Wednesday, 7 March 2018

Astronaut Selection and Training


History of Astronaut Selection

Man’s scope of space exploration has broadened since the first U.S. manned space flight in 1961. But the nation will never forget the original seven pilots who focused our vision on the stars. In 1959, NASA asked the military services to list their members who met specific qualifications. In seeking its first astronauts, NASA required jet aircraft flight experience and engineering training. Height should be no more than 5feet 11 inches because of limited cabin space available in the mercury space capsule being designed. After many intense physical and psychological screenings, NASA selected seven men from an original field of 500 candidates. They were Air Force Captains   L. Gordon Cooper Jr., Virgil “Gus” Grissom and Donald K. “Deke” Slayton, Marine Lieutenant Colonel John H. Glenn Jr., Navy Lieutenant M. Scott Carpenter and Navy Lieutenant Commanders Walter M. Schirra Jr., Alan B. Shepard.

By 1964, prime emphasis had shifted away from flight experience and toward superior academic qualification. Applicants were invited on the basis of educational background alone. These were the scientist astronauts, so called because, as a minimum, applicants were required to have a doctorate level degree equivalent experiences in the natural sciences, medicine or engineering.

Since selection of the first class of astronauts, many men and women have pursued and realized their dreams of flying in space. Thus all began by submitting their applications to become astronauts.

Basic Qualification Requirements

The Astronaut Candidate selection process was developed to select highly qualified individuals for human space programs.  Astronaut Candidates are selected on an as needed basis. Both civilian and military personnel are considered for the program. Applicants, all of whom must be citizens of the United States, must meet a series of minimum requirements.
          
The requirements for Astronaut Candidates are a bachelor degree from an accredited institution in engineering, biological science, physical science or mathematics. Quality of academic preparation is important. Degree must be followed by at least 3 years of related, progressively responsible, professional experience or at least 1,000 hours of pilot-in-command time in jet aircraft. An advanced degree is desirable and may be substituted for experience as follows: master’s degree 1 year of experience, doctoral degree 3 years of experience. Teaching experience, including experience at the k-12 levels, is considered to be qualifying experience for the Astronaut Candidate position: therefore, educators are encouraged to apply.

Additional requirements include the ability to pass the NASA long-duration space flight physical, which includes the following specific requirements: Distant and near visual acuity must be correctable to 20/20 in each eye, blood  pressure not to exceed 140/90 measured in a sitting position, and the candidate must have a standing height between 62 and 75 inches.
Applicants for the Astronaut Candidate Program must meet the basic education requirements for NASA engineering and scientific positions, specifically, successful completion of standard professional curriculum in an accredited college or university leading to at least a bachelor’s degree with major study in an appropriate field of engineering, biological sciences, or mathematics. The following degree fields, while related to engineering and the sciences, are not considered qualifying: degrees in technology (engineering technology, aviation technology, medical technology, etc.); degrees in psychology (except for clinical psychology, physiological psychology, which are qualifying); degrees in nursing; degrees in exercise physiology and similar fields; degrees in social sciences(geography, anthropology, archaeology, etc.); and degrees in aviation, aviation management or similar fields.

Astronaut selection and training

Following the preliminary screening of applications, a week long process of personal interviews, medical screening, and orientation are required for both civilian and military applicants under final consideration. Once final selections have been made, all applicants are notified of the outcomes.

Selected applicants are designated Astronaut Candidates and are assigned to the Astronaut Office at the Johnson Space Centre (JSC) IN Houston, Texas. The Astronaut Candidate undergo a training and evaluation period lasting approximately 2 years. During this time they will participate in the basic Astronaut Candidate training program, which is designated to develop the knowledge and skills required for formal mission training upon selection for a flight. Military proficiency in NASA aircraft during their candidate period.

As a part of Astronaut Candidate training program, candidates are required to complete military water survival before beginning their flying syllabus, and become SCUBA qualified to prepare them for spacewalk. Consequently, all Astronaut Candidates are required to pass a swimming test during their first month of training. They must swim 3 lengths of a 25-metre pool without stopping, and then swim 3 lengths of the pool in a flight suit and tennis shoes with no time limit. They must also tread water continuously for 10 minutes wearing a flight suit.

Candidates are also exposed to the problems associated with high (hyperbaric) and low (hypobaric) atmospheric pressures in the altitude chambers and learn to deal with emergencies associated with these conditions. In addition, Astronaut Candidate are given exposure to the microgravity of space flights in a modified jet aircraft as it performs parabolic manoeuvres that produce periods of weightlessness for about 20 seconds. The aircraft then returns to the original altitude and the sequence is repeated up to 40 times in a day.

Final selection as an astronaut will depend upon satisfactory completion of the training evaluation period. Graduation from the Astronaut Candidate Program will require successful completion of the following: International Space Station systems training, Extravehicular Activity skills training, Robotics skills training, Russian Language training, and aircraft flight readiness training. Civilian candidates who successfully complete the training and evaluation and are selected as astronauts become permanent Federal employees. Civilian candidates who are not selected s astronauts may be placed in other positions within NASA, depending upon agency requirements and workforce constraints at that time. Equal opportunity in employment means opportunity not just for some but for all. NASA provides equal opportunity in Federal employment regardless of race, colour, gender, national origin, religion, age, non-disqualifying physical or mental disability, genetic information, sexual orientation, status as a parent, or gender identity.

