Indian Space Program: News & Discussions

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ISRO Awaits Advanced Materials



Calls for national effort to make crucial components for upcoming missions
A national effort is needed to develop and produce advanced materials to drive the future space programme, Indian Space Research Organisation (ISRO) chairman K. Sivan has said.

Along with high propulsion systems for its launch vehicles, the ISRO is pursuing materials that have extraordinary properties, such as aluminium and beryllium alloys and carbon nanotubes. These are needed for the upcoming high-profile national missions such as the Human Space Programme (HSP), the Reusable Launch Vehicle (RLV), re-entering crew capsules, fuel-saving scramjet missions and the distant single-stage launchers. Locally made materials will also help to cut imports and also lower mission costs, Dr. Sivan said here.

He was delivering the 37th annual Brahm Prakash Memorial Lecture organised by the Indian Institute of Metals and the Indian Institute of Science. Brahm Prakash was a renowned metallurgist and former director of ISRO’s Vikram Sarabhai Space Centre, Thiruvananthapuram, in the 1970s.

“In recent years, ISRO has indigenised a large number of materials that are hard to get. This has reduced the import content from around 32% to 8% now. However, development of advanced materials such as carbon carbon composites and those for electronics is the immediate need of the space programme. A national effort is required in these two areas,” Dr. Sivan said.

Over the years, ISRO has localised maraging steel, many aluminium alloys, composites, chemicals, coatings and high temperature items. A hafnium-neobium has been produced to create a superalloy of columbium for advanced missions and needs to be produced on a large scale. ISRO is now looking for aluminium and beryllium alloys to make smaller structures; and carbon-carbon composites for the nose cone of the RLV; and carbon nanotubes for fuel tank systems and silica alternatives for thermal tiles. Next-generation semicryogenic launchers and electric propulsion systems of smaller future satellites need them. Industry must take it forward in an aggressive way, he said addressing metallurgists.

“Lab-level R&D can produce small quantities of special materials. We want industry to come forward to produce them in large quantities,” Dr. Sivan later told this newspaper. A carbon fibre technology developed with National Aeronaticial Labs awaits a production partner.

Material costs alone are 85% of a launch vehicle. The remaining 15% includes the propellant, technology, labour, tracking and everything else. “Materials are the heart of any space programme. Without advancements in them we cannot keep it going.”

New materials are needed to make lighter, stronger, faster and safer space vehicles of the future. They must ensure that satellites and launchers work safely and well in extreme hot and cold conditions of space; amidst high pressure and protect crews from radiation hazards. They should also protect space vehicles from the impact of micro meteorites that may hit them.

Much of ISRO’s materials research is conducted at VSSC, the rocket development centre, with other centres chipping in. A few hundred scientists work on developing metals, ceramics, materials used in electronics.

VSSC’s transfer of titanium sponge technology to Kerala Metals and Minerals Ltd is a major success story. Since 2015, it has erased ISRO's import of 200-300 tonnes each year, bringing down the material's cost and creating a surplus supply in the country.

ISRO awaits advanced materials

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Indigenisation of Copper-Chromium-Zirconium-Titanium Alloy for Cryo and Semi-Cryo engines- A Success Story

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Copper Alloy (Cu-0.5Cr-0.05Ti-0.05Zr) is an important and vital item required for cryogenic/semi-cryogenic engines for the realisation of thrust chamber inner shell and injector face plates of Cryogenic Upper Stage (CUS) engine for GSLV Mk-II, CE20 engine for GSLV Mk-III and Semi-Cryo (SC) stage. This is also required for the Steering Engines (SE) of CUS engine, Gas generator of CUS & CE20 engines, injectors, pre-burner and pyro components of SC engine.

These projects require Copper Alloy plates, rods and forgings of various dimensions. For plates, thickness requirement range from 12 mm to 18 mm and width of 850 mm. Rods and forgings of this alloy are also required with diameters ranging from 30 mm upto 300 mm.

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Indigenisation efforts were made through NFTDC, Hyderabad for CUS, CE20 and SC. Melt capacity was augmented to 1000 kg and plate rolling mill capable of 1500 mm width was established for meeting the project requirements. All required products using this alloy have been successfully realized for CUS, CE20 and Semi-Cryo projects. The hot test of the CUS engine using this copper alloy for 200 sec in the nominal and 13% uprated thrust regime was carried out at IPRC, Mahendragiri. This engine will power the cryogenic stage of GSLV Mk-II, which is scheduled to launch GSAT-7A in November this year.

