Sunday, June 20, 2010

Cosmic Collisions



universe is a breeding ground for violent impacts.

SUPERNOVA:Some stars behave as if it's better to burn out than to fade away. These stars end their evolutions in massive cosmic explosions known as supernovae.When supernovae explode they jettison matter into space at some 9,000 to 25,000 miles (15,000 to 40,000 kilometers) per second. These blasts produce much of the material in the universe—including some elements, like iron, which make up our planet and even ourselves. Heavy elements are only produced in supernovae, so all of us carry the remnants of these distant explosions within our own bodies.Supernovae add enriching elements to space clouds of dust and gas, further interstellar diversity, and produce a shock wave that compresses clouds of gas to aid new star formation.

Few stars become supernovae. Many stars cool in later life to end their days as white dwarfs and, later, black dwarfs.

Star Fusion

But massive stars, many times larger than our own sun, may create a supernova when their core's fusion process runs out of fuel. Star fusion provides a constant outward pressure, which exists in balance with the star's own mass-driven, inward gravitational pull. When fusion slows, outbound pressure drops and the star's core begins to condense under gravity—becoming ever denser and hotter.
White Dwarfs

Supernovae also occur in binary star systems. Smaller stars, up to eight times the mass of our own sun, typically evolve into white dwarves. A star condensed to this size, about that of Earth, is very dense and thus has strong enough gravitational pull to gather material from the system's second star if it is close enough.
If a white dwarf takes on enough mass it reaches a level called the Chandrasekhar Limit. At this point the pressure at its center will become so great that runaway fusion occurs and the star detonates in a thermonuclear supernova.
A supernova can light the sky up for weeks, and the massive transfer of matter and energy leaves behind a very different star.Typically only a tiny core of neutrons, a spinning neutron star, is left to evidence a supernova. Neutron stars give off radio waves in a steady stream or, as pulsars, in intermittent bursts.
If a star was so massive (at least ten times the size of our sun) that it leaves behind a large core, a new phenomenon will occur. Because such a burned-out core has no energy source to fuse, and thus produces no outward pressure, it may become engulfed by its own gravity and turn into a cosmic sinkhole for energy and matter—a black hole.

COSMIC COLLISIONS:
For example, we most likely have a moon because a protoplanet about the size of Mars careened into early Earth, breaking off a glob of material that coalesced in orbit around us.

We also most likely have dominion over the planet because another huge object crashed the dinosaur's party about 65 million years ago, triggering the mass extinction that allowed mammals to flourish.Considering that it's happened before, astronomers are anticipating that catastrophic collisions with Earth might happen again, and there are people who have dedicated their lives to understanding the risks and thinking up solutions.

Water Discovered on an Asteroid


Water has been spotted on an orbiting asteroid for the first time, according to a new study of a space rock that appears to be coated with frost..,the frost seems to be mixed with carbon-bearing material, according to results from two independent teams studying the asteroid, which is known as 24 Themis.,
Asteroids are believed to be the leftovers of planet formation, with compositions that have remained almost pristine for 4.6 billion years.The asteroid 24 Themis orbits about x million miles (480 million kilometers) from the sun. It's one of the largest asteroids in the main asteroid belt, which lies between the orbits of Mars and Jupiter. (Explore an interactive solar system).Unlike comets, which originate from beyond the orbit of Neptune, asteroids are thought to be relatively dry, since they orbit much closer to the sun.Asteroid composition could arrive as early as June, when the Japanese spacecraft Hayabusa returns to Earth potentially carrying the first sample taken directly from an asteroid. Hayabusa landed on the asteroid Itokawa in 2005. Although the craft failed to collect any formal samples, scientists think some dust from the space rock's surface might have accidentally gotten into the sampling chamber
By some accounts, Earth should have been too hot in its early days to have retained any of its original water. This has led some scientists to suspect our oceans were delivered by a barrage of asteroids or comets once the planet had cooled.

