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Operator | NASA / JPL |
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Mission type | Flyby |
Flyby of | Jupiter, Saturn |
Launch date | 1977-09-05 12:56:00 UTC (34 years, 11 months and 21 days ago) |
Launch vehicle | Titan IIIE-Centaur |
Launch site | Space Launch Complex 41 Cape Canaveral Air Force Station, Florida, United States |
Mission duration | In progress (Interstellar mission) (33 years, 7 months and 22 days elapsed)
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COSPAR ID | 1977-084A |
Homepage | NASA Voyager website |
Mass | 721.9 kg (1,592 lb) |
Power | 420 W (3 RTGs) |
Monday, August 27, 2012
NASA's Voyager 1
The Death Of Neil Armstrong
The Death Of Neil Armstrong
Three days ago we lost one of the most inspirational people i ever known and perhaps you guys may known him too... He is Neil Armstrong
Armstrong, the first man to walk on the moon and commander of NASA's Apollo 11 lunar landing mission, died at age 82
due to complications from recent heart surgery, his family said.
Armstrong had heart bypass surgery earlier this month to clear blocked
arteries.
Many astronauts with NASA and other space agencies cited Armstrong as a
major inspiration in their lives, Others reflected on the legendary
astronaut's modesty, despite his global fame.
Several active and former NASA astronauts wrote that Armstrong inspired them to pursue dreams of flying in space.
"I know I am joined by millions of others in mourning Neil's passing — a
true American hero and the best pilot I ever knew," wrote Apollo 11
astronaut Buzz Aldrin, who walked with Armstrong on the moon on July 20,
1969, in his Twitter post. He writes as @TheRealBuzz.
Neil Armstrong 1 small step will inspire generations to come.
Good Bye Neil Armstrong...
*Source: Wikipedia & Fox News*
Friday, August 17, 2012
NASA's Mars Pathfinder
Mars Pathfinder
Mars Pathfinder (MESUR Pathfinder) was an American spacecraft that landed a base station with a roving probe on Mars in 1997. It consisted of a lander, renamed the Carl Sagan Memorial Station, and a lightweight (10.6 kg/23 lb) wheeled robotic Mars rover named Sojourner.Launched on December 4, 1996 by NASA aboard a Delta II booster a month after the Mars Global Surveyor was launched, it landed on July 4, 1997 on Mars's Ares Vallis, in a region called Chryse Planitia in the Oxia Palus quadrangle. The lander then opened, exposing the rover which conducted many experiments on the Martian surface. The mission carried a series of scientific instruments to analyze the Martian atmosphere, climate, geology and the composition of its rocks and soil. It was the second project from NASA's Discovery Program, which promotes the use of low-cost spacecraft and frequent launches under the motto "cheaper, faster and better" promoted by the then administrator, Daniel Goldin. The mission was directed by the Jet Propulsion Laboratory (JPL), a division of the California Institute of Technology, responsible for NASA's Mars Exploration Program. The project manager was JPL's Tony Spear.This mission was the first of a series of missions to Mars that included rovers, and was the first successful lander since the two Vikings landed on the red planet in 1976. Although the Soviet Union successfully sent rovers to the Moon as part of the Lunokhod program in the 1970s, its attempts to use rovers in its Mars probe program failed.In addition to scientific objectives, the Mars Pathfinder mission was also a "proof-of-concept" for various technologies, such as airbag-mediated touchdown and automated obstacle avoidance, both later exploited by the Mars Exploration Rover mission. The Mars Pathfinder was also remarkable for its extremely low cost relative to other unmanned space missions to Mars. Originally, the mission was conceived as the first of the Mars Environmental Survey (MESUR) program.Mission objectives
Sojourner rover on Mars on sol 22 - To prove that the development of "faster, better and cheaper" spacecraft was possible (with three years for development and a cost under $150 million).
- To show that it was possible to send a load of scientific instruments to another planet with a simple system and at one fifteenth the cost of a Viking mission. (For comparison, the Viking missions cost $935 million in 1974 or $3.5 billion in 1997 dollars)
- To demonstrate NASA's commitment to low-cost planetary exploration by finishing the mission with a total expenditure of $280 million, including the launch vehicle and mission operations.
Science experiments
- The Mars Pathfinder conducted different investigations on the Martian soil using three scientific instruments. The lander contained a stereoscopic camera with spatial filters on an expandable pole called Imager for Mars Pathfinder (IMP), and the Atmospheric Structure Instrument/Meteorology Package (ASI/MET) which acts as a Mars meteorological station, collecting data about pressure, temperature, and winds. The MET structure included three windsocks mounted at three heights on a pole, the topmost at about one meter (yard) and generally registered winds from the West.