Pay and Benefits

Salaries for civilian Astronaut Candidates are based on the Federal Government’s General Schedule pay scales for grades GS11 through GS14, and are set in accordance with each individual’s academic achievements and work experience. Selected military personnel will be detailed to JSC, but will remain in an active duty status for pay, benefits, leave, and other similar military matters.

Astronaut Responsibilities

Astronauts are involved in all aspects of on-orbit operations of the International Space Sation (ISS). This includes extravehicular activities (spacewalks), robotics operations using the remote manipulator system, experiment operations, and onboard maintenance tasks. Astronauts are required to have a detailed knowledge of the space station systems, as well as detailed knowledge of the operational characteristics, mission requirements and objectives, and supporting systems and equipment for each experiment on their assigned missions. Long-duration missions aboard the space station generally last from 3 to 6 months. Training for long-duration missions is arduous and takes approximately 2 to 3 years beyond the initial training and evaluation period. This training requires extensive travel, including long periods in other countries training with our international partners. Tips to and from the space station will initially be aboard other future spacecraft presently being developed.

Astronaut Formal Training

The astronaut begin their formal training program during their year of candidacy by reading training manuals and by taking computer-based training lessons on the various vehicle systems.
The next step in the training process involves the spacecraft systems trainers. The astronauts are trained to operate each system, to recognize malfunctions, and to perform corrective actions if needed.

The Sonny Carter Training Facility, or Neutral Buoyancy laboratory (NBL), provides controlled neutral buoyancy operations in the facility water tank to simulate the zero-g or weightless condition that is experienced by the crew during space flight. It is an essential tool for the design, testing, and development of the International Space Station and future NASA programs. For the astronaut, the facility provides important preflight training in becoming familiar with planned crew activities and with the dynamics of body motion under weightless conditions in order to perform spacewalks.
Several full-scale mockups and trainers are also used to train astronauts. These mockups and trainers are used for onboard systems orientation and habitability training. Astronauts practice meal preparation, equipment stowage, trash management, use of cameras, and experiment operations.
Astronauts, who are pilots maintain flying proficiency by flying 15 hours per month in NASA’s fleet of two-seat T38 jets. Non-pilot astronauts fly a minimum of 4 hours per month. The T38 is used for flight readiness training to help the astronauts become adjusted to the flight environment, including the g-forces experienced on launch.

The astronaut training is designed to prepare personal for space flight on the International Space Station, Russian Soyuz spacecraft, NASA’s Orion vehicle, and future spacecraft.

International Space Station Program Description

The International Space Station is the largest international scientific and technological endeavor ever undertaken. The space station is a permanent scientific laboratory in which gravity, temperature and atmospheric pressure can be manipulated for scientific and engineering pursuits impossible in ground-based laboratories.

The International Space Station marked its 10th anniversary of continuous human occupation on Nov.2, 2010. Since Expedition 1, which launched in October 2000, the space station has been visited by more than 200 individuals, travelled more than 1.5 billion miles (equivalent to eight to the Sun) and orbited the Earth more than 60,000 times.

NASA and the world have learned much about building in space and about how humans and spacecraft systems function on orbit. But there is much more to do and learn. The voyage of research and discovery is just beginning as NASA shifts its focus from assembly to scientific research, technology development, exploration, commerce, and education.

Aboard the orbiting laboratory, crew members pursue novel avenues of research and development that impact medical research, advance materials and processes to benefit industries on Earth, and can accelerate breakthroughs in technology and engineering that have proven themselves as practical applications for life on Earth.

The station continuous to expand the boundaries of space research. The unique capabilities of its laboratories will lead to discoveries that will benefit missions farther into outer space. Using the station to study human endurance in space and test new technologies and techniques, NASA will prepare for longer journeys to other destinations, such as Mars and beyond.

21st Century Astronauts

The astronauts of the century will continue to work aboard the International Space Station in cooperation with the international partners; help to build and fly a new NASA vehicle, the Orion Multi-Purpose Crew Vehicle (MPCV) designed for human deep space exploration; and further NASA’s efforts to partner with industry to provide a commercial capability for space transportation to the space station.

The Orion MPCV draws from more than 50 years of spaceflight experience and is designed to meet the evolving needs of our nation’s future human space exploration program. Orion features dozens of technology advancements and innovations that have been incorporated into the spacecraft’s subsystem and component design and includes both crew and service modules, a spacecraft adaptor, and a revolutionary launch abort system that will significantly increase crew safety. Its life support, propulsion, thermal protection, and avionics systems, in combination with other deep space elements, will enable extended duration deep space missions. These systems have been developed to make possible the integration of new technical innovations as they become available.
Orion will be capable of carrying astronauts on diverse expeditions beyond Earth’s orbit-ushering in a new era of human space exploration.
NASA is in the process of identifying possible near-Earth asteroids to explore with the goal of visiting an asteroid in 2025. With that goal, and keeping in mind that the plan is to send a robotic precursor mission to the asteroid approximately five years before humans arrive, NASA will need to select the first set of targets to explore within the next decade.