Monday, May 31, 2010

RAKESH REDDY


my best friend DOMA RAKESH REDDY..he was very good guy...wen ever i feel bore or depress he was to cheer me...from last one month we use to go nampally if i miss he was to make a call and remind me .....chalo jayenge....his bday was on 12th april...he use to remember mine by multiplying 12 with 2 =24 d day and month ..4 divided by 2=2

on 22nd may 2010 we went to ocean park after complition our semester exams...it was d last memory that i have with him...he will be always in hearts...ya one thing he was the only person who was able to understand my feelings....really am missing him...few words of him i can hear....he expired on 26th may 2010..i came to knew on 27th may....

Monday, May 10, 2010

SPACECRAFT

SPACECRAFT
By NIRMITH KUMAR MISHRA
(email: nirmithkumar.m08@mlrinstitutions.ac.in; ph: 9959984365; aero II B; MLRIT.)




Abstract:
A spacecraft is a craft or machine designed for spaceflight. Spacecraft are used for a variety of purposes, including communications, earth observation, meteorology, navigation, planetary exploration and space tourism. Spacecraft and space travel are common themes in works of science fiction.
On a sub-orbital spaceflight, a spacecraft enters space and then returns to the surface, without having gone into an orbit. For orbital spaceflights, spacecraft enter closed orbits around the Earth or around other celestial bodies. Spacecraft used for human spaceflight carry people on board as crew or passengers, while those used for robotic space missions operate either autonomously or telerobotically. Robotic spacecraft used to support scientific research are space probes. Robotic spacecraft that remain in orbit around a planetary body are artificial satellites. Only a handful of interstellar probes, such as Pioneer 10 and 11, Voyager 1 and 2 , and New Horizons, are currently on trajectories that leave our Solar System.
On a sub-orbital spaceflight, a spacecraft enters space and then returns to the surface, without having gone into an orbit. For orbital spaceflights, spacecraft enter closed orbits



around the Earth or around other celestial bodies. Spacecraft used for human spaceflight carry people on board as crew or passengers, while those used for robotic space missions operate either autonomously or telerobotically. Robotic spacecraft used to support scientific research are space probes. Robotic spacecraft that remain in orbit around a planetary body are artificial satellites. Only a handful of interstellar probes, such as Pioneer 10 and 11, Voyager 1 and 2 , and New Horizons, are currently on trajectories that leave our Solar System.
A spacecraft system comprises various subsystems, dependent upon mission profile. Spacecraft subsystems comprise the spacecraft "bus" and may include: attitude determination and control (variously called ADAC, ADC or ACS), guidance, navigation and control (GNC or GN&C), communications (Comms), command and data handling (CDH or C&DH), power (EPS), thermal control (TCS), propulsion, and structures. Attached to the bus are typically payloads.
Life support:
Spacecraft intended for human spaceflight must also include a life support system for the crew.
Attitude control:
A Spacecraft needs an attitude control subsystem to be correctly oriented in space and respond to external torques and forces properly. The attitude control subsystem consists of sensors and actuators, together with controlling algorithms. The attitude control subsystem permits proper pointing for the science objective, sun pointing for power to the solar arrays and earth-pointing for communications.
GNC:
Guidance refers to the calculation of the commands (usually done by the CDH subsystem) needed to steer the spacecraft where it is desired to be. Navigation means determining a spacecraft's orbital elements or position. Control means adjusting the path of the spacecraft to meet mission requirements. On some missions, GNC and Attitude Control are combined into one subsystem of the spacecraft.
Command and data handling:
The CDH subsystem receives commands from the communications subsystem, performs validation and decoding of the commands, and distributes the commands to the appropriate spacecraft subsystems and components. The CDH also receives housekeeping data and science data from the other spacecraft subsystems and components, and packages the data for storage on a data recorder or transmission to the ground via the communications subsystem. Other functions of the CDH include maintaining the spacecraft clock and state-of-health monitoring.
Power:
Spacecraft need an electrical power generation and distribution subsystem for powering the various spacecraft subsystems. For spacecraft near the Sun, solar panels are frequently used to generate electrical power. Spacecraft designed to operate in more distant locations, for example Jupiter, might employ a Radioisotope Thermoelectric Generator (RTG) to generate electrical power. Electrical power is sent through power conditioning equipment before it passes through a power distribution unit over an electrical bus to other spacecraft components. Batteries are typically connected to the bus via a battery charge regulator, and the batteries are used to provide electrical power during periods when primary power is not available, for example when a Low Earth Orbit (LEO) spacecraft is eclipsed by the Earth.
Thermal control:
Spacecraft must be engineered to withstand transit through the Earth's atmosphere and the space environment. They must operate in a vacuum with temperatures potentially ranging across hundreds of degrees Celsius as well as (if subject to reentry) in the presence of plasmas. Material requirements are such that either high melting temperature, low density materials such as Be and C-C or (possibly due to the lower thickness requirements despite its high density) W or ablative C-C composites are used. Depending on mission profile, spacecraft may also need to operate on the surface of another planetary body. The thermal control subsystem can be passive, dependent on the selection of materials with specific radiative properties. Active thermal control makes use of electrical heaters and certain actuators such as louvers to control temperature ranges of equipments within specific ranges.
A launch vehicle, like this Proton rocket, is typically used to bring a spacecraft to orbit.