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The Sojourner rover had an Alpha Proton X-ray Spectrometer (APXS),
which was used to analyze the components of the rocks and soil. The
rover also had two black-and-white cameras and a color one. These
instruments could investigate the geology of the Martian surface from
just a few millimeters to many hundreds of meters, the geochemistry and evolutionary history of the rocks and surface, the magnetic and mechanical properties of the land, as well as the magnetic properties of the dust, atmosphere and the rotational and orbital dynamics of the planet.Three cameras were onboard of the rover: Two black and white 0.3-megapixel cameras were located on the front (768 horizontal pixels × 484 vertical pixels configured in 4×4 pixel blocks), coupled with five laser stripe projectors, which enabled stereoscopic images to be taken along with measurements for hazard detection on the rover's path. A third camera with the same resolution but taking colour images was located on the back, near the APXS, and rotated by 90°. It provided images of the APXS's target area and the rover's tracks on the ground. The pixels of this colour camera were arranged in such a way, that out of the 16 pixel of a 4×4 pixel block, 12 pixel were sensitive to green, 2 pixel to red and 2 pixel were sensitive to infrared as well as blue. As all cameras had lenses made out of zinc-selenide, which blocks light below a wavelength of 500 nm, no blue light actually reached these "blue/infrared" pixels, which therefore recorded only infrared.All three cameras were CCDs manufactured by Eastman Kodak Company, and were controlled by the rover's CPU. They all had auto-exposure and capabilities for handling bad pixels, and the image parameters (exposure time, compression used, etc.) were included in the transmitted images as part of the image header. The rover could compress the front cameras' images using the block truncation coding (BTC) algorithm, but it could only do the same for the back camera's images only if the colour information was discarded. The cameras' optical resolution was sufficient to resolve 0.6 cm details across a 0.65 m range.
Labels:
Mars,
Mars Pathfinder,
Nasa,
Sojourner,
Space
Wednesday, August 15, 2012
NASA's Mars Exploration Rover (MER)
NASA's Mars Exploration Rover Mission (MER) is an ongoing robotic space mission involving two rovers, Spirit and Opportunity, exploring the planet Mars. It began in 2003 with the sending of the two rovers—MER-A Spirit and MER-B Opportunity—to explore the Martian surface and geology.
Objectives
The scientific objectives of the Mars Exploration Rover mission are to:
- Search for and characterize a variety of rocks and soils that hold clues to past water activity. In particular, samples sought include those that have minerals deposited by water-related processes such as precipitation, evaporation, sedimentary cementation, or hydrothermal activity.
- Determine the distribution and composition of minerals, rocks, and soils surrounding the landing sites.
- Determine what geologic processes have shaped the local terrain and influenced the chemistry. Such processes could include water or wind erosion, sedimentation, hydrothermal mechanisms, volcanism, and cratering.
- Perform calibration and validation of surface observations made by Mars Reconnaissance Orbiter instruments. This will help determine the accuracy and effectiveness of various instruments that survey Martian geology from orbit.
- Search for iron-containing minerals, and to identify and quantify relative amounts of specific mineral types that contain water or were formed in water, such as iron-bearing carbonates.
- Characterize the mineralogy and textures of rocks and soils to determine the processes that created them.
- Search for geological clues to the environmental conditions that existed when liquid water was present.
- Assess whether those environments were conducive to life.
During the next two decades, NASA will conduct several missions to address whether life ever existed on Mars. The search begins with determining whether the Martian environment was ever suitable for life. Life, as humans understand it, requires water, hence the history of water on Mars is critical to finding out if the Martian environment was ever conducive to life. Although the Mars Exploration Rovers do not have the ability to detect life directly, they offer important information on the habitability of the environment in the planet's history
History
The probes were launched June and July 2003 and landed January 2004 in widely separated equatorial places on Mars.
On January 21, 2004, the Deep Space Network lost contact with Spirit, for reasons originally thought to be related to a thunderstorm over Australia. The rover transmitted a message with no data, but later that day missed another communications session with the Mars Global Surveyor. The next day, JPL received a beep from the rover, indicating that it was in fault mode. On January 23, the flight team succeeded in making the rover send. The fault was believed to have been caused by an error in the rover's flash memory subsystem. The rover did not perform any scientific activities for ten days, while engineers updated its software and ran tests. The problem was corrected by reformatting Spirit's flash memory and using a software patch to avoid memory overload; Opportunity was also upgraded with the patch as a precaution. Spirit returned to full scientific operations by February 5.