Process Flow: Cast ingots from the melt furnace are made into skinned ingots weighing 375 to 400 kg. These are converted into as forged plates which gets further forged to skinned plates ready for rolling. Plates of required size are generated through hot rolling process.


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Products Realised:

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The major challenges faced in the endeavor are:

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    Optimisation of chemical composition and the melting practice to achieve the designed chemistry and mechanical properties at ambient and high temperatures.
  • Optimisation of press forging to avoid defects in UT for higher width plates leading to considerable increase in the yield.
  • Achieving fine grains by optimizing heat treatment from 9800 C for 10 min. to 7500C for 20 min.
  • Ultrasonic Trasducer (UT) – Normal beam with TR probe and Angle beam scanning with Class A acceptance criteria.
  • Bend tests on samples from plates subjected to annealing at 7500C for 20 min. followed by air cooling ensuring formability.
  • bend_tests.png
  • Benefits of the indigenization include:
  • Very cost effective compared to import.
  • Self-reliance through establishment of facilities at M/s. NFTDC, Hyderabad which is the second known processing unit globally for production of aerospace quality Cu-Cr-Zr-Ti alloy.
  • Low establishment costs
    • Refurbishment route of available facilities adopted
    • Rolling mill components designed and realized through various units within India and integrated at NFTDC
    • Existing melt furnace coils at NFTDC were modified to increase the melt capacity to 1000kg
Indigenisation of Copper-Chromium-Zirconium-Titanium Alloy for Cryo and Semi-Cryo engines- A Success Story - ISRO

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ISRO Doppler Weather Radars’ Role in the Kerala Flood Rescue Operation

During the month of August 2018, most of the districts of Kerala, mainly, Iddukki, Patthanmthitta, Ernakulam, Trichur and Palakkad received more than expected rainfall (deviation by more than 164% as per India Meteorological Department (IMD) report) from this year’s South West monsoon. In just the first 20 days of the month, Kerala has received the highest rainfall for the entire month in 87 years, with Idukki district breaking a 111-year record for the highest rainfall for the month, as per IMD’s records. This rainfall has brought flood in several parts of the state. The state has faced this kind of disaster after nearly 123 years. More than 370 people lost their lives; thousands are stranded and huge property loss occurred.

ISRO has monitored the whole event through its various satellites which helped a lot in the prediction and safety measures. ISRO not only extended support through its space based sensors, but ground based sensors as well. Two of its radars, one C-Band Polarimetric Doppler Weather Radar (DWR) at TERLS, Vikram Sarabhai Space Centre (VSSC), Thiruvanthapuram and one S-Band DWR at Kochi were continuously monitoring the weather on 24X7 basis up to 500 Km radius. These radars were installed by Radar Development Area (RDA) of ISRO Telemetry Tracking and Command Network (ISTRAC), Bangalore. The data gets transferred seamlessly to IMD and MOSDAC (Meteorological and Oceanographic Data Archival Centre), Space Application Centre (SAC) immediately after each volume scan for further data analysis and centralised weather monitoring. The data is made available in near real time for public through the MOSDAC and IMD websites. These radars helped a lot in long range weather surveillance, forecast and nowcast of the weather and rainfall activity in Kerala. National Disaster Management Authority and Kerala state Disaster Management authority were continuously monitoring the data received by the radar and images were continuously updated in the IMD website for their decision making on various activities.

The DWR measures radar reflectivity, mean radial velocity, and velocity spread to infer many aspects of hydrometeors. In addition to this, the Polarimetric DWR has the capability to measure additional four parameters, such as Differential Reflectivity, Correlation Coefficient, Linear Depolarization Ratio and Specific Differential Phase. These seven parameters provide accurate rainfall rate along with hydrometeor classification, such as type of rain by obtaining information of drop shape and size. Thus the DWR system provides quantitative information in digital form, the intensity and mean velocity of cyclones along with rain fall rate and accumulation. It improves the understanding and forecasting of thunderstorm, hailstorms, tidal wave height, wind turbulence and shear.The radar completes one volume scan in 11 minutes, comprising of 360 degree azimuth scan for 10 different elevation angles ranging from 0.5 to 21 degrees.

