billion per year to the existing program. Scrap Ares I and substitute Commercial Crew Access to LEO. The money saved is used to keep the ISS operating until 2020. Scrap Ares V in favor of a the Direct Team’s Jupiter 241, which is completed in 2022. Visit EML-1 or EML-2 in 2023. Develop the Propellant Depot by 2024. Visit a Near Earth Object (NEO) in 2027 and Phobos in 2029. Return to the Moon in 2030.

Those are the options explored by the Augustine Commission in their Final Report.

Notice, however, that there is one more slide, Option 5D. This is the architecture that was presented to the Augustine Commission during their first public session on 17 June 2009 by the Direct Team. It provides for:

  • Add $1 Billion per year to the existing program.
  • Extend Shuttle until 2012.
  • Scrap Ares I and develop the Jupiter Core (Jupiter 130) for carrying crew on Orion to LEO and ISS by 2014.
  • Develop Commercial Crew Access to LEO to replace the Jupiter 130 by 2015. Use Jupiter 130 for ferrying the few large payloads needed by ISS.
  • Continue ISS operations until 2020.
  • Scrap Ares V in favor of the Upper Stage for the Jupiter Core (Jupiter 241 or Jupiter 246), which is completed in 2017.
  • Visit EML-1 or EML-2 in 2018.
  • Orbit the Moon in 2019.
  • Visit a Near Earth Object (NEO) in 2022.
  • Visit Phobos in 2025.
  • Develop the Propellant Depot by 2028.

The key here is that the goal of expansion of human civilization into the Solar System is better served, is accomplished sooner, and costs less. Indeed, even without the additional $1 Billion per year, only the extension of the Shuttle operation need be eliminated.

Option 1
Option 2
Option 3
Option 4
Option 4B
Option 5A
Option 5B
Option 5C
Option 5D

Final Conclusions

  • Options 1, 2 and 3, which are favored by the politicians with space flight facilities, get us nowhere and cost far too much.
  • Options 4 and 4B get us to the Moon, but neither builds infrastructure for support of future exploration.
  • Options 5A, 5B and 5C builds the skills and infrastructure for space exploration, but leave us a crew to LEO gap of five to six years.
  • Option 5D builds the skills and infrastructure for space exploration, reduces the crew to LEO gap to one or two years, and gives the international community the ability to descend to the surface of the Moon and Mars.

Time is of the Essence

Finally, this note about the political realities. First, if a decision is delayed for four to six months while the politicians fight for every last bit of funding they want, the infrastructure on which the Jupiter program builds will be dismantled and Options 4B, 5C and 5D will be eliminated.

Second, Congress will likely decide that the Constellation program as currently envisioned is too costly for what will be developed and not worth throwing more money down the drain. Options 1, 2, 3, 4B and 5A will be eliminated.

Thus, only commercial crew and cargo capabilities will be funded. NASA will be reduced to research and contracting for services. The Marshall Space Flight Facility will have little purpose. And the politicians will lose most of the jobs and funding that their districts currently enjoy.

Special thanks are in order to Philip Metschan for permission to use screen shots of his presentation.

(Part 1. Part 2. Part 3. Part 4. Part 5. Wrap Up.)

Posted in Asteroids, Astronauts, Augustine Commission, Comets, Commercial Spaceflight, Direct, European Space Agency, Human Exploration, International Space Station, Moon, Mars and beyond, NASA, Rocket, Satellites, Space, Space Exploration, Space Settlement | Tagged: , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , | 6 Comments »

Intelsat 14 – Atlas V Launch

Posted by drdave on November 22, 2009

At 10:33 PM Phoenix time, we have eight (8) minutes and counting until a planned hold at T minus 4 minutes in the launch of the Atlas 5 carrying the Intelsat 14 satellite.