INDIAN ASTRONAUTS

During the mid-80’s Rakesh Sharma proved to be a pioneer in the field of piloting. He was the first Indian to venture in to the space and bring a new perspective to the country. Though it is long ago Rakesh undertook the Historical journey to space, it is still remembered among the people. Owing to his dedication and struggle, he became a part of most distinctive space program that involved only best military cadets. The Inter cosmos Research Team was a program conducted by Soviet Union and included active participation from allied countries such as India, Syria and France. Rakesh Sharma was now chosen for this assignment and ever since he has been an inspiration to upcoming cosmonauts.

Kalpana Chawla an Indian-American astronaut and the first Indian woman in space was the one of the seven astronauts who lost their life in the space shuttle Columbia disaster on Feb1, 2003. A role model for many young for her incredible journey from Karnal, where she was born, to NASA where she become an astronaut to fulfil her dream of reaching the stars.  

 





Collected By:
                          Sindhhu D G
                          Tashhreefa
                          Vidya Saraswathi A
                          Vinutha

Source: Internet

Tuesday, 6 March 2018

EYE TO THE SKY


Physics Behind the Wonders.....!

Sometimes we get caught up in the day-to-day grind that we forget how amazing and at times mysterious and terrifying the world around us really is .It is easy to take nature for granted,   its many unfathomable wonders. In this article, a selection of the most compelling and occasionally haunting optical illusions and atmospheric phenomena that the natural world has to offer are explored. When light from the Sun and the Moon enters our atmosphere, it is sometimes reflected, refracted and dispersed by tiny ice crystals, water droplets and dust to produce a whole host of fantastic atmospheric visions. Some are even more common than we realise.

Rainbow



A rainbow is a meteorological phenomenon that is caused by reflection, refraction and dispersion of light in water droplets resulting in a spectrum of light appearing in the sky. It takes the form of a multicoloured circular arc. Rainbows caused by sunlight always appear in the section of sky directly opposite the sun.

Rainbows can be full circles. However, the observer normally sees only an arc formed by illuminated droplets above the ground, and centered on a line from the sun to the observer's eye.

In a primary rainbow, the arc shows red on the outer part and violet on the inner side. This rainbow is caused by light being refracted when entering a droplet of water, then reflected inside on the back of the droplet and refracted again when leaving it.

In a double rainbow, a second arc is seen outside the primary arc, and has the order of its colours reversed, with red on the inner side of the arc. This is caused by the light being reflected twice on the inside of the droplet before leaving it.

Aurora


An aurora , sometimes referred to as polar lights, northern lights (aurora borealis) or southern lights (aurora australis), is a natural light display in the Earth's sky, predominantly seen in the high-latitude regions (around the Arctic and Antarctic).

Auroras are produced when the magnetosphere is sufficiently disturbed by the solar wind that the trajectories of charged particles in both solar wind and magnetospheric plasma, mainly in the form of electrons and protons, precipitate them into the upper atmosphere (thermosphere/exosphere) due to Earth's magnetic field, where their energy is lost.

The resulting ionization and excitation of atmospheric constituents emits light of varying colour and complexity. The form of the aurora, occurring within bands around both polar regions, is also dependent on the amount of acceleration imparted to the precipitating particles. Precipitating protons generally produce optical emissions as incident hydrogen atoms after gaining electrons from the atmosphere. Proton auroras are usually observed at lower latitudes.

Aurora came from the Latin word for "dawn, morning light", since auroras were formerly thought to be the first light of dawn.

Halo


Halo is the name for a family of optical phenomena produced by light interacting with ice crystals suspended in the atmosphere. Halos can have many forms, ranging from coloured or white rings to arcs and spots in the sky. Many of these are near the Sun or Moon, but others occur elsewhere or even in the opposite part of the sky. Among the best known halo types are the circular halo (properly called the 22° halo), light pillars and sun dogs, but there are many more; some of them fairly common, others (extremely) rare.

The ice crystals responsible for halos are typically suspended in cirrus or cirrostratus clouds high (5–10 km, or 3–6 miles) in the upper troposphere, but in cold weather they can also float near the ground, in which case they are referred to as diamond dust. The particular shape and orientation of the crystals are responsible for the type of halo observed. Light is reflected and refracted by the ice crystals and may split up into colours because of dispersion. The crystals behave like prisms and mirrors, refracting and reflecting light between their faces, sending shafts of light in particular directions.

Sun dog


A sun dog or mock sun, formally called a parhelion is an atmospheric optical phenomenon that consists of a bright spot to the left and/or right of the Sun Two sun dogs often flank the Sun within a 22° halo.

The sun dog is a member of the family of halos, caused by the refraction of sunlight by ice crystals in the atmosphere. Sun dogs typically appear as a pair of subtly colored patches of light, around 22° to the left and right of the Sun, and at the same altitude above the horizon as the Sun. They can be seen anywhere in the world during any season, but are not always obvious or bright. Sun dogs are best seen and most conspicuous when the Sun is near the horizon.

