Showing posts with label Space Portal. Show all posts
Showing posts with label Space Portal. Show all posts

Wednesday, 5 April 2017

Mars Reconnaissance Orbiter Completes 50000th Orbit around Mars.



                                    Mars Reconnaissance Orbiter is an american spacecraft designed to conduct multiple experiment for the exploration of Mars. It was designed under the supervision of NASA Project director Lookheed Martin ( Jet Propulsion Laboratory) and it was controlled by California Institute of Technology,USA. It was launched on 12 August 2005 from Cape Canaveral Air force station and reached mars orbit on 10 March 2010. It became one of the five active mission on Mars (2001 Mars odyssey, Mars Global Surveyor, Mars Express, Mars Exploration Rovers ( Twin Rovers = Spirit and Opportunity). It became the best relay satellite for the measurement of weather monitoring, choose site for future landing missions and an intermediate to communicate between the Mars Exploration Rovers and Earth. It carried many scientific instruments such as radars, spectrometers to study mars. It is listed as one of the currently active mission on Mars. It completed its 50,000th orbit around Mars on 27 March 2017.

Wednesday, 1 March 2017

Ultra-fast Black. Hole

Scientists from Michael Parker institute of Astronomy , Cambridge found an ultrafast wind flowing from the vicinity of a blackhole at nearly quarter of the speed of light.
Outflowing of gas is the common feature of supermassive black holes that reside in the centre of the galaxies. They have massive gas which is million or billion times larger than the sun. This ultra-fast black hole feed out the surrounding gases and stars supressing the birth of new stars. Space telescope saw this bright emmission, including Xrays from the innermost part of the disc around that black hole.

    These winds are an important characteristics to study, because it has strong influence on regulating the growth of host galaxies. These ultrafast blackhole has been found by European Space Agency's XMM Newton and NASA  Nustar telescopes. Scientists found this galaxy named or identified as IRAS-13224-3809. The velocity of gases in this Blackhole is around 71000 km/s. 0.24 times the speed of the light which is 300000 km/s.
   They took this image after focusing for a period of 17 days straight revealing the variable nature of winds. After a long observation campaign, they have seen the changes such as increase in temperature of winds and greater X-ray emission from the disc right next to the black hole. It will help us to  understand that how black hole winds get launched and accelerated, how moderate star formed in the host galaxy.

Wednesday, 22 February 2017

Juno Mission till 2018

Juno Jupiter Orbital around gas giant since July 4,2016 will remain to active till July 2018. It is in its current 53 day orbit around Jupiter. This will allow Juno to accomplish its goals, avoiding the risk of engine firing previously.. It already reduced the orbital period of 14 days of this Spacecraft. Juno is healthy and its instruments are operational. Juno completed its orbit around Jupiter for four times. Recently orbited in February 2,2017. The next close flyby to Jupiter on March 27, 2017. June's mission will be extended in the next review cycle..  Credit: Nasa

Friday, 17 February 2017

Alnitak Star

           Students from (ACPU) Astro Club Of Pondicherry University took photo of Alnitak Star from their hand made telescope. The southern most bright star in the Orion belt..

Congrats and All the very best to ACPU students. Pondicherry University.

Monday, 13 February 2017

Hourglass Nebulae


            The Hourglass Nebulae otherwise called Mycn18 is located 8000 light years away from earth. This picture has been composed of three separate images taken in the light if  ionized nitrogen (represented by red) doubly ionized oxygen (blue) hydrogen (green). #Hubble updates....

Credit: European Space Agency

Sunday, 12 February 2017

Supernova Exploison in 2022

SUPERNOVA EXPLOSION IN 2022

       Since decades research have been going on about the supernova blast. Researchers said that in 2022 there will be a huge explosion of supernova in our Milky way galaxy. We can see the explosive light of supernova from Earth with our naked eye. The explosive light will remain in the night sky for minimum one year. Further research is going on about this massive supernova . If it comes true, we were the luckiest people's to see such explosion.

Wednesday, 8 February 2017

Calabash Nebulae ( Rotten egg's Nebulae )

   The calabash nebulae is known as rotten egg nebulae, it is transitioning from red giant nebulae to planet nebulae.. It is located nearly 5000 light years from the Earth. It mostly contains sulfur, that's why it is called rotten egg's nebulae... This image has been taken by esa/ NASA Hubble space telescope..




It look like yellow color due to sulfur content. It moves with a speed of 1 million kilometer per hour...

The gas in blue is the surrounding material being pushed out of the way. The big acceleration likely started about 800 years ago,according to NASA. But the frantic pace won't last long, on a cosmic scale, before it transitions to a more long-lasting, slowly expanding feature.

Wednesday, 1 February 2017

NGC-6861 Hubble Space Telescope

This is NGC 6861, seen by the NASA/ESA Hubble Space Telescope. One of the Most prominent features in the disk of dark bands circling the centre of thus galaxy. These dust lanes are a result of large clouds of dust particles obscuring the light emitted by the Stars behind them.