On March 23, 2004, a news conference was held announcing "major discoveries" of evidence of past liquid water on the Martian surface. A delegation of scientists showed pictures and data revealing a stratified pattern and cross bedding in the rocks of the outcrop inside a crater in Meridiani Planum, landing site of MER-B, Opportunity. This suggested that water once flowed in the region. The irregular distribution of chlorine and bromine also suggests that the place was once the shoreline of a salty sea, now evaporated.
On April 8, 2004, NASA announced that it was extending the mission life of the rovers from three to eight months. It immediately provided additional funding of US $15 million through September, and $2.8 million per month for continuing operations. Later that month, Opportunity arrived at Endurance crater, taking about five days to drive the 200 meters. NASA announced on September 22 that it was extending the mission life of the rovers for another six months. Opportunity was to leave Endurance crater, visit its discarded heat shield, and proceed to Victoria crater. Spirit was to attempt to climb to the top of the Columbia Hills.
With the two rovers still functioning well, NASA later announced another 18 month extension of the mission to September 2006. Opportunitywas to visit the "Etched Terrain" and Spirit was to climb a rocky slope toward the top of Husband Hill. On August 21, 2005, Spirit reached the summit of Husband Hill after 581 sols and a journey of 4.81 kilometers (2.99 mi).
![](http://upload.wikimedia.org/wikipedia/commons/thumb/f/ff/Sol582A_P2299_L456-A590R1_br.jpg/220px-Sol582A_P2299_L456-A590R1_br.jpg)
Spirit's "postcard" view from the summit of Husband Hill: a windswept plateau strewn with rocks, small exposures of outcrop, and sand dunes. The view is to the north, looking down upon the "Tennessee Valley". This approximate true-color composite spans about 90 degrees and consists of eighteen frames captured by the rover's panoramic camera.
Spirit celebrated its one Martian year anniversary (669 sols or 687 Earth days) on November 20, 2005. Opportunity celebrated its anniversary on December 12, 2005. At the beginning of the mission, it was expected that the rovers would not survive much longer than 90 Martian days. The Columbia Hills were "just a dream", according to rover driver Chris Leger. Spirit explored the semicircular rock formation known as Home Plate. It is a layered rock outcrop that puzzles and excites scientists. It is thought that its rocks are explosive volcanic deposits, though other possibilities exist, including impact deposits or sediment borne by wind or water.
Spirit's front right wheel ceased working on March 13, 2006, while the rover was moving itself to McCool Hill. Its drivers attempted to drag the dead wheel behind Spirit, but this only worked until reaching an impassable sandy area on the lower slopes. Drivers directed Spirit to a smaller sloped feature, dubbed "Low Ridge Haven", where it spent the long Martian winter, waiting for spring and increased solar power levels suitable for driving. That September, Opportunity reached the rim of Victoria crater, and Spaceflight Now reported that NASA had extended mission for the two rovers through September 2007. On February 6, 2007, Opportunity became the first spacecraft to traverse ten kilometers (10,000 meters) on the surface of Mars.
Opportunity was poised to enter Victoria Crater from its perch on the rim of Duck Bay on June 28, 2007, but due to extensive dust storms, it was delayed until the dust had cleared and power returned to safe levels. Two months later, Spirit and Opportunity resumed driving after hunkering down during raging dust storms that limited solar power to a level that nearly caused the permanent failure of both rovers.
On October 1, 2007, both Spirit and Opportunity entered their fifth mission extension that extended operations into 2009, allowing the rovers to have spent five years exploring the Martian surface, pending their continued survival.
On August 26, 2008, Opportunity began its three-day climb out of Victoria crater amidst concerns that power spikes, similar to those seen on Spirit before the failure of its right-front wheel, might prevent it from ever being able to leave the crater if a wheel failed. Project scientist Bruce Banerdt also said, "We've done everything we entered Victoria Crater to do and more." Opportunity will return to the plains in order to characterize Meridiani Planum's vast diversity of rocks—some of which may have been blasted out of craters such as Victoria. The rover had been exploring Victoria Crater since September 11, 2007. As of January 2009, the two rovers had collectively sent back 250,000 images and traveled over 21 kilometers (13 mi).