Sun dogs are commonly caused by the refraction and scattering of light from plate-shaped hexagonal ice crystals either suspended in high and cold cirrus or cirrostratus clouds, or drifting in freezing moist air at low levels as diamond dust. The crystals act as prisms, bending the light rays passing through them with a minimum deflection of 22°. As the crystals gently float downwards with their large hexagonal faces almost horizontal, sunlight is refracted horizontally, and sun dogs are seen to the left and right of the Sun. Larger plates wobble more, and thus produce taller sundogs.
Sun dogs are red-coloured at the side nearest the Sun; farther out the colors grade through oranges to blue.


Corona


A corona is an optical phenomenon produced by the diffraction of light from the Sun or the Moon by individual small water droplets and sometimes tiny ice crystals of a cloud or on a foggy glass surface. In its full form, a corona consists of several concentric, pastel-coloured rings around the celestial object and a central bright area called aureole. The aureole is often (especially in case of the Moon) the only visible part of the corona and has the appearance of a bluish-white disk which fades to reddish-brown towards the edge. The angular size of a corona depends on the diameters of the water droplets involved: Smaller droplets produce larger coronae. For the same reason, the corona is the most pronounced when the size of the droplets is most uniform. Coronae differ from halos in that the latter are formed by refraction (rather than diffraction) from comparatively large rather than small ice crystals.

Pollen corona: - Each year trees of the Northern forests release copious clouds of pollen. The pollen grains from a given tree variety usually have very similar sizes - ideal for corona formation. 

Unlike water droplets, pollens are non spherical. Many have air sacs to assist wind dispersal and they are consequently become specially oriented as they drift in the air. The result is elongated coronae, sometimes with bright patches on their rings.

Pollens are comparatively large and so their coronae are small. Look close to a well shielded sun  or, preferably, search for them in the reflection of the sky in a pool or dark glass.


Mirage


A mirage is a naturally occurring optical phenomenon in which light rays bend to produce a displaced image of distant objects or the sky. The word comes to English via the French mirage, from the Latin   mirari, meaning "to look at, to wonder at". This is the same root as for "mirror" and "to admire".  In contrast to a hallucination, a mirage is a real optical phenomenon that can be captured on camera, since light rays are actually refracted to form the false image at the observer's location. What the image appears to represent, however, is determined by the interpretive faculties of the human mind. For example, inferior images on land are very easily mistaken for the reflections from a small body of water.

For exhausted travelers in the desert, an inferior mirage may appear to be a lake of water in the distance. An inferior mirage is called "inferior" because the mirage is located under the real object. The real object in an inferior mirage is the (blue) sky or any distant (therefore bluish) object in that same direction. The mirage causes the observer to see a bright and bluish patch on the ground in the distance.

Light rays coming from a particular distant object all travel through nearly the same air layers and all are bent over about the same amount. Therefore, rays coming from the top of the object will arrive lower than those from the bottom. The image usually is upside down, enhancing the illusion that the sky image seen in the distance is really a water or oil puddle acting as a mirror.


Diamond ring effect 


The Baily's beads effect, or diamond ring effect, is a feature of total and annular solar eclipses. As the Moon covers the Sun during a solar eclipse, the rugged topography of the lunar limb allows beads of sunlight to shine through in some places while not in others. The effect is named after Francis Baily, who explained the phenomenon in 1836. The diamond ring effect is seen when only one bead is left, appearing as a shining "diamond" set in a bright ring around the lunar silhouette.

Lunar topography has considerable relief because of the presence of mountains, craters, valleys, and other topographical features. The irregularities of the lunar limb profile (the "edge" of the Moon, as seen from a distance) are known accurately from observations of grazing occultations of stars. Astronomers thus have a fairly good idea which mountains and valleys will cause the beads to appear in advance of the eclipse. While Baily's beads are seen briefly for a few seconds at the center of the eclipse path, their duration is maximized near the edges of the path of the umbra, lasting 1–2 minutes.

Red moon


The moon does not have any light  its own ,it shines because its surface reflects sunlight. During a total lunar eclipse, the earth moves between the sun and the moon and cuts off the moon’s light supply. When this happens ,the surface of the moon takes the reddish glow instead of going completely dark.
        
The red colour of a totally eclipsed moon has prompted many people in recent years to refer to total lunar eclipses as Blood Moon.
        
The reason why the Moon takes on a reddish colour during totality is a phenomenon called Rayleigh scattering.  It is the same mechanism responsible for causing colourful sunrises and sunsets and the sky to look blue.
            
When sunlight entering the Earth's atmosphere strikes the particles that are smaller than the light's wavelength, it gets scattered into different directions. Not all colours in the light spectrum, however, are equally scattered. Colours with shorter wavelengths, especially the violet and blue colours, are scattered more strongly, so they are removed from the sunlight before it hits the surface of the Moon during a lunar eclipse. Those with longer wavelengths, like red and orange, pass through the atmosphere. This red-orange light is then bent or refracted around Earth, hitting the surface of the Moon and giving it the reddish-orange glow that total lunar eclipses are famous for.


Collected By:

                          Reshna K
                          Sahana H
                          Shilpa M P
                          Sinchana K P

Source: Internet

Thursday, 11 January 2018

ISRO: EXPLORING THE SPACE BEYOND!

Indian Space Research Organization
It is the space station of the government of India, head quartered in the city of Bangalore, Karnataka, India.
It’s vision is to ‘harness space technology for national development while pursuing space science research and planetary.