Intelsat 14 - Construction

Intelsat 14 under construction.
Credit: ULA TV

Intelsat 14 on Atlas 5

T minus 8 Minutes.
Credit: ULA TV

Launch is scheduled beginning at 10:50 PM Phoenix time. Weather is satisfactory.

We have a new T minus zero scheduled at 11:15 PM Phoenix time. Weather is green through the window. Extended hold due to reprogramming the flight computer (to take into account balloon data) taking longer than expected.

Weather Balloon Profile

Weather Balloon Profile.
Credit: ULA TV

Wind Shear Aloft

Wind shear aloft.
Credit: ULA TV

And the weather information updates are taking a long time. New launch time is 11:35 PM.

Wind shear aloft is a problem. Flight profile would not be good. A new balloon has been launched, and we are awaiting a new launch time.

And the weather aloft has now pushed the launch back to 11:55 PM Phoenix time. The US Air Force Range has approved the change. It is going to be a late night for all concerned.

Eye Candy Details

Eye Candy Details.
Credit: ULA TV

Details at T minus 4 minutes and holding for weather

More Details, at T minus 4 minutes and holding for weather.
Credit: ULA TV

The latest word from ULA is that “Things are improving with regard to developing a new flight program. They’re going to have one more shot to create a new program if this one doesn’t work, that will take us to the end of the window.”

All of this is based on the changing wind profiles aloft.

Weather aloft has improved. The launch director is polling all systems prior to coming out of the hold.

… and we are GO for LAUNCH!

T minus 3:48

T minus 3:48 and counting.
Credit: ULA TV

Ignition

Ignition.
Credit: ULA TV

Launch

Launch.
Credit: ULA TV

Ascent

Ascent.
Credit: ULA TV

Animation - Centaur Burn

Animation – Centaur Burn.
Credit: ULA TV

Animation - Centaur Burn

Mid Course Correction.
Credit: ULA TV

All systems are go. We are on the way to Geo Stationary Orbit.

Good Night All.

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The Augustine Commission – Final Report – Hits and Misses – Part 5

Posted by drdave on November 22, 2009

(Part 1. Part 2. Part 3. Part 4. Part 5. Wrap Up.)

In Part 1, we looked at the pieces strewn about our living room floor. In Part 2, we examined the Goals and Destinations in Chapter 3.0. And in Part 3, the three current Human Space Flight programs were reviewed (International Space Station, the Space Shuttle and the Constellation Program). In Part 4, we looked at the launch vehicles examined by The Augustine Commission.

Chapter 6 of the Augustine Commission Final Report deals with Program Options and Evaluation. This is one of the many contentious issues commentators have with the Commission. While they did select five possible exploration programs (Chapter 6), and while they did evaluate various launch vehicles (Chapter 5), the Committee seems to have ignored the possibility that different launch vehicles have greater or lesser ability to cover the five exploration programs. This failure may in the end, prove to be disastrous for human space exploration. As we write, the Space Shuttle infrastructure is being actively dismantled. The end result of failing to evaluate the physical infrastructure and the human infrastructure capable of supporting a Shuttle derived architecture may be that the United States is left with no heavy lift human space flight capability for at least the next several decades. We may have surrendered our space faring capability to Europe, China, Russia, India and Japan.

6.1 Evaluation Criteria

As noted by the Commission:

The Committee did not intend that the evaluation would generate a single numerical score; rather, it would provide a basis for comparison across options, highlighting the opportunities and challenges associated with each. Assigning weights to individual figures of merit is within the purview of the ultimate decision-makers.

Three primary evaluation dimensions were identified:

  • Benefits to Stakeholders
  • Risk
  • Budget Realities

These three dimensions were expanded into 12 criteria for comparing the options.