The subject of this image is NGC 6861, a galaxy discovered in 1826 by the Scottish astronomer James Dunlop. Almost two centuries later we now know that NGC 6861 is the second brightest member of a group of at least a dozen galaxies called the Telescopium Group — otherwise known as the NGC 6868 Group — in the small constellation of Telescopium (The Telescope).
This NASA/ESA Hubble Space Telescope view shows some important details of NGC 6861. One of the most prominent features is the disc of dark bands circling the centre of the galaxy. These dust lanes are a result of large clouds of dust particles obscuring the light emitted by the stars behind them.
Dust lanes are very useful for working out whether we are seeing the galaxy disc edge-on, face-on or, as is the case for NGC 6861, somewhat in the middle. Dust lanes like these are typical of a spiral galaxy. The dust lanes are embedded in a white oval shape, which is made up of huge numbers of stars orbiting the centre of the galaxy. This oval is, rather puzzlingly, typical of an elliptical galaxy.
So which is it — spiral or elliptical? The answer is neither! NGC 6861 does not belong to either the spiral or the elliptical family of galaxies. It is a lenticular galaxy, a family which has features of both spirals and ellipticals.
The relationships between these three kinds of galaxies are not yet well understood. A lenticular galaxy could be a faded spiral that has run out of gas and lost its arms, or the result of two galaxies merging. Being part of a group increases the chances for galactic mergers, so this could be the case for NGC 6861.
A version of this image was entered into the Hubble’s Hidden Treasures image processing competition by contestant Josh Barrington.
Credit: ESA/NASA


Source: Main page of ESA/NASA

Tuesday, 24 January 2017

Small GEO's ride Arrives at ESA


                         The Soyuz launcher that will carry SmallGEO's first flight into orbit was transferred to its launch zone at Europe's Spaceport in Kourou, French Guiana

Monday, 16 January 2017

SmallGEO/H36W-! ESA

A special media briefing on SmallGEO and its first flight is taking place on Wednesday 18 January, at ESA HQ in Paris, following on from Director General Jan Woerner's annual meeting of the press.  

SmallGEO is a multipurpose satellite platform capable of accommodating a wide range of commercial telecommunications payloads and missions, from TV broadcasting to multimedia applications, Internet access and mobile or fixed services in a wide range of frequency bands. 

Its new, modular and flexible design boosts European industry’s ability to play a significant role in commercial satcoms by easing entry into the lower-mass telecom satellite market. It was developed by Germany's OHB System AG under ESA's ARTES Advanced Research in Telecommunications Systems programme.  

Hispasat's Hispasat 36W-1 will be the first satellite to use the SmallGEO platform, marking the first partnership between ESA and a Spanish operator. It is set for launch in the early hours of 28 January (CET) from Europe's Spaceport in Kourou, French Guiana.  

H36W-1 will provide Europe, the Canary Islands and South America with faster multimedia services through its Redsat payload, which offers better signal quality and flexible land coverage. Redsat enables H36W-1 to provide advanced connectivity services based on the latest communication standards. 

The briefing will be shared by the Director General and the Director of Telecommunications & Integrated Applications, Magali Vaissiere. Speakers include Carlos Espinós, Hispasat CEO, Andreas Lindenthal, of OHB System AG's Management Board and Gerd Gruppe, Director of Space Administration at the DLR German Aerospace Center. It will be followed by a Q&A. Media and the public may ask questions during the briefing on Twitter to @esa using the hashtag #askSmallGEO.

UK at the forefront of NASA's CYGNSS mission

A UK company is at the forefront of NASA’s latest Earth observation mission to see inside tropical storms and hurricanes like never before.

Surrey Satellite Technology has developed the Space GNSS Receiver Remote Sensing Instrument (SGR-ReSI) for the Cyclone Global Navigation Satellite System (CYGNSS) mission providing scientists with innovative satellite technology.
The CYGNSS mission, which launched from Cape Canaveral Air Force Station in Florida on 15 December, is part of a NASA programme to improve extreme weather prediction by studying how tropical cyclones form.

CYGNSS will measure ocean surface winds in and near a hurricane’s inner core, including regions previously could not be measured from space. CYGNSS will use both direct and reflected satellite navigation signals to obtain estimates of surface wind speed over the ocean.

Surrey Satellite Technology demonstrated the technology for the first time on its UK-DMC mission launched in 2003. It has subsequently developed the SGR-ReSI with sponsorship from the UK Space Agency, Innovate UK and the UK Centre for Earth Observation and Instrumentation and Space Technology. The first flight of the SGR-ReSI is on the UK TechDemoSat-1 mission, with exploitation support from the European Space Agency.

The UK is already a world-leader in satellite technology and Earth observation. In September the UK Space Agency unveiled new support to help the UK space sector maintain its leading position in Earth observation, helping to tackle global issues such as deforestation and disaster monitoring. This support included a new £2m joint programme for UK companies and academia to develop innovative technologies to observe the Earth from space.

Working together with the University of Leicester, Airbus Defence and Space UK, and RAL Space, the £2m funding from UK Space Agency will support UK companies and academia to develop their technologies and help them gain access to government funding worth up to £10 million.

For more information on the UK’s involvement in the mission, check out the SSTL website.

Wednesday, 11 January 2017

Air Force's Mysterious X-37B Space Plane Wings by 600 Days in Orbit

The U.S. Air Force's mysterious X-37B space plane has now spent 600 days in Earth orbit on the vessel's latest mission, and is nearing a program record for longest time spent in space.

The robotic X-37B lifted off atop a United Launch Alliance Atlas V rocket from Florida's Cape Canaveral Air Force Station on May 20, 2015, kicking off the program's fourth space mission (which is known as Orbital Test Vehicle-4, or OTV-4).
If the uncrewed spacecraft spends 74 more days aloft, it will break the duration record set during OTV-3, which touched down in October 2014.