Moto: Space technology in the service of human kind

ISRO was established in the year 1961 to focus the talent of Indian Researchers into advancing the space program. Dr Vikram Sarabhai was the founding father of Indian space program. After the launch of Sputnik in 1957 by Russia, he recognized the potential that satellites provided.

He was born on 12 August 1919. He was an Indian scientist and innovator widely regarded as the father of India’s space program. Dr. Sarabhai was considered as a great institution builder and established or helped to establish a large number of institutions in diverse fields. He was instrumental in establishing the Physical Research Laboratory (PRL).

The establishment of the Indian Space Research Organization (ISRO) was one of his greatest achievement. He successfully convinced the government about the importance of a space program for a developing country like India.

Dr. Homi Jehangir Bhabha, widely regarded as the father of India's nuclear science program, supported Dr. Sarabhai in setting up the first rocket launching station in India. This center was established at Thumba near Thiruvananthapuram on the coast of the Arabian Sea, primarily because of its proximity to the equator. After a remarkable effort in setting up the infrastructure, personnel, communication links, and launch pads, the inaugural flight was launched on November 21, 1963 with a sodium vapour payload.

As a result of Dr. Sarabhai's dialogue with NASA in 1966, the Satellite Instructional Television Experiment (SITE) was launched during July 1975 - July 1976 (when Dr. Sarabhai was no more). Dr. Sarabhai started a project for the fabrication and launch of an Indian Satellite. As a result, the first Indian satellite, Aryabhata, was put in orbit in 1975 from a Russian Cosmodrome. Dr. Sarabhai was very interested in science education and founded a Community Science Centre at Ahmedabad in 1966. Today, the Centre is called the Vikram A Sarabhai Community Science Centre.

Centers:

Satish Dhawan Space Centre (SDSC)SHAR, Sriharikota, the Spaceport of India, is responsible for providing Launch Base Infrastructure for the Indian Space Programme. This Centre has the facilities for solid propellant processing, static testing of solid motors, launch vehicle integration and launch operations, range operations comprising telemetry, tracking and command network and mission control centre.

The Centre has two launch pads from where the rocket launching operations of PSLV and GSLV are carried out. The mandate for the centre is (i) to produce solid propellant boosters for the launch vehicle programmes of ISRO (ii) to provide the infrastructure for qualifying various subsystems and solid rocket motors and carrying out the necessary tests (iii) to provide launch base infrastructure for satellites and launch vehicles.

SDSC SHAR has a separate launch pad for launching sounding rockets. The centre also provides the necessary launch base infrastructure for sounding rockets of ISRO and for assembly, integration and launch of sounding rockets and payloads.

Vikram Sarabhai Space Centre (VSSC): It is a major space research centre of the ISRO focusing on rocket and space vehicles for India’s satellite programme. It is located in Thiruvananthapuram, in the Indian state of Kerala. The centre had its beginnings as the thumb an equatorial rocket launching station (TERLS) in 1962. It is one of the main research and development establishments within ISRO.

Liquid Propulsion System Centre (LPSC): It is the centre of excellence in the area of liquid propulsion for ISRO’s launch vehicle and spacecraft programmes. Its headquarters and design office is at Thiruvananthapuram.

ISRO satellite centre (ISAC): ISAC at Bangalore is engaged in developing satellite technology and implementation of satellite systems for scientific, technological and application missions.

ISRO propulsion complex (IPRC): IPRC, Mahendragiri is equipped with state of-the-art-facilities necessary for realizing the cutting edge technology products for ISRO’s space research programme.

National Remote Sensing Centre (NRSC): The centre is responsible for remote sensing satellite data acquisition and processing data dissemination, aerial remote sensing and decision support for disaster management.

Master Control Facility (MCF): MCF at Hassan in Karnataka; Bhopal and in Madhya Pradesh monitors and controls all the geo-stationary satellites of ISRO.

ISRO telemetry tracking and command network (ISTRAC): ISTRAC is responsible for providing space operation services that include space craft control, TTC support services and other related projects and services, for the launch vehicle; low earth orbiting space craft and deep space missions of ISRO and other space agencies around the world.

Achievements:

Aryabhata: The Aryabhata spacecraft, named after the famous Indian astronomer, was India's first satellite; it was completely designed and fabricated in India and launched by a Soviet Kosmos-3M rocket from Kapustin Yar on April 19, 1975.

Reusable Launch Vehicle (RLV)India successfully tested the launched of indigenously made Reusable Launch Vehicle (RLV), capable of launching satellites into orbit around earth and then re-enter the atmosphere, from Sriharikota in Andhra Pradesh. RLV is dubbed as India’s own space shuttle. (The ‘Space Shuttle’ was a partially reusable low Earth orbital spacecraft system operated by the U.S. National Aeronautics and Space Administration (NASA), as part of the Space Shuttle program.)

RLV is the unanimous solution to achieve low cost, reliable and on—demand space access. The making of the Indian space shuttle or RLV-TD has taken five years and the government has invested Rs. 95 crore in the project. This flight will test the capability of the vehicle to survive a re-entry at speeds higher than that of sound. The solution to reducing cost of launching satellites into orbit is to recycle the rocket or make it reusable.