One of the products derived from the observation from the DWR is MAXZ, which shows the intensity of cloud system across the region of observation and height of the cloud system (in adjacent panels) giving an indication as to what could be the probable intensity of rain expected in and around the region. The DWR covers a distance of 250 km (up to 500 km for S -Band) with a spatial resolution of 150 or 300 m. Using these DWR products, weather forecast, nowcast and precipitation accumulation were derived in addition to other instruments’ data which helped the civic body in advance for evacuation and rescue of many lives and property.

Both C-Band and S-Band radar is a ground based monostatic pulse Doppler radars.

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S-Band DWR at Kochi C-Band DWR at VSSC, Thiruvanathapuram

Some of the rainfall events captured by these DWRs during the floods are shown below.

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Rainfall captured by C-DWR:Top two is MAX(Z) product

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Rainfall captured by C-DWR: Plan Position Indicator Velocity(PPIV) and Surface Rainfall Intensity (SRI) product

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ISRO Doppler Weather Radars’ Role in the Kerala Flood Rescue Operation - ISRO

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AstroSat Picture of the Month Aug, 2018
X-raying a supernova

This month, for the first time, we bring you an X-ray image from AstroSat. We feature the image of the Tycho Supernova remnant or SN 1572, imaged by the Soft X-ray Telescope (SXT). Located in the constellation Cassiopeia, at a distance of about 10000 light years, SN 1572 is a historic object. It is one of the 8 supernova explosions that were seen with the naked eye. This new star appeared in the sky during early November in 1572, and was observed by many astronomers across Europe and China. It is named after Tycho Brahe since he was the one who studied it in great detail till it faded away in 1574. He published his observations in his work 'Concerning the Star, new and never before seen in the life or memory of anyone', which included a star chart too. At its peak, it rivalled Venus at its brightest, confounded astronomers at that time, and changed their perspective of an unchanging sky.

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X-ray image of the Tycho Supernova Remnant in the 0.8-2.0 nanometres (0.6-1.6 keV) range, made by the Soft X-ray Telescope on board AstroSat.

The supernova remnant is roughly 8 arcminutes big (3.7 times smaller than the full moon in the sky) and the emission is brighter near the edge of the expanding supernova remnant.

Pic Credit: Kulinder Pal Singh (IISER Mohali) and the entire SXT Instrument and POC teams at TIFR, University of Leicester, and IUCAA

We now know, from historic data, that this was a Type 1a supernova. Sometimes, a normal star and a white dwarf (which is a very compact object that is the end stage of stars like our Sun) orbit each other. Material from the normal star is pulled on to the white dwarf due to gravity, making it heavier. When the mass of the white dwarf exceeds the famous Chandrasekhar Limit, it explodes, leading to a Type 1a supernova, like our SN 1572. What we see today is what is left of this explosion. The debris is expanding outwards like a sphere, with an edge which is the shock front. This supernova remnant, discovered first in radio wavelengths, and then in optical and X-rays and infrared, is a beautiful object indeed.

X-rays can penetrate metal easily. Hence, the cleverly designed Soft X-ray Telescope uses 320 concentric gold coated mirrors and a very cold CCD to form images in the X-ray. The image of the Tycho Supernova remnant shown here is made from photons with wavelengths between 0.8 to 2.0 nanometres (0.6-1.6 keV). Most of this emission, coming from the limb of the expanding shell, is due to emission from Iron atoms where electrons jump from higher levels to the 2nd level.

The full article can be downloaded from SXT: early results

AstroSat Picture of the Month Aug, 2018 - ISRO
 
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India, France plan satellites for maritime surveillance: French space agency chief

India and France have planned eight-10 satellites as part of a “constellation” for maritime surveillance, French space agency CNES chief Jean-Yves Le Gall has said.

This will be India's largest space cooperation with any country, officials said.

They added that the launch of eight-10 maritime surveillance satellites will focus on the Indian Ocean, a region that has been witnessing increasing Chinese presence.

France will also share its expertise with the Indian Space Research Organisation (ISRO) on inter-planetary missions to Mars and Venus, the Indian space agency's two major missions, Gall said.

"We started (talks) on constellation of new satellites for maritime awareness. Of course, it will take time," Gall told PTI in an interaction.

Asked how many satellites will be part of the project, he said, "It would be between eight-10."

The purpose of the constellation is monitoring sea traffic management, a CNES official said, adding that it would take less than five years to launch the satellites.