The first OTV mission began on April 22, 2010, and concluded on Dec. 3 of that year, following 224 days of orbit. OTV-2 lifted off on March 5, 2011, and landed on June 16, 2012, after 468 days in orbit.
The record-setting OTV-3 mission chalked up nearly 675 days in orbit, circling Earth from Dec. 11, 2012, until Oct. 17, 2014.
All three previous OTV missions have come down to Earth at Vandenberg Air Force Base in California, but that may change for OTV-4's landing, whenever it occurs.

Progress has been made on consolidating X-37B space plane operations, including the use of NASA's Kennedy Space Center (KSC) in Florida as a landing site for the robotic space plane.
A former KSC space-shuttle facility known as Orbiter Processing Facility-1 (OPF-1) was converted into a structure that will enable the Air Force "to efficiently land, recover, refurbish and relaunch the X-37B Orbital Test Vehicle (OTV)," according to representatives of the aerospace giant Boeing.
X-37B vehicle development falls under the control of Boeing Space and Intelligence Systems in El Segundo, California, which is Boeing's center for all space and experimental systems and government and commercial satellites.
The Air Force Rapid Capabilities Office is leading the Department of Defense's OTV initiative, by direction of the under secretary of defense for acquisition, technology and logistics and the secretary of the Air Force.


Fleet size

 The U.S. Air Force's X-37B space plane waits in the encapsulation cell of the Evolved Expendable Launch Vehicle on April 5, 2010, at the Astrotech facility in Titusville, Florida. The vehicle launched on the first X-37B mission on April 22, 2010.

To date, only two reusable X-37B vehicles have been confirmed as constituting the space plane fleet. The current OTV-4 mission is the second flight of the second X-37B vehicle built for the Air Force by Boeing.

The military space plane looks like a miniature version of NASA's retired space shuttle orbiter. The X-37B is just 29 feet (8.8 meters) long and 9.6 feet (2.9 m) tall, and has a wingspan of nearly 15 feet (4.6 m). For comparison, the space shuttles were each 122 feet (37 m) long, with wingspans of 78 feet (24 m).
The X-37B has a payload bay about the size of a pickup truck bed that can be outfitted with a robotic arm. It has a launch weight of 11,000 lbs. (4,990 kilograms) and is powered in orbit by gallium arsenide solar cells with lithium-ion batteries.
Some payloads aboard the OTV-4 craft have been previously identified.
For example, Aerojet Rocketdyne has said that its XR-5A Hall Thruster had completed initial in-orbit validation testing aboard the X-37B space plane. Also on board is a NASA advanced-materials investigation.

Such test-bedding of equipment is one of the main purposes of OTV missions, along with the development of reusable-spacecraft technologies, Air Force officials have said.  
"It remains a very useful way to test out things," Winston Beauchamp, deputy undersecretary of the Air Force for space, told Space.com last September during an American Institute of Aeronautics and Astronautics (AIAA) meeting in Long Beach, California.



Tuesday, 10 January 2017

New Opportunity For Space Industry

New opportunity for space industry - NASA announced on April 21, 2016 that they would like to spend some money on new satellite. Martian satellite of course!

In spite of plans of cooperation with SpaceX during their Mars mission planned for 2018, NASA still has developing own Mars program with Mars 2020 mission which will consist of lander and Mars rover. In spite of progress in Mars 2020, NASA would like to launch in 2020 Martian satellite, which will be support in further manned journey to Mars. Spacecraft will be imaging satellite operating in high resolution with necessary communication equipment for lossless and fast downlink. It could be also considered as communication support of Mars rover which should land on Red Planet on 2020. Also it is planned to utilize satellite as platform for various science experiments and testing new technologies. Responsible for planning mission and formulating technical demands for satellite is Jet Propulsion Laboratory, which also will be responsible for Mars 2020 mission. To sum up, satellite will be testing platform for new technologies, will be equipped in highly efficient communication instruments and will be developed under public-private partnership. As far as testing new technologies it will be mainly focused on technologies useful during future Mars exploration. First place among of planned subjects of experiments is new highly efficient solar electric propulsion which is recently developed by NASA under Advanced Electric Propulsion System (AEPS) program. Next crucial technology in further Mars exploration is new fast optical communication system. If conventional radio communication is useful in robotic missions, during manned mission even delay of 11 minutes while Mars is closest to Earth could have crucial meaning. Sense of the new satellite mission was well described by John Grunsfeld, associate administrator of NASA’s Science Mission Directorate:
“Our success in exploring Mars, to unravel the mysteries of the Red Planet, depends on having high bandwidth communication with Earth and overhead imaging,.. Currently, we depend on our orbiting science missions to perform dual service in making measurements and acting as communication relays, but we can’t depend on them to last forever. This new orbiter will use cutting-edge technology to revitalize our ability to continue to explore Mars and support transformative science, including a potential sample return mission in the future.”