After driving about 3.2 kilometers (2.0 mi) since it left Victoria crater, Opportunity first saw the rim of Endeavour crater on March 7, 2009. It passed the 10-mile mark (16 kilometers) along the way on sol 1897.Meanwhile, at Gusev crater, Spirit was dug in deep into the Martian sand, much as Opportunity was at Purgatory Dune in 2005.
On January 3 and January 24, 2010, Spirit and Opportunity marked six years on Mars, respectively. On January 26, NASA announced that Spirit will be used as a stationary research platform after several months of unsuccessful attempts to free the rover from soft sand.
NASA announced on March 24, 2010, that Opportunity, which has an estimated remaining drive distance of 12 km to Endeavour Crater, has traveled over 20 km since the start of its mission. Each rover was designed with a mission driving distance goal of just 600 meters.One week later, they announced that Spirit may have gone into hibernation for the Martian winter and might not wake up again for months.
On September 8, 2010, it was announced that Opportunity had reached the halfway point of the 19-kilometer journey between Victoria crater and Endeavour crater.
On May 24, 2011, NASA announced that it will cease attempts to contact Spirit, which has been stuck in a sand trap for two years. The last successful communication with the rover was on March 22, 2010. The final transmission to the rover was on May 25, 2011.
Design and construction
Spirit (and its twin, Opportunity) are six-wheeled, solar-powered robots standing 1.5 m (4.9 ft) high, 2.3 m (7.5 ft) wide and 1.6 m (5.2 ft) long and weighing 180 kg (400 lb). Six wheels on arocker-bogie system enable mobility over rough terrain. Each wheel has its own motor. The vehicle is steered at front and rear and is designed to operate safely at tilts of up to 30 degrees. Maximum speed is 50 mm/s (2 in/s);0.18 km/h, although average speed is about 10 mm/s (0.4 in/s). Both Spirit and Opportunity have pieces of the fallen World Trade Center's metal on them which were "turned into shields to protect cables on the drilling mechanisms".
Solar arrays generate about 140 watts for up to four hours per Martian day (sol) while rechargeable lithium ion batteries store energy for use at night. Spirit's onboard computer uses a 20 MHz RAD6000 CPU with 128 MB of DRAM, 3 MB of EEPROM, and 256 MB of flash memory. The rover's operating temperature ranges from −40 °C to +40 °C (−40 °F to 104 °F) andradioisotope heater units provide a base level of heating, assisted by electrical heaters when necessary. A gold film and a layer of silica aerogel provide insulation.
Communications depends on an omnidirectional low-gain antenna communicating at a low data rate and a steerable high-gain antenna, both in direct contact with Earth. A low gain antenna is also used to relay data to spacecraft orbiting Mars.
Fixed science instruments include
- Panoramic Camera (Pancam) – examines the texture, color, mineralogy, and structure of the local terrain.
- Navigation Camera (Navcam) – monochrome with a higher field of view but lower resolution, for navigation and driving.
- Miniature Thermal Emission Spectrometer (Mini-TES) – identifies promising rocks and soils for closer examination, and determines the processes that formed them.
The rover arm holds the following instruments
- Mössbauer spectrometer (MB) MIMOS II – used for close-up investigations of the mineralogy of iron-bearing rocks and soils.
- Alpha particle X-ray spectrometer (APXS) – close-up analysis of the abundances of elements that make up rocks and soils.
- Magnets – for collecting magnetic dust particles.
- Microscopic Imager (MI) – obtains close-up, high-resolution images of rocks and soils.
- Rock Abrasion Tool (RAT) – exposes fresh material for examination by instruments on board.
The cameras produce 1024-pixel by 1024-pixel images, the data is compressed, stored, and transmitted later.
- MER - A Spirit
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The launch patch for Spirit, featuring Marvin the Martian |
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Artist's conception of rover on Mars |
Spirit, MER-A (Mars Exploration Rover – A), active from 2004 to 2010. It was one of two rovers of NASA's ongoing Mars Exploration Rover Mission. It landed successfully on Mars at 04:35 Ground UTC on January 4, 2004, three weeks before its twin, Opportunity (MER-B), landed on the other side of the planet. Its name was chosen through a NASA-sponsored student essay competition. The rover became stuck in late 2009, and its last communication with Earth was sent on March 22, 2010.