(Nasa grounded its space shuttle programme in 2011 after using its reusable vehicles like Discovery, Endeavor, Columbia and Challenger for over three decades to launch various missions, including the International Space Station (ISS) and the Hubble telescope.)

Indian national satellite system (INSAT): Launched by ISRO in 1983, INSAT is a series of multi-purpose geostationary satellite. It is used for telecommunication, broadcasting, meteorology, search and reuse operations. Commissioned in 1983, INSAT is the largest domestic communication system in the Asia Pacific Region. It is a joint venture of the Department of Space, Department of Telecommunications, India Meteorological Department, All India Radio and Doordarshan.

Space capsule recovery experiment (SRE-1): On 10 January 2007, an Indian experiment spacecraft was launched using the PSLVC3 rocket from Sriharikota. Before reentering the atmosphere of the earth and diving into the Bay of Bengal, the capsule stayed in the orbit for twelve days.

SRE-1 was designed to demonstrate the capability to recover an orbiting space capsule, and the technology of an orbiting platform for performing experiments in microgravity conditions. It was also intended to test reusable Thermal Protection System, navigation, guidance and control, hypersonic aero-thermodynamics, management of communication blackout, deceleration and flotation system and recovery operations. The information obtained from this technology and experiment is being applied to the design of India's Gaganyaan crewed orbital capsule.

Chandrayaan-1: Is the India's first mission to Moon, was launched successfully on October 22, 2008 from SDSC SHAR, Sriharikota. The spacecraft was orbiting around the Moon at a height of 100 km from the lunar surface for chemical, mineralogical and photo-geologic mapping of the Moon. The spacecraft carried 11 scientific instruments built in India, USA, UK, Germany, Sweden and Bulgaria.

After the successful completion of all the major mission objectives, the orbit has been raised to 200 km during May 2009. The satellite made more than 3400 orbits around the moon and the mission was concluded when the communication with the spacecraft was lost on August 29, 2009.

Mangalayaan (MOM): The Mars Orbiter Mission (MOM), also called Mangalyaan is a space probe orbiting Mars since 24 September 2014. It was launched on 5 November 2013 by the Indian Space Research Organisation (ISRO). It is India's first interplanetary mission and it made it the fourth space agency to reach Mars, after Roscosmos, NASA, and the European Space Agency. It is the first Asian nation to reach Mars orbit, and the first nation in the world to do so in its first attempt

PSLV-C37: Was the 39th mission of the Indian Polar Satellite Launch Vehicle (PSLV) program and its 16th mission in the XLconfiguration. PSLV-C37 successfully carried and deployed (in one go) a record 104 satellites in sun-synchronous orbits. Launched on 15 February 2017 by the Indian Space Research Organisation (ISRO) from the Satish Dhawan Space Centre at Sriharikota, Andhra Pradesh, it broke the earlier record of launching 37 satellites by a Russian Dnepr rocket on 19 June 2014. According to ISRO, the 101 international satellites were launched as part of a commercial arrangement between several firms and its commercial arm Antrix Corporation Limited, run under the auspices of the Indian Government's Department of Space. PSLV-C37 is also known as cartosat-2 series satellite. The cartosat-2 serves as, India’s earth observation satellite.

Future Projects: 

Chandrayana-II: Is India's second lunar exploration mission after Chandrayaan-1 (will be launched in the January-March window in 2019 ) Developed by the Indian Space Research Organisation (ISRO), the mission is planned to be launched to the Moon by a Geosynchronous Satellite Launch Vehicle Mark III (GSLV Mk III). It includes a lunar orbiter, lander and rover, all developed by India.

NISAR: The NASA-ISRO Synthetic Aperture Radar (NISAR) mission is a joint project between NASA and ISRO to co-develop and launch a dual frequency synthetic aperture radar satellite. The satellite will be the first radar imaging satellite to use dual frequency and it is planned to be used for remote sensing to observe and understand natural processes on Earth

Collected By:

Havyashree G P
Ivy Anjali Dsouza
Lekshmi Priya L
Pallavi V M

Source: Internet

Tuesday, 9 January 2018

DWARF PLANETS IN OUR SOLAR SYSTEMS

There are 5 officially recognized dwarf planets in our solar system; they are Ceres, Pluto, Haumea, Makemake and Eris. With exception of Ceres, which is located in the asteroid belt, the other dwarf planets are found in the outer solar system. There are another 6 objects in our solar system that are almost certainly dwarf planets and there are as many as 10000. Of the dwarf planets only 2 have been visited by space probes, in 2015 NASA’s Dawn and New Horizons missions reached Ceres and Pluto respectively.

WHAT IS DWARF PLANET?

A dwarf planet is a planetary-mass object that is neither a planet nor a natural satellite. The International Astronomical Union’s definition of a dwarf planet is:
A “dwarf planet” is a celestial body that
  • is in orbit around the Sun,
  • has sufficient mass for its self-gravity to overcome rigid body forces, so that it assumes a hydro static equilibrium (nearly round) shape,
  • has not cleared, the neighborhood around its orbit, and
  • is not a satellite.The key difference is that a planet has cleared other objects in the area of its orbit, while a dwarf planet has not.
The largest dwarf planet in the solar system is Pluto followed by Eris, Makemake, Haumea with the smallest being Ceres. The order of dwarf planet from closest to Sun outwards is Ceres, Pluto, Haumea, Makemake and with the Eris being the farthest from the Sun.