For this mission NASA also would like to acquire international partners to extend as much as possible usage of opportunities given by satellite. This mission is third planned for next four years and focused on Mars. Insight, cooperation with DLR and CNES is planned for 2018 and landing of next Mars rover is scheduled for 2020. NASA still is trying to keep its conception of leaving LEO for commercial companies and focus on deep space exploration, but after unveiling recently by Spacenews.com, fact that budget for future Mars landing technology demonstrator was reduced for 85%, satellite mission with potential first contracts for concept studies for $400000 (contest for satellite concept will be announced after further four months) is much more less expectable than developing Mars lander. If we combine these facts with SpaceX plan for Mars mission in 2018 with landing, gathering probes and return to Earth we will see that NASA seems to leave Mars for commercial companies (it seems that only remaining question is how deep should be space to not be left by NASA to SpaceX...).
Sources:

http://www.nasa.gov/press-release/nasa-seeks-industry-ideas-for-an-advanced-mars-satellite

Asteroid sleuths go back to the future

                        ASTEROID SLEUTHS GO BACK TO THE FUTURE
10 January 2017
 
Careful sleuthing through decade-old images has enabled ESA’s asteroid team to decide that a newly discovered space rock poses little threat of hitting Earth any time soon.
Spotting a previously unknown asteroid for the first time always raises the big question: is there a risk it will impact Earth?
Yet, upon discovery, analysts often have very little to go on. The initial image from the observatory, survey team or individual backyard astronomer who spotted the rock typically gives only basic information – its location in the sky and its brightness – and sometimes these aren’t known terribly accurately.
The most crucial information needed to determine with any degree of confidence whether it is a ‘near-Earth object’ (NEO) – and that it will miss Earth (or not) – is the new object’s path. And determining that requires a series images acquired over a period of days or even months.
“We need multiple follow-on images to compute the trajectory and make a risk estimate, but even then the uncertainty can be very large. It really takes many months of observations to get a good, reliable impact risk estimate, and in the meantime, there can be reason to worry,” says Ettore Perozzi of the NEO Coordination Centre at ESA’s facility in Italy. 

Spotted from Arizona: 

This is precisely what happened on 19 October, when asteroid 2016 WJ1 was discovered by the Catalina Sky Survey.
Additional images were taken by observers worldwide over the next few weeks, including by a team working at ESA’s own observatory on Tenerife in the Canary Islands, but uncertainty of the path meant that a possible close approach in June 2065 – with a worrying impact probability of about 1 in 8000 – could not be excluded.
“The additional images allowed us to refine our knowledge of the trajectory sufficiently to begin searching astronomical archives, to see if anyone had previously imaged this asteroid without having recognised it as such,” says Marco Micheli, observer at the NEO centre.
If any were found, the team would score what astronomers call a ‘precovery’ – short for pre-discovery.

Precovering: 

The investigation quickly bore fruit: images found online from the Pan-STARRS survey taken earlier in October showed what might be the target asteroid.
While these were inconclusive, the team assumed they were, in fact, accurate and then used these to call up additional, highly accurate images from a Canadian astronomical image search system.

Bingo: two sets of images from 4 and 5 July 2003 with the Canada–France–Hawaii Telescope were found.
“After careful inspection we were able to pinpoint the object, and the team were able to perform some very accurate determinations,” says Detlef Koschny, responsible for the NEO portion of ESA’s Space Situational Awareness programme.
“The result was that we could preclude any risk of Earth impact from asteroid 2016 WJ1 anytime soon or well into the future.”
ESA is now developing a new set of automated, wide-field-of-view ‘Fly-Eye’ telescopes that will conduct nightly sky surveys, creating a large future archive of images that will make critical precovery confirmations more efficient in future.

First Colour Image of UK and Algerian Cubesat

   First colour image for joint UK and Algerian CubeSat

Image taken from space of the Arkhangelsk Oblast region, on the North West coast of Russia. Image courtesy Alsat Nano mission, Open University, December 2016
 
AlSat Nano, a UK-Algeria CubeSat mission, has captured its first full colour image following its launch in September 2016. The image was taken by the Open University C3D2 instrument's wide field camera on 3rd December, 2016, over the Arkhangelsk Oblast region, on the North West coast of Russia. It was captured under twilight conditions at dawn, showing the coastline to the top, and a brief winter sunrise over the arctic region with a deep red-brown hue.

Through the cloud cover there is evidence of hills and snow on mountains, and mist in the river valleys. The object in the foreground is the Oxford Space Systems Ltd AstroTubeTM Boom payload, also carried on board the spacecraft.

This marks an important milestone for the mission as all core payloads have now been commissioned successfully, paving the way for further scientific and commercial exploitation.

Dr Chris Castelli, UK Space Agency Director of Programmes said: "Successfully delivering this joint UK-Algeria mission from payload selection to launch readiness in 18 months is a great achievement from all programme partners. As this latest image demonstrates, mission operations are going from strength to strength, validating cutting edge UK space technology and our open approach to working with international partners."

AlSat Nano is Algeria's first CubeSat mission and shows the capability of UK technology in partnership with industry and academia. With a spacecraft the size of a shoebox yet featuring all the core subsystems of much larger satellites, the programme demonstrates how CubeSats can be assembled quickly and launched at a fraction of the cost. This will help Algeria strengthen its domestic space technology capability by giving their scientists and engineers first-hand experience of spacecraft operations.

Dr Abdewahab Chikouche, Director of Space Programmes at Algerian Space Agency, said: "The Alsat-1N project is a concrete example of the success of our cooperation with UKSA. This project, very enriching from the scientific and technological point of view, allowed ASAL engineers to progress in the integration and testing of nanosatellites and acquire autonomy in its operation. This project will enable Algerian researchers and academics to strengthen national capabilities in advanced space technology."

