Tuesday, 18 March 2008

Indonesia Aerospace Engineering School

Disusun Ulang Oleh:

Arip Nurahman
Department of Physics
Faculty of Sciences and Mathematics, Indonesia University of Education

and

Follower Open Course Ware at Massachusetts Institute of Technology
Cambridge, USA
Department of Physics
http://web.mit.edu/physics/
http://ocw.mit.edu/OcwWeb/Physics/index.htm
&
Aeronautics and Astronautics Engineering
http://web.mit.edu/aeroastro/www/
http://ocw.mit.edu/OcwWeb/Aeronautics-and-Astronautics/index.htm


















Aerospace engineering is the branch of engineering behind the design, construction and science of aircraft and spacecraft. Aerospace engineering has broken into two major and overlapping branches: aeronautical engineering and astronautical engineering. The former deals with craft that stay within Earth's atmosphere, and the latter deals with craft that operate outside of Earth's atmosphere. While "aeronautical" was the original term, the broader "aerospace" has superseded it in usage, as flight technology advanced to include craft operating in outer space.[1] Aerospace engineering is often informally called rocket science.

Contents

 

Aerospace Engineering

Aerospace engineering is a complex, rapidly changing field whose primary application is the design and development of flight vehicles such as aircraft, missiles, spacecraft and satellites.

Aerospace engineering is also important and applicable to other vehicles and systems such as submarines, automobiles, trucks and rapid transit, and can include advanced robotics, exotic materials and computational simulations.


The goals of Indonesia Aerospace Engineering School, aerospace engineering program are to

(a) using a high quality faculty, provide a comprehensive aerospace engineering education that develops in students the fundamental skills necessary for the design, synthesis, analysis and research development of aircraft, spacecraft and other high technology flight systems; and

(b) prepare students for the aerospace engineering profession and related fields by developing in them the attributes needed so that they can contribute successfully to society and the engineering profession now and in the future.

The curriculum includes

(a) sciences and mathematics to provide a foundation for engineering, aerospace engineering and design; and

(b) humanities, social sciences, visual and performing arts, and international and cultural diversity topics to ensure an awareness of cultural heritage.

In the junior and senior years, coursework includes aerodynamics, structures and materials, propulsion, dynamics and control, and astrodynamics. These studies provide a strong fundamental basis for specialization and advanced study, while technical electives allow exploration of special interests.

Advanced courses emphasize new technologies and skills, and a senior-level design-build-fly sequence requires students to work in teams to design an aerospace system, such as an aircraft, rocket, or spacecraft.
All courses utilize modern computational tools. The department has an extensive array of computing resources including PCs and workstations.

Studies are supported by well-equipped laboratories: water and wind tunnels for aerodynamic analysis, a jet engine test facility, research aircraft, a flight simulator, and a state-of-the-art materials and structures testing facility.

Aerospace engineering at Texas A&M

More about aerospace engineering


Welcome to the Aerospace Engineering Department at Texas A&M University!

Find answers to frequently-asked questions:

What is an aerospace engineer?
Why should you choose aerospace engineering at Texas A&M?
Want to visit Texas A&M and the Aerospace Engineering Department?
Want to know about our Undergraduate or Graduate programs?
Need some K-12 resources?







































Semoga Bermanfaat

Wednesday, 12 March 2008

What Is the Universe Made Of ?



By:

Arip Nurahman

Department of Physics, Faculty of Sciences and Mathematics

Indonesian University of Education



Every once in a while, cosmologists are dragged, kicking and screaming, into a universe much more unsettling than they had any reason to expect. In the 1500s and 1600s, Copernicus, Kepler, and Newton showed that Earth is just one of many planets orbiting one of many stars, destroying the comfortable Medieval notion of a closed and tiny cosmos. In the 1920s, Edwin Hubble showed that our universe is constantly expanding and evolving, a finding that eventually shattered the idea that the universe is unchanging and eternal. And in the past few decades, cosmologists have discovered that the ordinary matter that makes up stars and galaxies and people is less than 5% of everything there is.

Grappling with this new understanding of the cosmos, scientists face one overriding question: What is the universe made of?
This question arises from years of progressively stranger observations. In the 1960s, astronomers discovered that galaxies spun around too fast for the collective pull of the stars' gravity to keep them from flying apart. Something unseen appears to be keeping the stars from flinging themselves away from the center: un illuminated matter that exerts extra gravitational force. This is dark matter.

Over the years, scientists have spotted some of this dark matter in space; they have seen ghostly clouds of gas with x-ray telescopes, watched the twinkle of distant stars as invisible clumps of matter pass in front of them, and measured the distortion of space and time caused by invisible mass in galaxies. And thanks to observations of the abundances of elements in primordial gas clouds, physicists have concluded that only 10% of ordinary matter is visible to telescopes
But even multiplying all the visible "ordinary" matter by 10 doesn't come close to accounting for how the universe is structured.

When astronomers look up in the heavens with powerful telescopes, they see a lumpy cosmos. Galaxies don't dot the skies uniformly; they cluster together in thin tendrils and filaments that twine among vast voids. Just as there isn't enough visible matter to keep galaxies spinning at the right speed, there isn't enough ordinary matter to account for this lumpiness. Cosmologists now conclude that the gravitational forces exerted by another form of dark matter, made of an as-yet-undiscovered type of particle, must be sculpting these vast cosmic structures. They estimate that this exotic dark matter makes up about 25% of the stuff in the universe--five times as much as ordinary matter.

But even this mysterious entity pales by comparison to another mystery: dark energy. In the late 1990s, scientists examining distant supernovae discovered that the universe is expanding faster and faster, instead of slowing down as the laws of physics would imply. Is there some sort of antigravity force blowing the universe up?
All signs point to yes.

Independent measurements of a variety of phenomena--cosmic background radiation, element abundances, galaxy clustering, gravitational lensing, gas cloud properties--all converge on a consistent, but bizarre, picture of the cosmos. Ordinary matter and exotic, unknown particles together make up only about 30% of the stuff in the universe; the rest is this mysterious anti-gravity force known as dark energy.

This means that figuring out what the universe is made of will require answers to three increasingly difficult sets of questions. What is ordinary dark matter made of, and where does it reside? Astrophysical observations, such as those that measure the bending of light by massive objects in space, are already yielding the answer. What is exotic dark matter? Scientists have some ideas, and with luck, a dark-matter trap buried deep underground or a high-energy atom smasher will discover a new type of particle within the next decade.

And finally, what is dark energy? This question, which wouldn't even have been asked a decade ago, seems to transcend known physics more than any other phenomenon yet observed. Ever-better measurements of supernovae and cosmic background radiation as well as planned observations of gravitational lensing will yield information about dark energy's "equation of state"--essentially a measure of how squishy the substance is. But at the moment, the nature of dark energy is arguably the murkiest question in physics--and the one that, when answered, may shed the most light.

Monday, 10 March 2008

Two Techniques Produce Slow Antihydrogen

SPECK, ANDREW J., (Williams College) 2000. (Harvard) 2002.

http://www.physics.harvard.edu/Thesespdfs/speck.pdf