HISTORY
Starting in 1801, astronomers discovered Ceres and the other bodies between the Mars and Jupiter which were for decades considered as a planet. Between then and around 1851, when the numbers of planet had reached 23, astronomers started using the word asteroid for the small bodies. With the discovery of Pluto in 1930, most astronomers considered Solar System to have 9 planets. For almost 50 years Pluto was thought to be larger than Mercury, but with the discovery of Pluto’s moon Charon, it was determined that mass of Pluto was much smaller than initial estimate. It was roughly one-twentieth the mass of Mercury. Furthermore, having some unusual characteristics, such as larger orbital eccentricity and a high orbital inclination, it became evident that Pluto was a different kind of body from any of the other planets.

Eris (then known as 2003UB313) was discovered in January 2005; it was thought to be slightly greater than Pluto, and some reports informally referred to it as the 10th planet. The issue became matter of intense debate during a IAU general assembly in August 2006. The IAU’s initial draft proposal included Pluto, Charon, Eris and Ceres in the list of planets. After all astronomer objected to this proposal, an alternative drawn up by Uruguayan astronomer Julio Angel Fernandez: He proposed an intermediate category for objects large enough to be round, but had not cleared their objects of planetesimals. Dropping Charon from the list, the new proposal also removed Pluto, Ceres and Eris, because they have not cleared their orbits. Thus the IAU resolves that planets and the other bodies except satellites, in our solar system be defined into 3 distinct categories. By this problem regarding to dwarf planet was solved.

EXPLORATION
On March 6, 2015, the ‘Dawn’ Spacecraft began to orbit Ceres, becoming the first Spacecraft to orbit of a dwarf planet. On July 14, 2015 the ‘New Horizons’ space probe flew by Pluto and its 5 moons. Dawn has also explored the former dwarf planet Vesta. This exploration helps in the study of the evolution of dwarf planet.

PLUTO
Pluto was discovered in 1830 by an astronomer from the United States. An astronomer Clyde W. Tombaugh discovered Pluto on February 18th 1930. Pluto was known as the smallest planet in the solar system and the ninth planet from the Sun.

But today Pluto is known as ‘dwarf planet’. A dwarf planet orbits the Sun just like other planets, but it is smaller. A dwarf planet is so small it cannot clear other objects out of its path.

Pluto is in the region called Kuiper (KY-per) Belt. Thousands of small, icy objects like Pluto are in the Kuiper belt. Pluto is only 1400 miles wide. That about half the width of the united states Pluto is slightly smaller than Earth’s moon. It takes Pluto 248 years to go around the Sun. One day on Pluto is about 6.5 days on the earth.

Pluto is called as Plutoid. A Plutoid is a dwarf planet that is farther out in space than the planet Neptune. The three known Plutoids are Pluto, Eris and Makemake. Astronomers used telescope to discover new objects like Plutoids scientists are learning more about the universe and the Earth’s place in it.

Pluto is very cold. The Pluto is far from Earth that scientist known very little temperature. Pluto is probably covered with ice. Pluto has about one-fifteenth the gravity of earth. A person who weighs 400 pounds in earth would weigh only 7 pounds on Pluto.

NASA learns about Pluto from pictures taken with telescopes. Pictures from Hubble space telescope helped scientists to find the four light areas on Pluto. Pluto is so far away that even pictures taken by telescope area little fazzy.

In 2006, NASA launched the first mission to Pluto’ New Horizon’. New Horizon is the space craft that is going to the edge of the solar system. This space craft is about the size of piano. It was 9 years trip. In 2015, New Horizon arrived at Pluto. New Horizon has cameras that will take pictures of Pluto. These pictures and information will help scientists to learn more about dwarf planet.

Pluto having one-third of water. This is in the form of water ice which is more than 3 times as much water as in all the earth’s ocean, the remaining two-third are rock.

Pluto’s location was predicted by Percival Lowell in 1915. When Pluto’s elliptical orbit takes it closer to the Sun, its surface ice melts and forms a thin atmosphere primarily of nitrogen which slowly escapes the planet. It also has methane. The methane is dissociated by sunlight when a Pluto travels away from the Sun. When Pluto travels away from the atmosphere then freezes back to its solid state.

Diameter - 2372 km
Mass - 1.31*1022 kg (0.17 moons)
Orbit Distance - 39.2 AU
Orbit Period - 248 years
Surface Temperature - 229 degree C


CERES
Ceres is the closest dwarf planet to the sun and is located in asteroid belt, between Mars and Jupiter, making it the only dwarf planet in the inner solar system. Ceres is the smallest of the bodies current classified as dwarf planets with a diameter of 950km. Ceres was the first asteroid to be discovered by Giuseppe Pazzi at Palermo on 1st January 1801. It was originally considered as planet, but was reclassified as an asteroid in the1850’s after many other objects in the similar orbits was discovered.

Dawn is a space probe launched by NASA in September 2007 with the mission of studying dwarf planet Ceres with the other protoplanets of the asteroid belt and Vesta.

