NASA & World Space Exploration...News, Views, Photos & videos

Jeff Head

General
Registered Member
this mars image is the best full disc image you can get anywhere
India is doing great with its mission to Mars...and that is indeed an excellent photo.

As to whether it is the best Full Disc image of Mars...well, let's just say that there are a lot of full disc images out there that are equally good. The US and others (like the EU) have been producing photos for a long time. As an example, here are a few from
Please, Log in or Register to view URLs content!
Please, Log in or Register to view URLs content!



16012215472_f70a552889_b.jpg

EU's Rosetta in 2007

16010956521_0cb129c1a5_b.jpg

NASA's Global Surveyor in 1999

16010956191_a9901fd131_b.jpg

Hubble Telescope in 1997

15393583673_79ba1ffff6_b.jpg

NASA lander in 1980

16013063455_4fd2c766d7_b.jpg

NASA Lander in 1976

Those are just a few of the many going back over 38 years now.

A REALLY neat thing is landing on the planet and then roving around on it for 2-3 years as various NASA landers have done. Curiosity has a site where you can track its movements on the planet and get high res images from what is is seeing.

Here a Map of its movements from it's day 685 through day 817 on Mars:


15393438973_9aeb6ddc81_b.jpg


...and here are some examples of the stunning photos it has been producing.


13884525301_0f1540ab32_b.jpg


13907641955_cf4f34d599_b.jpg


13884524841_46d7f05eec_b.jpg


13884525221_3bed871589_b.jpg


See
Please, Log in or Register to view URLs content!
for more pictures.

As I say...one day we will have pictures of manned expeditions to Mars and human's taking those pictures in person. Exciting stuff.
 
Last edited:

aksha

Captain
B4jZN5VCMAAHi7v.jpg:large

ISRO's LVM 3 X flight planned on Dec 18 will carry active Solid boosters, Liquid core stage and a passive Cryo stage .flight will carry the CARE (Crew-module Atmospheric Re-entry Experiment) Module, to be recovered from the Bay of Bengal.
hopefully things will go all right

the rocket payload and range is inferior to to other similar rockets around the world,but it will serve us well.
after all we did a great work with the PSLV despite many calling it an outdated one.
 

aksha

Captain
NASA's Curiosity Rover Finds Clues to How Water Helped Shape Martian Landscape

B1zBJfz.jpg

Observations by NASA's Curiosity Rover indicate Mars' Mount Sharp was built by sediments deposited in a large lake bed over tens of millions of years.

This interpretation of Curiosity's finds in Gale Crater suggests ancient Mars maintained a climate that could have produced long-lasting lakes at many locations on the Red Planet.

"If our hypothesis for Mount Sharp holds up, it challenges the notion that warm and wet conditions were transient, local, or only underground on Mars," said Ashwin Vasavada, Curiosity deputy project scientist at NASA's Jet Propulsion Laboratory in Pasadena, California. "A more radical explanation is that Mars' ancient, thicker atmosphere raised temperatures above freezing globally, but so far we don't know how the atmosphere did that."

Why this layered mountain sits in a crater has been a challenging question for researchers. Mount Sharp stands about 3 miles (5 kilometers) tall, its lower flanks exposing hundreds of rock layers. The rock layers - alternating between lake, river and wind deposits -- bear witness to the repeated filling and evaporation of a Martian lake much larger and longer-lasting than any previously examined close-up.

"We are making headway in solving the mystery of Mount Sharp," said Curiosity Project Scientist John Grotzinger of the California Institute of Technology in Pasadena. "Where there's now a mountain, there may have once been a series of lakes."

Curiosity currently is investigating the lowest sedimentary layers of Mount Sharp, a section of rock 500 feet (150 meters) high, dubbed the Murray formation. Rivers carried sand and silt to the lake, depositing the sediments at the mouth of the river to form deltas similar to those found at river mouths on Earth. This cycle occurred over and over again.

"The great thing about a lake that occurs repeatedly, over and over, is that each time it comes back it is another experiment to tell you how the environment works," Grotzinger said. "As Curiosity climbs higher on Mount Sharp, we will have a series of experiments to show patterns in how the atmosphere and the water and the sediments interact. We may see how the chemistry changed in the lakes over time. This is a hypothesis supported by what we have observed so far, providing a framework for testing in the coming year."