![](http://upload.wikimedia.org/wikipedia/commons/thumb/a/a5/MER_Spirit_Lander_Pan_Sol16-A18R1_br2.jpg/220px-MER_Spirit_Lander_Pan_Sol16-A18R1_br2.jpg)
On May 1, 2009 (5 years, 3 months, 27 Earth days after landing; 21.6 times the planned mission duration), Spirit became stuck in soft soil. This was not the first of the mission's "embedding events" and for the following eight months NASA carefully analyzed the situation, running Earth-based theoretical and practical simulations, and finally programming the rover to make extrication drives in an attempt to free itself. These efforts continued until January 26, 2010 when NASA officials announced that the rover was likely irrecoverably obstructed by its location in soft soil, though it continued to perform scientific research from its current location.
The rover continued in a stationary science platform role until communication with Spirit stopped on sol 2210 (March 22, 2010). JPL continued to attempt to regain contact until May 24, 2011, when NASA announced that efforts to communicate with the unresponsive rover had ended. A formal farewell was planned at NASA headquarters after the Memorial Day holiday and was televised on NASA TV.
Mission overview
The primary surface mission for Spirit was planned to last at least 90 sols. The mission received several extensions and lasted about 2,208 sols. On August 11, 2007, Spirit obtained the second longest operational duration on the surface of Mars for a lander or rover at 1282 Sols, one Sol longer than the Viking 2 lander. Viking 2 was powered by a nuclear cell whereas Spirit is powered by solar arrays. Until Opportunity overtook it on May 19, 2010, the Mars probe with longest operational period was Viking 1 which lasted for 2245 Sols on the surface of Mars. On March 22, 2010, Spirit sent its last communication, thus falling just over a month short of surpassing Viking 1's operational record. An archive of weekly updates on the rover's status can be found at the Spirit Update Archive.
Spirit's total odometry as of March 22, 2010 (sol 2210) is 7,730.50 meters (4.80 mi).
- MER - B Opportunity
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The launch patch for Opportunity, featuring Duck Dodgers (Daffy Duck). |
Opportunity, MER-B (Mars Exploration Rover – B), is a robotic rover on the planet Mars, active since 2004. Launched from Earth on July 7, 2003, it landed on Meridiani Planum on January 25, 2004 at 05:05 Ground UTC (about 13:
15 local time). This was three weeks after its twin Spirit (MER-A), also part of NASA's Mars Exploration Rover Mission, touched down on the other side of the planet. Its twin became immobile in 2009 and in 2010 ceased communications, but MER-B is still active as of 2012, having already exceeded its planned duration of activity thirty times over.
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Opportunity in April 2003 (Before Launch) |
Mission highlights include completion of the 90 Sol (90 Martian days) mission, discovery of an extramartian meteorite (Meridiani Planum), and over two years studying Victoria crater. It survived dust-storms in 2007 and reached Endeavour crater in 2011, which has been described as the equivalent of a "second landing site". After conducting stationary science in the bleak winter months, it began moving again in May 2012.
Mission overview
The primary surface mission for Opportunity was planned to last 90 sols. The mission has received several extensions and has been operating for 3125 days since landing. An archive of weekly updates on the rover's status can be found at the OpportunityUpdate Archive.
From its initial landing, by chance, into an impact crater amidst an otherwise generally flat plain,Opportunity has successfully investigated soil and rock samples and taken panoramic photos of its landing site. Its sampling allowed NASA scientists to make hypotheses concerning the presence of hematite and past presence of water on the surface of Mars. Following this, it was directed to travel across the surface of Mars to investigate another crater site,Endurance crater, which it investigated from June – December 2004. Subsequently, Opportunity examined the impact site of its own heat shield and discovered an intact meteorite, now known as Heat Shield Rock, on the surface of Mars.
From late April 2005 to early June of that year, Opportunity was perilously lodged in a sand dune, with several wheels buried in the sand. Over a six week period Earth-based physical simulations were performed to decide how best to extract the rover from its position without risking a permanent immobilization of the valuable vehicle. Successful maneuvering a few centimeters at a time eventually freed the rover, which resumed its travels.
Opportunity was directed to proceed in a southerly direction to Erebus crater, a large, shallow, partially buried crater and a stopover on the way south towards Victoria crater, between October 2005 and March 2006. It experienced some mechanical problems with its robotic arm.
In late September 2006, Opportunity reached Victoria crater and explored along the rim in a clockwise direction. In June 2007 it returned toDuck Bay, its original arrival point; in September 2007 it entered the crater to begin a detailed study. In August 2008, Opportunity left Victoria crater for Endeavour crater, which it reached on August 9, 2011.[12]
Opportunity's total odometry as of July 24, 2012 (sol 3022) is 34,633.40 meters (21.52 mi).