  • Exploration Preparation
  • Technology Innovation
  • Science Knowledge
  • Expanding and Protecting Human Civilization
  • Economic Expansion
  • Global Partnerships
  • Public Engagement
  • Schedule and Programmatic Risk
  • Mission Safety Challenges
  • Workforce Impact
  • Programmatic Sustainability
  • Life-Cycle Cost

6.2 Key Decisions and Integrated Options

6.2.1 Key Decisions

1. What should be the future of the Space Shuttle?
2. What should be the future of the International Space Station (ISS)?
3. On what should the next heavy-lift launch vehicle be based?
4. How should crews be carried to low-Earth orbit?
5. What is the most practicable strategy for exploration beyond low-Earth orbit?

6.2.2 Integrated Options

The Committee identified five basic options: One based on the Program of Record (POR – Constellation – Ares I and V, Orion and Altair), and four alternatives. Options 2 and 3 were budget compatable alternatives to the POR. Option 4 was a Moon First program (with two variations), and Option 5 was the Flexible Path (avoiding the gravity well of the Moon).

6.2.3 Methodology for Analyzing the Integrated Options

Two budgets were used. The “Constrained Budget” used the FY 2010 budget, while the “Less Constrained Budget” allowed for an increase by 2014 of $3 Billion per year higher than FY 2010.

6.2.4 Reference Cases of the Entirely Unconstrained Program of Record

The Program of Record was evaluated and found to be a total of $45 Billion over the FY 2010 budget by 2020, wherein it is $5 Billion a year over FY 2010 in 2016 and $7 Billion per year over FY 2010 in 2019.

6.3 Integrated Options Constrained to the FY 2010 Budget

6.3.1 Evaluation of Integrated Options 1 and 2

Option 1 was found to allow for rocket development, but lacked funds for exploration. Option 2 extends the lifetime of the ISS, delays rocket development, and has no funds for exploration.

6.3.2 Examination of alternate budget guidance

The Committee found no alternatives to Options 1 or 2 that were viable under the FY 2010 budget. This conclusion has been disputed.

6.4 Moon First Integrated Options Fit to the Less-Constrained Budget

6.4.1 Evaluation of Integrated Options 3 and 4

Option 3 was to execute the POR under a less constrained budget. The ISS is de-orbited in 2010, and the Shuttle flies the remaining missions into 2011. Human lunar return occurs in the mid 2020s and the lunar base becomes operation late in the decade. An alternate extending ISS to 2020 was found to push these dates out by three to four more years.

Option 4 uses the less constrained budget, scraps Ares I and substitutes commercial crew services by 2016 It extends the ISS to 2020. Ares V is scrapped in favor of a dual-launch Ares V Lite vehicle for lunar missions.

Option 4A retires the Shuttle in 2011, while Option 4B extends the Shuttle to 2015 and develops a Shuttle Derived Heavy Lift vehicle in place of Ares V Lite.

6.4.2 Examination of the key decision on the ISS extension

Given the International Partnerships that have been developed, and the fact that the extension to 2020 would only delay the lunar return by a few years, the Committee found that the extension provides greater value than ending the ISS mission.

6.4.3 Examination of the key decision on Ares V vs. Ares V Lite dual launch

Baseline Ares V has more launch capability than the Saturn V, but current NASA studies show that when used in combination with Ares I, it does not have enough launch capability to robustly deliver the currently planned landing and surface systems to the Moon.

The Committee concluded that Ares V Lite represents less development risk, likely will reduce costs and provides more substantial margin for the lunar mission.

6.4.4 Examination of the key decision on the provision of crew transport to low-Earth orbit

Commercial crew services, based on a high-reliability rocket with a capsule and launch escape system could significantly reduce development costs, as well as lower operating costs.

6.4.5 Examination of the key question on Shuttle extension

The Committee favored early retirement of the Shuttle (2010 or 2011), although they noted several advantages to Shuttle extension to 2015, including up-mass and down-mass capability and workforce retention.

6.5 Flexible Path Integrated Options Fit to the Less-Constrained Budget

6.5.1 Evaluation of Integrated Option 5

Option 5 operates the Shuttle into 2011 and extends the International Space Station mission until 2020. A variety of destinations beyond low earth orbit are possible. The Committee developed three variants of this option.