After the crater filled to a height of at least a few hundred yards, or meters, and the sediments hardened into rock, the accumulated layers of sediment were sculpted over time into a mountainous shape by wind erosion that carved away the material between the crater perimeter and what is now the edge of the mountain.

On the 5-mile (8-kilometer) journey from Curiosity's 2012 landing site to its current work site at the base of Mount Sharp, the rover uncovered clues about the changing shape of the crater floor during the era of lakes.

"We found sedimentary rocks suggestive of small, ancient deltas stacked on top of one another," said Curiosity science team member Sanjeev Gupta of Imperial College in London. "Curiosity crossed a boundary from an environment dominated by rivers to an environment dominated by lakes."

Despite earlier evidence from several Mars missions that pointed to wet environments on ancient Mars, modeling of the ancient climate has yet to identify the conditions that could have produced long periods warm enough for stable water on the surface.

NASA's Mars Science Laboratory Project uses Curiosity to assess ancient, potentially habitable environments and the significant changes the Martian environment has experienced over millions of years. This project is one element of NASA's ongoing Mars research and preparation for a human mission to the planet in the 2030s.

"Knowledge we're gaining about Mars' environmental evolution by deciphering how Mount Sharp formed will also help guide plans for future missions to seek signs of Martian life," said Michael Meyer, lead scientist for NASA's Mars Exploration Program at the agency's headquarters in Washington.

Please, Log in or Register to view URLs content!
 

Miragedriver

Brigadier
Some scientists think we'll find signs of aliens within our lifetimes. Here's how.

lz0mWwE.jpg


(VOX) Finding extraterrestrial life is the essence of science fiction. But it's not so far-fetched to predict that we might find evidence of life on a distant planet within a generation.
"With new telescopes coming online within the next five or ten years, we'll really have a chance to figure out whether we're alone in the universe," says Lisa Kaltenegger, an astronomer and director of Cornell's new Institute for Pale Blue Dots, which will search for habitable planets. "For the first time in human history, we might have the capability to do this."
new telescopes could spot distant planets that have signs of life

Over the past decade, researchers have found thousands of distant planets — which they call exoplanets. Unfortunately, most of them so far have been huge, gaseous planets (akin to Jupiter or Saturn) that are easier to spot, but unlikely to contain life as we know it.

But that's all about to change. New telescopes and increasingly sophisticated analyses will soon allow us to detect rocky, Earth-sized planets and maybe even detect atmospheric gases that indicate the presence of life. Here's a step-by-step guide to how scientists plan to search for evidence of extraterrestrials

1) Find a star
PkC6BjH.jpg


This is the sun. (NASA/SDO)
Any extraterrestrial life is likely to need energy, which means that it is most likely to evolve on a planet bathed in light from a nearby star. So the first step for finding an inhabited exoplanet is locating suitable stars. (There are some planets that drift through space and don't actually orbit any stars, but those seem far less promising.)

This step is the easiest: We've already located pretty much all the stars that are close enough to us that we might be able to spot an orbiting planet and analyze its atmosphere. Scientists generally believe that main sequence stars — the 90 percent of stars in the universe that, like our sun, release energy by converting hydrogen to helium — are most likely to give rise to life.

2) Find a planet

ooflQEe.jpg


An illustration of Kepler-20e, a planet that's roughly Earth-sized, but is likely way too hot for life. (NASA/Ames/JPL-Caltech)
We've already found thousands of exoplanets (and counting), mostly using NASA's Kepler space telescope and something called the transit method.

Here's how the method works: Imagine staring at a star far away. If there is a planet orbiting that star, it might occasionally pass between us and the star, briefly blocking it from view. Scientists can't actually see the planets doing this blocking, but they can indirectly detect their presence.

"We measure the brightness of a star, and when a planet passes in front of it, it blocks out some of the starlight for a period of a few hours," Thomas Barclay, an exoplanet researcher, told me in April. If scientists observe a star dimming by a consistent amount on a predictable schedule, they can infer the size of an exoplanet that's occasionally blocking some of the light.

mnWwZSg.gif

A diagram shows how the transit method helped detect five planets in the star system Kepler-186. (Sean Raymond)
There are a few other methods for detecting exoplanets, but the transit method is the most straightforward — and it has led to the most discoveries to date.