Approximately half of the spacecraft's volume was made available as part of an open call to the UK CubeSat community as a free flight opportunity for self-funded payloads. AlSat Nano stuck to a tight development schedule, with less than 18 months between payload selection and flight readiness.

Prof Guglielmo Aglietti, Director of Surrey Space Centre said: "AlSat Nano has been an exciting project for the Surrey Space Centre to be leading. Educational and research elements, and the technology knowledge transfer with the Algerian Space Agency were key parts of this project. Additionally, the development of this nanosatellite platform has been a great opportunity to work with UK payload providers, who are demonstrating some exciting new technologies."

Monday, 9 January 2017

Dark Nebulae Glows Red

                       Dark Nebula Glows Red in Amateur Astronomer's Photo



Thick blankets of dust surround the predominantly dark region in Barnard 343, a dark nebula in the constellation Cygnus.
Astrophotographer Jeffrey O. Johnson took this image from his backyard in Las Cruces, New Mexico.

Barnard 343 belongs to the Gamma Cygni Complex – a group of clouds in Cygnus approximately 2,000 light-years away. A light-year is the distance light travels in one year, or about 6 trillion miles (10 trillion kilometers). 
The brilliant red regions are caused by a large amount of hydrogen emissions present in the visible part of the spectrum. Johnson used a Takahashi TOA-130F @ f/7.7 telescope with a Takahashi EM200 Temma II Mount with a QSI 540wsg @ -15C camera.

Saturday, 7 January 2017

Earth Image from Mars Reconnaissance Orbitor


            IMAGE OF EARTH FROM MARS RECONNAISSANCE ORBITOR

                                A  NASA spacecraft has given humanity a breathtaking, Mars-eye view of Earth and its moon.

The Mars Reconnaissance Orbiter (MRO) used its High Resolution Imaging Science Experiment (HiRISE) camera to capture this new telescopic image of our planet and its natural satellite on Nov. 20, 2016. At the time, Mars and Earth were about 127 million miles (205 million kilometers) apart, NASA officials said.
The amazing new photo is actually a composite of two separate exposures taken to calibrate HiRISE, which is so powerful that it's able to resolve features as small as 3.3 feet (1 meter) across on the Martian surface from MRO's orbital perch.

"The combined view retains the correct positions and sizes of the two bodies [Earth and the moon] relative to each other," NASA officials wrote in a description of the image, which was released today (Jan. 6). 

"The distance between Earth and the moon is about 30 times the diameter of Earth," they added. "Earth and the moon appear closer than they actually are in this image because the observation was planned for a time at which the moon was almost directly behind Earth, from Mars' point of view, to see the Earth-facing side of the moon."

The newly released image is sharp enough to reveal continent-size details on Earth; indeed, the reddish-brown feature in the middle of the planet is Australia, NASA officials said.
The $720 million MRO mission launched in August 2005 and slipped into orbit around the Red Planet in March 2006. For the past decade-plus, the probe has been studying Martian geology and climate; looking for signs of past water activity on the planet's surface; providing a vital communications link between Mars surface craft such as the Curiosity rover and their handlers here on Earth; and helping researchers evaluate potential landing sites for future robotic and human missions, among other tasks.

Space X Falcon 9

                  SPACE X ( FALCON 9 OVERVIEW & UPDATES )

WASHINGTON — An explosion on a Florida launch pad early Sept. 1 destroyed a SpaceX Falcon 9 rocket and its payload, the Amos-6 communications satellite, being prepared for an upcoming launch there.

Authorities said the explosion occurred at approximately 9:07 a.m. Eastern at Space Launch Complex 40 at Cape Canaveral Air Force Station, where SpaceX was preparing to conduct a static fire test of the Falcon 9 in advance of a scheduled Sept. 3 launch. The test, which entails briefly firing the rocket’s first stage, is a routine pre-launch procedure for Falcon 9 missions.
SpaceX Chief Executive Elon Musk, in a tweet four hours after the incident, said the explosion originated around the Falcon 9’s the upper stage liquid oxygen tank while it was being loaded in the minutes before the scheduled static fire test. He said there was no information yet on the cause of the explosion.

SpaceX confirmed both the Falcon 9 and its Amos-6 payload were lost in the explosion, but that there were no injuries in the explosion. “SpaceX can confirm that in preparation for today’s static fire, there was an anomaly on the pad resulting in the loss of the vehicle and its payload. Per standard procedure, the pad was clear and there were no injuries,” SpaceX said via Twitter.

The loss of Amos-6 is a major, untimely setback for its owner, Spacecom. With a pending sale of the Israeli satellite fleet operator contingent on the successful launch of Amos-6, shares of Spacecom’s stock fell sharply as the first reports of an explosion began rolling in.

A major user of Amos-6 was to be Facebook, the social networking company that purchased the Ka-band capacity of the satellite to provide Internet access to underserved regions of sub-Saharan Africa. “We are disappointed by the loss but remain committed to our mission of connecting people to the Internet around the world,” a Facebook spokesperson said Sept. 1.

The failure is also a setback to several other companies preparing to launch payloads on the Falcon 9, most notably Iridium. It had planned to launch its first ten next-generation satellites on a Falcon 9 from Vandenberg Air Force Base in California later in September, a launch likely to be delayed by at least several weeks while this incident is investigated.