In March this year, India and France unveiled a joint vision for space, resolving to strengthen cooperation between ISRO and CNES.

"ISRO and CNES would work together for design and development of joint products and techniques, including those involving Automatic Identification System, to monitor and protect assets in land and sea. In particular, both sides will pursue the study of a constellation of satellites for maritime surveillance," the joint vision statement said.

Several crucial sea lanes of communications pass through the Indian Ocean, a region critical to the strategic interests of India and France.

While the Indian Ocean region is the prime focus for New Delhi, Paris has its territories spread across the Indian Ocean, the Pacific Ocean and the Atlantic Ocean, officials said.

The robust space cooperation between India and France goes back six decades.

Last week, the two countries signed an agreement to share expertise on ISRO's human mission programme Gaganyaan. The space agencies of the two countries have also been working on climate monitoring on the joint missions Megha-Tropiques (launched in 2011) and Saral-Altika (launched in 2013).

They are also working on the Trishna satellite for land Infrared monitoring and the Oceansat3-Argos mission. Discussing collaboration for the mission to Venus and Mars and France's expertise on the matter, Mathieu Weiss, the managing director of CNES' India liaison office, explained, "The eyes and scientific heart of Curiosity Rover (NASA) on Mars were developed by us. France and Russia have jointly worked for the Venus mission in the past. In both the inter-planetary missions, the French scientific community is very strong and among best in the world," Weiss told PTI.

In a media briefing at Paris on Friday, Gall said CNES is currently working with Japan Aerospace Exploration Agency (JAXA) and German space agency DLR on Hayabusa 2/ MASCOT, a mission to asteroid Ryugu. CNES has also scheduled Mission BepiColombo to Mercury.

Read more at:
//economictimes.indiatimes.com/articleshow/65828365.cms?utm_source=contentofinterest&utm_medium=text&utm_campaign=cppst
 
44th PSLV launch puts 2 UK satellites into orbit


The Indian Space Research Organisation’s (Isro) workhorse, the Polar Satellite Launch Vehicle (PSLV) in its 44th flight put into orbit two UK earth observation satellites in a textbook launch.

Both the satellites together weighed about 889 kg, and the commercial launch was carried out under an arrangement between Surrey Satellite Technologies Limited (SSTL) and Isro’s commercial arm Antrix Corporation Limited.

NovaSAR is an S-Band Synthetic Aperture Radar (SAR) satellite intended for forest mapping, land use and ice cover monitoring, flood and disaster monitoring. Its SAR payload has a dedicated maritime mode designed with a very wide swath area (400-km) to enable the monitoring of the marine environment, and will provide direct radar ship detection information simultaneously with AIS ship tracking data to assist with the identification and tracking of sea-going vessels.

S1-4 is a high resolution Optical Earth Observation Satellite, used for surveying resources, environment monitoring, urban management and for the disaster monitoring.

Just hours before the launch, Vikram Sarabhai Space Centre (VSCC) director S Somanath had said: “When I joined Isro in 1985, the PSLV was still on paper, and the only rocket we had was SLV-3, the ASLV was struggling with people ridiculing us and asking when it will reach space. It had earned the moniker of Always Sea Launch Vehicle (ASLV) as it kept failing and landing in water. To see PSLV grow from an idea and to become Isro’s workhorse is a great feeling.”

Somanath had told TOI that the rare night launch was at the request of the customer — SSTL — as the satellites needed specific imaging and illumination requirements.

The PSLV-C42, was only the third launch of PSLV after the rare failure it encountered in August last year due to problems in the heat shield. It took off at 10.08pm, the first stage separated about two minutes after that, while the fourth state separated nearly 17 minutes after the take off. The satellites separated 17.44 minutes after the launch before being placed in the desired Sun Synchronous orbit, about 583 km away.

This is Isro’s first dedicated commercial launch in several months, and Antrix hopes to increase the frequency of such missions in the future, with the help from industry. While the space agency’s commercial arm does not give out mission-specific earnings, in the three years between April 2015 and March 2018, it earned Rs 5,600 crore.

Of this only 10% to 20% came from launch services like Sunday’s, while the most was earned from marketing products and services.

Isro presently has 84 major clients using its communication services, including big service providers like Reliance and television groups like Sun Network. And, in the said period, Isro launched 99 satellites — 69 of which were foreign satellites — including several student and university satellites.Isro chairman K Sivan had told TOI earlier that the agency will, in the near future, be able to spare more PSLVs for Antrix. However, this will depend on how reliable the GSLV class of vehicles becomes for Isro.
 