  • Option 5A develops the Ares V Lite, visits the Lagrange points, near Earth objects, on-orbit refueling and achieves a lunar return by the end of the 2020s.
  • Option 5B develops commercial heavy lift capability, restructures NASA, and follows a similar mission profile as 5A, but on a slower time line.
  • Option 5C scraps Ares V Lite and develops a Shuttle Derived Heavy Lift vehicle. 5C follows a similar mission profile as 5A, but on a slower time line.

6.5.2 Examination of the key question on Ares V family vs. Shuttle-derived heavy launcher

While the Shuttle derived in-line launch vehicle (SDLV) with two four-segment solid rocket motors (SRM) and the 8.4 meter external tank (ET) was the 2005 ESAS candidate for the cargo vehicle, it was forced to evolve into the Ares V due to the problems encountered with the underpowered Ares I. For some reason, the Committee decided that in order to match the capabilities of the Ares V, or the Ares V Lite dual-launch mission, that there had to be three SDLV launches. Therefore, operations would be more costly.

This is a clear Committee miss, as the current planned lunar return missions can be accomplished with good margin by a dual-launch SDLV program, thus costing less than the Ares V Lite. There is no need for the enhanced capabilities of the dual-launch Ares V Lite.

6.5.3 Examination of the key question on NASA heritage vs. EELV-heritage super-heavy vehicles

The Committee considers the EELV-heritage super-heavy vehicle to be a way to significantly reduce the operating cost of the heavy lifter to NASA in the long run. It would be a less-capable vehicle, but probably sufficiently capable for the mission. Reaping the long-term cost benefits would require substantial disruption in NASA, and force the agency to adopt a new way of doing business.

6.6 Comparisons Across Integrated Options

6.6.1 Cross-option comparisons

The Flexible Path program (Option 5A) scores more highly than the Baseline (Option 3) on 9 of the 12 criteria outlined in section 6.1 ( See figure 6.6.1-1). The higher rankings include:

  • Exploration Preparation (due to much more capable launch system)
  • Technology (due to investment in technology)
  • Science (because of more places visited)
  • Human Civilization (due to the ISS extension)
  • Economic Expansion (because of commercial involvement in space elements and crew transport)
  • Global Partnerships (gained by extending the ISS)
  • Public Engagement (by visiting more new locations, and doing so each year)
  • Schedule (exploring beyond low-Earth orbit sooner)
  • Life-Cycle Costs (due to commercial crew services)

6.6.2 Examination of the key question on exploration strategy

Three exploration strategies were examined in Chapter 3. The choice of Mars First was found not to be viable due to technological problems. Two strategies remained:

  • Moon First on the Way to Mars, with surface exploration focused on developing capability for Mars.
  • Flexible Path to Mars via the inner solar system objects and locations, with no immediate plan for surface exploration, then followed by exploration of the lunar and/or Martian surface.

The Moon first is favorable to lunar science and exploration (although much can be done robotically). The Flexible Path missions explore more of the Solar System, while initially doing less on the Moon. Flexible Path has the advantage of developing infrastructure for deep space exploration, including the moons of Mars and Mars itself. The Committe notes that:

Considering that we have visited and obtained samples from the Moon, but not near-Earth objects or Mars, and also that the Flexible Path develops the ability to service space observatories, the Science Knowledge criterion slightly favors the Flexible Path. Broadly, the more complex the environment, the more astronaut explorers are favored over robotic exploration. In practice, this means that astronauts will offer their greatest value-added in the exploration of the surface of Mars.

Final Scoring

Although the Augustine Commission did not publish a final tally of the scores (for reasons they made clear), the following table does compare and tabulate the scores.