SpaceX, which has launched eight times this year, faced a crowded end-of-the-year manifest. Nine customers were still expecting to launch on Falcon 9 before January; all but three of those missions were to lift off from Florida. SpaceX also hoped to squeeze in the first flight of its new Falcon Heavy rocket.

The failure could also have repercussions in civil and military space. SpaceX provides commercial cargo services for NASA and is developing a commercial crew system, while it is also competing for national security launches once in the exclusive domain of United Launch Alliance.

“Today’s incident reminds us all that space flight is an inherently risky business,” said Sen. Bill Nelson (D-Fla.), ranking member of the Senate Commerce Committee, in a statement issued shortly after the explosion. “As we continue to push the frontiers of space, there will be both triumphs and setbacks. But at the end of the day, I’m confident that our commercial space industry will be very successful.”

Updates as on Jan 2, 2017
 

January 2, 2017, 9:00am EST

Over the past four months, officials at the Federal Aviation Administration (FAA), the U.S. Air Force (USAF), the National Aeronautics and Space Administration (NASA), the National Transportation Safety Board (NTSB), along with several industry experts, have collaborated with SpaceX on a rigorous investigation to determine the cause of the anomaly that occurred September 1 at Space Launch Complex 40 (SLC-40) at Cape Canaveral Air Force Station in Florida. This investigation team was established according to SpaceX's accident investigation plan as approved by the FAA. As the primary federal licensing body, the FAA provided oversight and coordination for the investigation.

Investigators scoured more than 3,000 channels of video and telemetry data covering a very brief timeline of events – there were just 93 milliseconds from the first sign of anomalous data to the loss of the second stage, followed by loss of the vehicle. Because the failure occurred on the ground, investigators were also able to review umbilical data, ground-based video, and physical debris. To validate investigation analysis and findings, SpaceX conducted a wide range of tests at its facilities in Hawthorne, California and McGregor, Texas. 

The accident investigation team worked systematically through an extensive fault tree analysis and concluded that one of the three composite overwrapped pressure vessels (COPVs) inside the second stage liquid oxygen (LOX) tank failed. Specifically, the investigation team concluded the failure was likely due to the accumulation of oxygen between the COPV liner and overwrap in a void or a buckle in the liner, leading to ignition and the subsequent failure of the COPV. 

Each stage of Falcon 9 uses COPVs to store cold helium which is used to maintain tank pressure, and each COPV consists of an aluminum inner liner with a carbon overwrap. The recovered COPVs showed buckles in their liners. Although buckles were not shown to burst a COPV on their own, investigators concluded that super chilled LOX can pool in these buckles under the overwrap. When pressurized, oxygen pooled in this buckle can become trapped; in turn, breaking fibers or friction can ignite the oxygen in the overwrap, causing the COPV to fail. In addition, investigators determined that the loading temperature of the helium was cold enough to create solid oxygen (SOX), which exacerbates the possibility of oxygen becoming trapped as well as the likelihood of friction ignition.

The investigation team identified several credible causes for the COPV failure, all of which involve accumulation of super chilled LOX or SOX in buckles under the overwrap. The corrective actions address all credible causes and focus on changes which avoid the conditions that led to these credible causes. In the short term, this entails changing the COPV configuration to allow warmer temperature helium to be loaded, as well as returning helium loading operations to a prior flight proven configuration based on operations used in over 700 successful COPV loads. In the long term, SpaceX will implement design changes to the COPVs to prevent buckles altogether, which will allow for faster loading operations.​ 

SpaceX is targeting return to flight from Vandenberg's Space Launch Complex 4E (SLC-4E) with the Iridium NEXT launch on January 8. SpaceX greatly appreciates the support of our customers and partners throughout this process, and we look forward to fulfilling our manifest in 2017 and beyond.

December 7, 10:30am EDT
We are finalizing the investigation into our September 1 anomaly and are working to complete the final steps necessary to safely and reliably return to flight, now in early January with the launch of Iridium-1. This allows for additional time to close-out vehicle preparations and complete extended testing to help ensure the highest possible level of mission assurance prior to launch.

October 28, 4:00pm EDT
The Accident Investigation Team continues to make progress in examining the anomaly on September 1 that led to the loss of a Falcon 9 and its payload at Launch Complex 40 (LC-40), Cape Canaveral Air Force Station, Florida.

Since the incident, investigators from SpaceX, the FAA, NASA, the US Air Force and industry experts have been working methodically through an extensive fault tree to investigate all plausible causes. As part of this, we have conducted tests at our facility in McGregor, Texas, attempting to replicate as closely as possible the conditions that may have led to the mishap.

The investigation team has made significant progress on the fault tree. Previously, we announced the investigation was focusing on a breach in the cryogenic helium system of the second stage liquid oxygen tank. The root cause of the breach has not yet been confirmed, but attention has continued to narrow to one of the three composite overwrapped pressure vessels (COPVs) inside the LOX tank. Through extensive testing in Texas, SpaceX has shown that it can re-create a COPV failure entirely through helium loading conditions. These conditions are mainly affected by the temperature and pressure of the helium being loaded.

SpaceX’s efforts are now focused on two areas – finding the exact root cause, and developing improved helium loading conditions that allow SpaceX to reliably load Falcon 9. With the advanced state of the investigation, we also plan to resume stage testing in Texas in the coming days, while continuing to focus on completion of the investigation. This is an important milestone on the path to returning to flight.
Pending the results of the investigation, we continue to work towards returning to flight before the end of the year. Our launch sites at Kennedy Space Center, Florida, and Vandenberg Air Force Base, California, remain on track to be operational in this timeframe.