6 months, 18 missions: ISRO sets new goals
On September 16, ISRO (Indian Space Research Organization) launched PSLV C42 in space, putting two UK satellites in orbit. As the current Prime Minister Narendra Modi announced the feat as the demonstration of India's prowess in the competitive space business, ISRO is all set to take it up a notch.

Indian Space Research Organization has made plans to launch 18 missions in the next six months.

ISRO to launch 18 missions within six months
The Indian Space Research Organisation (ISRO) on Sunday night (September 16, 2018) successfully launched NovaSAR and S1-4 earth observation satellites of the UK-based Surrey Satellite Technologies Ltd.

And now in a press release, ISRO Chairman K Sivan said, "We are going to have 18 missions in the next six months, virtually one launch every two weeks."

According to senior scientists, some of the planned launches include GSAT-11, Chandrayaan-2 moon mission and GSLV-MkIII-D2 missions, as reported by PTI.

GSAT-11
GSAT-11 is a multi-beam communication satellite, which is expected to be launched from French Guiana.

Chandrayaan-2
Chandrayaan-2 is the second mission to the moon in which ISRO will launch the lander carrying a six-wheel rover.

ISRO had successfully launched Chandrayaan-1 in October 2008 which orbited the moon at a height of 100 km from the lunar surface for chemical, mineralogical and photo-geologic mapping of the moon.

In Chandrayaan-2, the scientists will make the lander soft-land on the moon and deploy the rover to study its surface.

GSLV-MKIII-D2
The GSLV-MkIII-D2 mission would, for the first time, carry communication payloads. It is targeted at Village Resource Centres in rural areas to bridge the digital divide.
6 months, 18 missions: ISRO sets new goals
 
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Russia & India sign space memorandum

A deal for space cooperation signed on Friday between Russia and India concerns a manned space program and the development of cooperation in the sphere of navigation systems, Roscosmos head Dmitry Rogozin told journalists.

The contract is the first of several expected to be signed between Russia and India during President Vladimir Putin’s two-day visit to India.

An Indian monitoring station will be built near the Russian city of Novosibirsk in Siberia, Rogozin said, without providing any further details about the project.

New Delhi also asked Moscow for help with its own space launch project in 2022, Russian Deputy Prime Minister Yury Borisov said on Friday. “The Indian side has approached us with a request on the implementation of its own project ensuring the launch of an Indian astronaut to space in 2022,” Borisov told reporters.

Reports saying that Russia may take an Indian astronaut to space earlier appeared in Indian media. “The first Indian astronaut was sent to space on a Russian Ship. They are likely to collaborate with us… sending a manned space ship,” sources told One India new portal. So far, Rakesh Sharma remains the only Indian to travel to space. He flew aboard the Soviet Soyuz rocket to the Salyut orbital station in 1984.
 
Space Science Missions Roadmap: 2008 to 2028

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2008: Chandrayaan-1
2013: Mars Orbiter Mission
2015: Astrosat
Jan 2019: Chandrayaan-2
Nov 2019: XpoSat
Jan 2020: Aditya-L1
2022: Mars Orbiter-2
2023: Venus Mission
2024: Lunar Polar Exploration
2028: Exoplanet mission (?)

...so how & what exactly are they planning for Exoworld missions? Something like Starshot?
 
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ISRO successfully tests Cryogenic Engine (CE-20) for GSLV Mk-III / Chandrayaan-2 Mission

The upper stage of GSLV MK-III vehicle is powered by Cryogenic Engine (CE)-20 which develops a nominal thrust of 186.36 kN with a specific impulse of 442 seconds in vacuum. The engine operates on gas generator cycle using LOX / LH2 propellants combination. The major subsystems of the engine are thrust chamber, gas generator, LOX and LH2 turbo pumps, igniters, thrust & mixture ratio control systems, Start-up system, control components and pyro valves. The fifth hardware of CE-20 integrated engine designated as E6 is earmarked for GSLV Mk-III M1-Chandrayaan 2 mission.

The flight acceptance hot test of E6 engine was successfully tested for 25 seconds at High Altitude Test facility, ISRO Propulsion Complex (IPRC), Mahendragiri on October 11, 2018. The test demonstrated steady state operation of engine. The performance of all engine subsystems were observed to be normal during the hot test.