Option Description Science Safety Cost Schedule NASA / Industry Jobs US Skills Retention Exploration Capability Technology Space Colony Potential Commercial Benefit Public Engagement international Cooperation Sustainability Total
1 The Status Quo 0 0 0 -2 -1 -1 -2 -2 -2 -1 -1 -2 -1 -15
2 ISS Extension plus Moon 0 0 1 -2 -1 -1 -2 1 -1 1 -1 0 0 -5
3 Status quo + $3 B 1 -1 0 0 0 -1 0 0 0 0 0 -2 0 -3
4 Shuttle + Moon 1 -1 1 0 0 -1 1 1 1 1 0 0 0 4
4B Shuttle 2015 + Moon 1 -1 0 0 0 0 1 1 1 1 0 0 1 5
5A Flexible Path + Ares Lite 2 -1 1 1 0 -1 2 1 1 2 1 0 0 9
5B Flexible Path + Commercial 2 -2 2 1 0 -1 1 2 1 2 1 0 -1 8
5C Flexible Path + Jupiter 241 2 -2 0 1 0 -1 1 1 1 2 1 0 1 7

Option 5D: We will have more to say about this proposal in our final segment: “Wrapped Up” or “The Augustine Commission for Dummies”.

Option Description Science Safety Cost Schedule NASA / Industry Jobs US Skills Retention Exploration Capability Technology Space Colony Potential Commercial Benefit Public Engagement international Cooperation Sustainability Total
5D Flexible Path + Direct 2 -2 1 1 1 1 2 1 1 2 1 1 1 13

(Part 1. Part 2. Part 3. Part 4. Part 5. Wrap Up.)

Posted in Asteroids, Astronauts, Augustine Commission, Comets, Commercial Spaceflight, Direct, Human Exploration, International Space Station, Moon, Mars and beyond, NASA, Robotic Exploration, Rocket, Satellites, Space, Space Exploration, Space Settlement, Technology | Tagged: , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , | 5 Comments »

STS-129 – Docking with ISS

Posted by drdave on November 18, 2009

This morning (7:45 AM Phoenix), we find Atlantis 27,000 feet from the International Space Station. Nicole Stott will be returning on Atlantis following her mission on the ISS. Live coverage on NASA TV.

Control Room

Control Room prior to Docking.
Image Credit: NASA TV

Atlantis Location and Attitude

Atlantis Location and Attitude.
Image Credit: NASA TV

Three miles from the ISS and Atlantis completes a short burn.

Nicole comments her ticket is stamped and ready to go for the return flight home.

8:11 AM Phoenix (10:11 EST) and Atlantis is 8,000 feet away. Docking is scheduled for 9:53 AM Phoenix time (11:53 EST)

And at 8:20, Atlantis is less than 5,000 feet away from ISS.

Approach Display

Control Room Approach Display.
Image Credit: NASA TV

Atlantis Go for 600 Foot Approach

Atlantis Go for 600 Foot Approach.
Image Credit: NASA TV

ISS from Atlantis

ISS from Atlantis.
Image Credit: NASA TV

Atlantis Closing

Atlantis Closing.
Image Credit: NASA TV

Cargo Bay Open

Cargo Bay Open.
Image Credit: NASA TV

Atlantis Closing on the IIS

Atlantis Closing on the IIS.
Image Credit: NASA TV

At about 8:53 AM (10:53 EST), Atlantis will perform the heat shield inspection back flip.

Tile Inspection

Tile Inspection.
Image Credit: NASA TV

Closing Display

Closing Display.
Image Credit: NASA TV

Shuttle Atlantis closing at 0.2 feet per second with 20 minutes to go until docking.

Speed is now down 0.17 foot per second as Atlantis is less than 100 feet away from the docking port.

50 feet.

Final approach maneuver at 30 feet.

20 feet. 15 feet. 10 feet. 5 feet.

Docking confirmed at 9:51 AM Phoenix time.

Posted in Astronauts, Human Exploration, International Space Station, NASA, Space, Space Shuttle | Tagged: , , , , | 1 Comment »