Propulsion:
Spacecraft may or may not have a propulsion subsystem, depending upon whether or not the mission profile calls for propulsion. The Swift spacecraft is an example of a spacecraft that does not have a propulsion subsystem. Typically though, LEO spacecraft (for example Terra (EOS AM-1) include a propulsion subsystem for altitude adjustments (called drag make-up maneuvers) and inclination adjustment maneuvers. A propulsion system is also needed for spacecraft that perform momentum management maneuvers. Components of a conventional propulsion subsystem include fuel, tankage, valves, pipes, and thrusters. The TCS interfaces with the propulsion subsystem by monitoring the temperature of those components, and by preheating tanks and thrusters in preparation for a spacecraft maneuver.
Structures:
Spacecraft must be engineered to withstand launch loads imparted by the launch vehicle, and must have a point of attachment for all the other subsystems. Depending upon mission profile, the structural subsystem might need to withstand loads imparted by entry into the atmosphere of another planetary body, and landing on the surface of another planetary body.
Payload:
The payload is dependent upon the mission of the spacecraft, and is typically regarded as the part of the spacecraft "that pays the bills". Typical payloads could include scientific instruments (cameras, telescopes, or particle detectors, for example), cargo, or a human crew.
Ground segment:
The ground segment, though not technically part of the spacecraft, is vital to the operation of the spacecraft. Typical components of a ground segment in use during normal operations include a mission operations facility where the flight operations team conducts the operations of the spacecraft, a data processing and storage facility, ground stations to radiate signals to and receive signals from the spacecraft, and a voice and data communications network to connect all mission elements.[1]
Launch Vehicle:
The launch vehicle is used to propel the spacecraft from the Earth's surface, through the atmosphere, and into an orbit, the exact orbit being dependent upon mission configuration. The launch vehicle may be expendable or reusable.

AIRFOIL

"http://www.grc.nasa.gov/WWW/K-12/airplane/foil2.html"

This is a beta 1.5a version of the FoilSim II program, and you are invited to participate in the beta testing.

FoilSim II

With this software you can investigate how an aircraft wing produces lift by changing the values of different factors that affect lift.

There are several different versions of FoilSim II which require different levels of experience with the package, knowledge of aerodynamics, and computer technology. This web page contains the on-line student version of the program. It includes an on-line user's manual which describes the various options available in the program and includes hyperlinks to pages in the Beginner's Guide to Aerodynamics describing the math and science of airfoils. More experienced users can select a version of the program which does not include these instructions and loads faster on your computer. You can download these versions of the program to your computer by clicking on this yellow button:

http://www.grc.nasa.gov/WWW/K-12/airplane/foil2.html


everything is clearly explained in the link given above....