September 23, 1:00pm EDT
Three weeks ago, SpaceX experienced an anomaly at our Launch Complex 40 (LC-40) at Cape Canaveral Air Force Station. This resulted in the loss of one of our Falcon 9 rockets and its payload.

The Accident Investigation Team (AIT), composed of SpaceX, the FAA, NASA, the U.S. Air Force, and industry experts, are currently scouring through approximately 3,000 channels of engineering data along with video, audio and imagery. The timeline of the event is extremely short – from first signs of an anomaly to loss of data is about 93 milliseconds or less than 1/10th of a second. The majority of debris from the incident has been recovered, photographed, labeled and catalogued, and is now in a hangar for inspection and use during the investigation.

At this stage of the investigation, preliminary review of the data and debris suggests that a large breach in the cryogenic helium system of the second stage liquid oxygen tank took place. [Updated 09/24: At this time, the cause of the potential breach remains unknown.] All plausible causes are being tracked in an extensive fault tree and carefully investigated. Through the fault tree and data review process, we have exonerated any connection with last year’s CRS-7 mishap.

The teams have continued inspections of LC-40 and the surrounding facilities. While substantial areas of the pad systems were affected, the Falcon Support Building adjacent to the pad was unaffected, and per standard procedure was unoccupied at the time of the anomaly. The new liquid oxygen farm – e.g. the tanks and plumbing that hold our super-chilled liquid oxygen – was unaffected and remains in good working order. The RP-1 (kerosene) fuel farm was also largely unaffected. The pad’s control systems are also in relatively good condition.

SpaceX’s other facilities, from the Payload Processing Facility at the Cape, to the pad and hangar at LC-39A, are located several miles from LC-40 and were unaffected as well. Work continues at Pad 39A in preparation for bringing it online in November. The teams have been in contact with our Cape Canaveral and Kennedy Space Center partners and neighbors and have found no evidence of debris leaving the immediate area of LC-40.

At SpaceX headquarters in Hawthorne, CA, our manufacturing and production is continuing in a methodical manner, with teams continuing to build engines, tanks, and other systems as they are exonerated from the investigation. We will work to resume our manifest as quickly as responsible once the cause of the anomaly has been identified by the Accident Investigation Team. Pending the results of the investigation, we anticipate returning to flight as early as the November timeframe.

Other efforts, including the Commercial Crew Program with NASA, are continuing to progress. Getting back to flight safely and reliably is our top priority, and the data gathered from the present investigation will result in an even safer and more reliable vehicle for our customers and partners.

September 2, 6:45pm EDT
SpaceX has begun the careful and deliberate process of understanding the causes and fixes for yesterday's incident.  We will continue to provide regular updates on our progress and findings, to the fullest extent we can share publicly.

We deeply regret the loss of AMOS-6, and safely and reliably returning to flight to meet the demands of our customers is our chief priority.  SpaceX's business is robust, with approximately 70 missions on our manifest worth over $10 billion.  In the aftermath of yesterday's events, we are grateful for the continued support and unwavering confidence that our commercial customers as well as NASA and the United States Air Force have placed in us.

Overview of the incident:
- Yesterday, at SpaceX's Launch Complex 40 at Cape Canaveral Air Force Station, an anomaly took place about eight minutes in advance of a scheduled test firing of a Falcon 9 rocket.
- The anomaly on the pad resulted in the loss of the vehicle.
- This was part of a standard pre-launch static fire to demonstrate the health of the vehicle prior to an eventual launch. 
- At the time of the loss, the launch vehicle was vertical and in the process of being fueled for the test.  At this time, the data indicates the anomaly originated around the upper stage liquid oxygen tank.  Per standard operating procedure, all personnel were clear of the pad.  There were no injuries.

To identify the root cause of the anomaly, SpaceX began its investigation immediately after the loss, consistent with accident investigation plans prepared for such a contingency.  These plans include the preservation of all possible evidence and the assembly of an Accident Investigation Team, with oversight by the Federal Aviation Administration and participation by NASA, the United States Air Force and other industry experts.  We are currently in the early process of reviewing approximately 3000 channels of telemetry and video data covering a time period of just 35-55 milliseconds.

As for the Launch Pad itself, our teams are now investigating the status of SLC-40.  The pad clearly incurred damage, but the scope has yet to be fully determined.  We will share more data as it becomes available.  SpaceX currently operates 3 launch pads – 2 in Florida and 1 in California at Vandenberg Air Force Base.  SpaceX's other launch sites were not affected by yesterday's events.  Space Launch Complex 4E at Vandenberg Air Force Base is in the final stages of an operational upgrade and Launch Complex 39A at Kennedy Space Center remains on schedule to be operational in November.  Both pads are capable of supporting Falcon 9 and Falcon Heavy launches.  We are confident the two launch pads can support our return to flight and fulfill our upcoming manifest needs.

Again, our number one priority is to safely and reliably return to flight for our customers, as well as to take all the necessary steps to ensure the highest possible levels of safety for future crewed missions with the Falcon 9. We will carefully and thoroughly investigate and address this issue.
September 2, 9:00am EDT
Statement from SpaceX President and COO, Gwynne Shotwell:
“We deeply regret the loss of Amos-6.  Our number one priority is to safely and reliably return to flight for our customers, and we will carefully investigate and address this issue.  We are grateful for the continued support that our customers have expressed to us.”