Ceres is the largest known asteroid in the asteroid belt until 2006. In 2006, the IAU formed a new class of solar system objects known as dwarf planets. By the definition a dwarf planet is spherical and travels in an orbit around the Sun. Ceres fit the definition perfectly. Hence it is considered as a dwarf planet.

The surface is probably a mixture of water-ice and various hydrated minerals such as carbonates and clay. Ceres appears to be differentiated in to a rocky core and an icy mantle, and may have a remnant internal ocean of liquid water under the layer of ice. Ceres has a tenuous water vapor atmosphere out-gassing from water-ice on the surface.

Ceres was the first object considered to be an asteroid. The first visit to Ceres is due in 2015. NASA’s Dawn spacecraft has been making its way to Ceres from the asteroid Vesta since September 2012. There is a high interest in this mission and is one possible destination for human colonization gives its abundance of ice, water and minerals.

Ceres has a mysterious white spot. This can be seen in both the old Hubble images and the more recent photos taken by Dawn spacecraft on its approach.

Every second Ceres loses 6 kg of its mass in steam. Plums of water vapor shooting up from Ceres surface were observed by the Herschel Space Telescope. This was the first definitive observation of water vapor in the asteroid belt.

Ceres accounts for one-third of the mass in the asteroid belt. For roughly the first 50 years after this discovery Ceres was frequently referred as a Planet. Ceres is the only dwarf planet with no moons. The other planets Pluto, Haumea, Makemake and Eris all have at least one moon.


HAUMEA
Haumea is the third closest dwarf planet from the Sun and is unique in its elongated shape making it the least spherical of the dwarf planets. It is spinning so quickly that it has been stretched in to the shape of an ellipsoid.

It was discovered in 28th December 2004 by a team headed by Mike Brown of Caltech and independently in 2005 by a team headed by Jose Luis Ortiz Moreno. On September 17, 2008 it was recognized as a dwarf planet by International Astronomical Union (IAU) and named after Haumea, the Hawaiian goddess of childbirth.

Haumea is a plutoid, a dwarf planet beyond Neptune’s orbit. It is classified as a dwarf planet because it is presumed to be massive enough to have been rounded by its own gravity into a shape in hydrostatic equilibrium, but not massive enough to have cleared its neighborhood of similarly sized objects.

A day in Haumea lasts 3.9 hours. Its rotational speed as well as its collision origin also makes Haumea one of the densest dwarf planets discovered to date. Haumea has a red spot, which stands for surrounding crystalline ice. Haumea is roughly one third of mass of Pluto.

Equatorial diameter - 1960 km to 1518 km
Polar diameter - 996 km
Mass - 4.01*1021 kg (0.05 moons)
Orbit distance - 6452000000 (43.13 AU)
Orbit period - 283.3years
Surface temperature - -241 degree C
Moons - 2 ( Hi’iaka and Namaka )


ERIS
Eris is the most distant dwarf planet from the Sun and has the greatest mass. Eris is the second largest dwarf planet and at one point was considered for the position of the 10th planet. Eris discovery promoted discussion that eventually leads to the classification of “Dwarf planets”.

Eris was discovered in 5th January 2005 by M. E. Brown, C.A. Trujillo and D.J. Babinowitz from images taken on October 21, 2003. The discovery was announced on July 29, 2005 the same day Makemake and two day after Haumea is declared.

Eris is unquestionably the most massive of the known dwarf planets (the largest object that is not a planet that orbits the Sun) and was once thought to be the largest due to its relative brightness. After a stellar occultation in 2010 its diameter was calculated to be smaller than previously thought and more recent measurement suggested Pluto was larger than thought making it the largest. All the objects in the Asteroid Belt could fit inside Eris. Eris is still smaller than Earth’s moon, having about two third of the moon’s diameter and one third of its volume. Eris is not always the most distant dwarf planet. At its closest point it is closer than Pluto’s most distant point.

Diameter - 2,326 km
Mass - 1.66*102 2 kg (0.23 moons)
Orbit distance - 68.01 AU
Orbit period - 560.9 years
Surface temperature - -231 degree C
Moons - 1 (Dysnomia)


MAKEMAKE
Makemake is the second farthest dwarf planet from the Sun and is the third largest dwarf planet in the solar system. Makemake was discovered on March 31st 2005 and was recognized as a dwarf planet by the International Astronomical Union (IAU) in July 2008. Until April 2016 Makemake was thought to be the only one of the four outer dwarf planets to not have any moons.

Makemake is the second brightest Kuiper Belt object after Pluto. Makemake and its moon MK2, which was spotted about 20000 km from Makemake is viewed by Hubble Space Telescope. Makemake was expected to have an atmosphere similar to that of Pluto, but in 2011 it was revealed that it mostly lacks a gas envelop. Makemake is a Kuiper Belt object; hence it remains stable over the age of the solar system since, it is not affected by the Neptune’s gravity.


Equatorial diameter - 1434 km
Polar diameter - 1422 km
Mass - 2.5*1021 kg
Orbit distance - 6850000000 km
Orbit period - 309.9 years
Surface temperature - -239 degree C
Moons - 1( MK2-5/2015(136472)1)


Collected By:

Tashreefa
Vidhya Saraswathi
Vijitha
Vinutha

Source: Internet