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ISRO successfully tests Cryogenic Engine (CE-20) for GSLV Mk-III / Chandrayaan-2 Mission - ISRO
 
Space Science Missions Roadmap: 2008 to 2028

View attachment 3366

2008: Chandrayaan-1
2013: Mars Orbiter Mission
2015: Astrosat
Jan 2019: Chandrayaan-2
Nov 2019: XpoSat
Jan 2020: Aditya-L1
2022: Mars Orbiter-2
2023: Venus Mission
2024: Lunar Polar Exploration
2028: Exoplanet mission (?)

...so how & what exactly are they planning for Exoworld missions? Something like Starshot?
star shot?
 
ISRO-NASA Project Finds Black Hole that Spins Near Max Possible Rate
The findings are significant, said researchers, because so far, high spin rates of only about five black holes have been quantified accurately

The Indian Space Research Organisation’s (Isro) AstroSat, India’s first dedicated astronomy satellite, in coordination with The National Aeronautics and Space Administration’s (Nasa) Chandra X-ray Observatory has found that a black hole in the binary stellar system 4U 1630−47 spins at a rate that is close to the maximum possible rate.

Researchers said studying black holes with high spin rates is important as it paves the way to test the fundamental laws and theories of the universe, one of which is Albert Einstein’s theory of gravity – general relativity. The significance? Black holes generate the strongest gravitational force in the universe.

A black hole, which is an exotic but a very simple astronomical object, is created when a massive star dies and the matter gets squeezed into a tiny space under a heavy force of gravity, trapping in the light.

Using the X-ray data from AstroSat and Chandra, an international team of astronomers from multiple institutions led by the Tata Institute of Fundamental Research (TIFR) found that the spin rate of the black hole was about 0.9. The spin rate is a dimensionless unit ranging between 0 and 1.

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The study comprising an international team of astronomers from multiple institutions and led by TIFR has been accepted for publication in The Astrophysical Journal, a peer-reviewed scientific journal of astrophysics and astronomy.

The findings are significant, said researchers, because so far, high spin rates of only about five black holes have been quantified accurately. Measurement by AstroSat-Chandra is one of them. This is one of the 20 black holes that have been discovered in our galaxy. Each of them about 10 times the mass of the Sun.

“As black holes get created, mass and spin rate are two properties that characterise them. Mass can be measured more easily as it has a long-range effect because of gravity as the black hole gets created,” said Sudip Bhattacharyya of TIFR, and principal investigator of Astrosat’s Soft X-ray Telescope (SXT).

“However, measurements especially of the spin rate are very difficult to make, and can be done only by high-quality X-ray observations in the correct state of the binary stellar system, in which the black hole is a gobbling matter from its companion star”, said the lead author Mayukh Pahari. Pahari started this work at TIFR, before joining a Royal Society-SERB Newton International Postdoctoral Fellow position at the University of Southampton in UK.

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It was the indigenously built SXT and Large Area X-ray Proportional Counter (LAXPC) instruments on-board the Astrosat that first observed the black hole in a favourable state so as to be able to interpret the X-ray at the end of 2016. Following this, the Astrosat team requested director of Chandra X-ray Observatory to observe the same black hole. Having independently measured the spin rates of the black hole, the results from Astrosat were consistent with data from Chandra satellite, making the findings robust. Bhattacharyya said, “This is the first cooperation between India and the US using AstroSat and Chandra for black hole studies. Since it was very successful, other collaborations will also now be possible.”

Isro-Nasa project finds black hole that spins near max possible rate

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AstroSat Picture of the month - Oct 2018
Ultraviolet wings of the Butterfly Nebula

This month, APOM brings to you the ultraviolet view of one of the most spectacular objects in the sky, NGC 6302. Located nearly 3,800 light years away in the constellation Scorpius, NGC 6302 is a planetary nebula, whose shape is strikingly similar to the wings of a butterfly, hence aptly named as the Butterfly Nebula. This is the second planetary nebula that we bring forth to you, the first being NGC 40, covered in the APOM issue of December 2017.