September 1, 1:28pm EDT 
At approximately 9:07 am ET, during a standard pre-launch static fire test for the AMOS-6 mission, there was an anomaly at SpaceX’s Cape Canaveral Space Launch Complex 40 resulting in loss of the vehicle.

The anomaly originated around the upper stage oxygen tank and occurred during propellant loading of the vehicle. Per standard operating procedure, all personnel were clear of the pad and there were no injuries.
We are continuing to review the data to identify the root cause. Additional updates will be provided as they become available.

September 1, 10:22am EDT
SpaceX can confirm that in preparation for today's static fire, there was an anomaly on the pad resulting in the loss of the vehicle and its payload. Per standard procedure, the pad was clear and there were no injuries
 
Space X Falcon Launch: 
 
GRAPEVINE, Texas — The U.S. Federal Aviation Administration (FAA) has issued a launch license to SpaceX for the upcoming return to flight of its Falcon 9, although its planned launch has been delayed by at least one day.
 
FAA spokesman Hank Price said in a Jan. 6 statement that the agency had reviewed and accepted SpaceX’s investigation into its Sept. 1 pad explosion. That accident destroyed a Falcon 9 rocket being prepared for a static fire test in advance of the launch of the Amos-6 communications satellite. With the report accepted, FAA then issued the license required for the launch of the first batch of 10 Iridium Next satellites.

"The FAA accepted the investigation report on the Amos-6 mishap and has closed the investigation," Price said. "SpaceX applied for a license to launch the Iridium Next satellites from Vandenberg Air Force Base. The FAA has granted a license for that purpose
 
SpaceX announced Jan. 2 that it had completed the investigation into the pad explosion, blaming the accident on composite overwrapped pressure vessels used to store helium in the liquid oxygen tank of the rocket’s upper stage. The aluminum liner of pressure vessel buckled and liquid oxygen pooled between the liner and carbon overwrap, which led to the failure of the pressure vessel.
At the time of the announcement, SpaceX said it had submitted its report to the FAA, but that the FAA was still reviewing it. Price said Jan. 5 that the FAA was still reviewing the report and continuing to work with the company. 

The license, valid until January 2019, covers all seven planned Falcon 9 launches of Iridium spacecraft from Vandenberg Air Force Base in California. The license also authorizes SpaceX to attempt landings of the rocket’s first stage on a “droneship” in the Pacific Ocean downrange from the launch site.

 The issuance of the license comes a day after SpaceX conduced a static-fire test of the Falcon 9 on the pad at Vandenberg. “Hold-down firing of @SpaceX Falcon 9 at Vandenberg Air Force completed. All systems are go for launch next week,” SpaceX Chief Executive Elon Musk tweeted Jan. 5.

When it released the results of its investigation into the September pad explosion Jan. 2, SpaceX stated that it was planning to carry out the launch Jan. 8. An Iridium spokesman said Jan. 6 that the launch has been delayed one day to Jan. 9, at 1:22 p.m. Eastern.

Weather, however, is not promising for a launch on either Jan. 9 or the next several days, with forecasts projecting cloudy skies and intermittent rain.

 

 

WASHINGTON — An explosion on a Florida launch pad early Sept. 1 destroyed a SpaceX Falcon 9 rocket and its payload, the Amos-6 communications satellite, being prepared for an upcoming launch there.
Authorities said the explosion occurred at approximately 9:07 a.m. Eastern at Space Launch Complex 40 at Cape Canaveral Air Force Station, where SpaceX was preparing to conduct a static fire test of the Falcon 9 in advance of a scheduled Sept. 3 launch. The test, which entails briefly firing the rocket’s first stage, is a routine pre-launch procedure for Falcon 9 missions.
SpaceX Chief Executive Elon Musk, in a tweet four hours after the incident, said the explosion originated around the Falcon 9’s the upper stage liquid oxygen tank while it was being loaded in the minutes before the scheduled static fire test. He said there was no information yet on the cause of the explosion.
- See more at: http://spacenews.com/developing-explosion-rocks-spacex-falcon-9-pad-at-cape-canaveral/#sthash.yCEgK2TP.dpuf
WASHINGTON — An explosion on a Florida launch pad early Sept. 1 destroyed a SpaceX Falcon 9 rocket and its payload, the Amos-6 communications satellite, being prepared for an upcoming launch there.
Authorities said the explosion occurred at approximately 9:07 a.m. Eastern at Space Launch Complex 40 at Cape Canaveral Air Force Station, where SpaceX was preparing to conduct a static fire test of the Falcon 9 in advance of a scheduled Sept. 3 launch. The test, which entails briefly firing the rocket’s first stage, is a routine pre-launch procedure for Falcon 9 missions.
SpaceX Chief Executive Elon Musk, in a tweet four hours after the incident, said the explosion originated around the Falcon 9’s the upper stage liquid oxygen tank while it was being loaded in the minutes before the scheduled static fire test. He said there was no information yet on the cause of the explosion.
- See more at: http://spacenews.com/developing-explosion-rocks-spacex-falcon-9-pad-at-cape-canaveral/#sthash.yCEgK2TP.dpuf