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SOURCE: Wikipedia & NASA
Sunday, August 12, 2012
NASA's Mars Science Laboratory
Mars Science Laboratory OR MSL
![](http://upload.wikimedia.org/wikipedia/commons/thumb/3/3f/Drawing-of-the-Mars-Science_Laboratory.png/250px-Drawing-of-the-Mars-Science_Laboratory.png)
Goals and objectives
The MSL mission has four scientific goals: Determine the landing site's habitability including the role of water, the study of the climate and the geology of Mars. It is also useful preparation for a future manned mission to Mars.To contribute to these goals, MSL has six main scientific objectives:
- Determine the mineralogical composition of the Martian surface and near-surface geological materials.
- Attempt to detect chemical building blocks of life (biosignatures).
- Interpret the processes that have formed and modified rocks and soils.
- Assess long-timescale (i.e., 4-billion-year) Martian atmospheric evolution processes.
- Determine present state, distribution, and cycling of water and carbon dioxide.
- Characterize the broad spectrum of surface radiation, including galactic radiation, cosmic radiation, solar proton events and secondary neutrons.
History
NASA called for proposals for the rover's scientific instruments in April 2004, and eight proposals were selected on December 14 of that year. Testing and design of components also began in late 2004, including Aerojet's designing of a monopropellant engine with the ability to throttle from 15–100 percent thrust with a fixed propellant inlet pressure.By November 2008 most hardware and software development was complete, and testing continued. At this point, cost overruns were approximately $400 million. The next month, NASA delayed the launch to late 2011 because of inadequate testing time.
Between March 23–29, 2009, the general public ranked nine finalist rover names through a public poll on the NASA website. On May 27, 2009, the winning name was announced to be Curiosity. The name had been submitted in an essay contest by Clara Ma, a sixth-grader from Kansas.
![](http://upload.wikimedia.org/wikipedia/commons/thumb/e/ee/Atlas_V_541_into_the_flight.png/220px-Atlas_V_541_into_the_flight.png)
![](http://upload.wikimedia.org/wikipedia/commons/thumb/2/23/MSL-Cruise_Stage_Test.jpg/220px-MSL-Cruise_Stage_Test.jpg)
At the time of its landing, six mission leaders are John Grunsfeld, NASA associate administrator; Charles Elachi, director, JPL; Pete Theisinger, MSL project manager; Richard Cook, MSL deputy project manager; Adam Steltzner, MSL entry, descent and landing (EDL) lead; and John Grotzinger, MSL project scientist.
Source: Wikipedia & Google Image
About Me
Hey my name is Agastya i am 13 years old boy from indonesia from Bekasi to be exact if you doesn't know where Bekasi is it about 16 kilometers or 1 miles from the Capital city of Indonesia Jakarta.
I am a student in one of government own junior high school, its called SMPN 1 Bekasi or 1 junior high school. I study in the 8 Grade, my favorites subject at school is History,Chemistry and Geography and the subjects that I do not like is Math and physics because it require me to calculate a lot of number and remembering a lot of formula. The reason i like History is because the teacher always tell us some story about the lesson that we are learning and we just have to listen to our teacher and she rarely gave us home work.
Beside school lesson i also attend some extra-curricular activities too such as Boys scout & Badminton.
My Hobbies are Listening to music & Playing computer game, I like First Person Shooter(FPS) game such as Call Of Duty and Battle Field,by now already have all of the Call of duty series from the first to the Call Of Duty Modern warfare 3, About music i love singer like Jason Mraz, Katy Perry, Bruno Mars and Owl City.
i also interested in Space exploration program, i usually read news about NASA space program and I am very excited about the new NASA exploration program on mars,they just managed to land a car size 900Kg rover on mars
I will post song lyric with review and some other stuff in this blog
That's all from me right now
I am sorry if my english isn't very good
Beside school lesson i also attend some extra-curricular activities too such as Boys scout & Badminton.
My Hobbies are Listening to music & Playing computer game, I like First Person Shooter(FPS) game such as Call Of Duty and Battle Field,by now already have all of the Call of duty series from the first to the Call Of Duty Modern warfare 3, About music i love singer like Jason Mraz, Katy Perry, Bruno Mars and Owl City.
i also interested in Space exploration program, i usually read news about NASA space program and I am very excited about the new NASA exploration program on mars,they just managed to land a car size 900Kg rover on mars
I will post song lyric with review and some other stuff in this blog
That's all from me right now
I am sorry if my english isn't very good
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