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Planetary nebulae are beautiful structures formed during the last few stages of the lives of stars like the Sun or a few times heavier. As the stars burn up all the hydrogen or helium fuel, they increase in size and become redder in colour, and are known as giant stars. As the giant star passes through few more stages, it continually sheds its outer layers revealing an inner hot core called the white dwarf. The white dwarf heats up the spewed-out gas which shines in the form of planetary nebula. Many of these planetary nebulae have strikingly symmetric shapes that need not be spherical and it has been suggested that this could be due to the various physical processes occurring in and around the star when it hurls out the gas from the outer layers. These nebulae are named planetary because when astronomers first observed them, they thought that these resembled planets. We now know that this is not the case, although the name has lingered.

Prof Kameshwar Rao, from the Indian Institute of Astrophysics (IIA), and his team have been investigating planetary nebulae in the ultraviolet light. They have imaged the Butterfly Nebula through the far and near-ultraviolet filters of the Ultraviolet Imaging Telescope (UVIT) of AstroSat. Using these images, they have discovered that gas which is bright in the far-ultraviolet extends beyond the known wings of the butterfly out to 5.5 light years from the centre, nearly three times of what is seen in the optical. The reddish coloured figure on the right is the far ultra-violet image of the Butterfly Nebula. The blue image is a cartoon that represents the full extent of the far-ultraviolet emission. These researchers argue that the extended far-ultraviolet light is due to cold hydrogen molecules in the gas present in the outer parts of the nebula which are excited by the central star. They suspect that these far-ultraviolet structures of the planetary nebula point to the possible presence of two central stars in a binary system that are gravitationally bound. The results have been published in the journal Astronomy & Astrophysics and the paper can be read here.

AstroSat Picture of the month - Oct 2018 - ISRO

https://arxiv.org/pdf/1810.02217.pdf

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Megha-Tropiques Successfully Completes Seven Years in Orbit

Megha-Tropiques satellite was built by ISRO and CNES as a Joint Venture. The satellite is meant to study water cycle and energy exchanges in tropical region for weather prediction and climate research. Megha-Tropiques was launched on 12th October 2011 from SDSC, Shriharikota. The satellite has successfully completed seven years of on-orbit observations with four Science instruments on board, namely, MADRAS, SAPHIR, SCARAB and ROSA. Megha-Tropiques provides scientific data on the contribution of the water cycle to the tropical atmosphere, with information on condensed water in clouds, water vapour in the atmosphere, precipitation, and evaporation.

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All science instruments provided valuable data to the user community. Many national and international papers have been generated by utilizing these datas. The Global response for the Announcement of Opportunities for science data utilisation of the instruments on-board Megha-Tropiques has been good and is increasing with time.

Megha-Tropiques Successfully Completes Seven Years in Orbit - ISRO

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@Picdelamirand-oil @Bon Plan :cool:

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CHANDRAYAAN-2 LANDER ACTUATOR PERFORMANCE TEST (LAPT PHASE-2)

The Lander Actuator Performance Test (LAPT) is one of the crucial tests required to be demonstrated for a successful soft and safe landing of Vikram (Chandrayaan-2 Lander). To carry out this test, an LAPT module which is a scaled down version of Vikram with all the required hardware was realised for testing in Earth environment. The reason for the scaling down is to compensate the effect of Earth’s gravity as compared to Moon’s gravity and to match the thrust generation of sea level Liquid Engines as compared to flight engines which will operate in vacuum environment. The module was tethered to a crane hook for conducting the test. To carry out this test, a special test facility was erected at ISRO Propulsion Complex, Mahendragiri.

Chandrayaan-2.jpg

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The objective of the test was to assess the closed loop integrated performance of Sensors, Actuators and Navigation, Guidance & Control (NGC) and guidance algorithms below 100 m height. Three tests have been conceived as part of LAPT Phase-2 activities to demonstrate these objectives. First test was conducted to demonstrate Vertical Descent while second Test was conducted to demonstrate Hovering.

The third and final test was successfully conducted to demonstrate re-targeting in a Parabolic Trajectory, on 25th Oct 2018 at ISRO Propulsion Complex, Mahendragiri. This test demonstrated the capability of the NGC system of Vikram to meet the mission requirement of safe, soft and precise landing on the lunar surface by steering the module horizontally as well as vertically down to a pre-defined target. With this, all the tests have been completed successfully. This is a major milestone accomplished in Chandrayaan-2 Lander.

CHANDRAYAAN-2 LANDER ACTUATOR PERFORMANCE TEST (LAPT PHASE-2) - ISRO