3) Find the right kind of planet
Scientists are still working on this step. For the most part, the planets we've found so far are too big, too gaseous, or too hot to be capable of supporting life. That's because bigger, gaseous planets are easier to detect — as are planets that are relatively close to their stars (and thus much hotter).

So we still have to find more suitable planets. Based on what we know about life on Earth, we'd expect life to be more likely to evolve on a rocky planet that orbits within its star's habitable zone — an area where there's enough warmth for liquid water, but not too much heat. (It's possible that a planet even further off than this could evolve life, perhaps due to a heat-trapping layer of ice a la Europa, but that ice would likely make all signs of life invisible to us anyway.)
Scientists have currently spotted about a dozen planets that are slightly bigger than Earth and may lie in their stars' habitable zones. The catch is that they're still too far away for us to be able to analyze their atmospheres to look for signs of life. That's because the Kepler telescope wasn't optimized to search for closer planets — it was built to observe a relatively distant portion of the Milky Way for an extended period of time.

rrvxGoN.jpg

The good news is that the Transiting Exoplanet Survey Satellite (TESS), which will be launched in 2017, should allow us to spot rocky, Earth-sized planets that are much closer to us


Kky97FG.png


4) Analyze the planet's atmosphere
Most exoplanets are probably way too far off for us to ever visit — even with uncrewed probes. So the best way to learn more about them is by analyzing the light spectrums that pass through their atmospheres, indicating the gases that are present.

So far, we've been able to directly analyze the spectrum of light passing through the atmospheres of a dozen or so exoplanets. However, they've all been large, gaseous planets with thicker atmospheres.
This search, too, will soon improve. The James Webb Space Telescope, scheduled to launch in 2018, will help us analyze the atmospheres of smaller, Earth-like planets that have already been spotted by TESS. The European Extremely Large Telescope, a ground-based telescope to be built in Chile in 2024, may also be used for this purpose.
Additionally, a proposed solar shade called the New Worlds Mission could enhance the capabilities of Webb or other future space telescopes. "It would go in space and work in tandem with a telescope to block out the light from a particular star," says Sara Seager, an MIT exoplanet researcher involved in the mission. This would allow the telescope to directly see a relatively faint planet next to that star, and potentially analyze its atmosphere.

FutCdxJ.gif

An illustration of the star shade, blocking out starlight so faint planets can be more easily seen by a telescope. (NASA/JPL-CalTech)

5) Search for biosignatures
The reason we'd want to analyze atmospheres is to look for biosignatures — gases that could be signs of alien life. "We can't go to these planets," Kaltenegger says. "So we're trying to figure out what a planet that has life might look like from far away, in ways that would be detectable by our telescopes."

At the moment, we only know of one planet with life — Earth — so scientists are using that as a model to determine what gases might support life. Kaltenegger and colleagues, for instance, have used our knowledge of Earth's history to generate what they call an alien ID chart — a series of snapshots of Earth's atmospheric composition over the last few billion years, as it's evolved due to the presence of life. There are some rare gases that are only produced by life forms

Meanwhile, other researchers are modeling how various life forms might alter the atmospheres of planets with geologic compositions that differ from Earth's. As far as we know, there are some gases (like oxygen and methane) that are abundantly produced by life, but can also be produced by geologic processes. On the other hand, there are some rare gases (like dimethyl sulfide) that are produced only by life forms — as far as we know — but in much smaller quantities.
This theoretical work, Seager says, is essential, because once all the telescopes are launched, our time with them may be limited. (The Webb telescope, for instance, also needs to be used for all sorts of observations beyond exoplanet analysis, and is only designed to last for a minimum of five years.) So having an idea of what to look for ahead of time is key. "We want to be able to understand the atmospheres of planets far away, and if any gases in those atmospheres don't belong and could be attributable to life," she says.

The big question: Will we actually find alien life?

In a sense, you can look at this question as a math problem (just like Frank Drake did years ago in creating his famous equation that attempted to estimate the likelihood of finding intelligent alien life).

There are an estimated 100 billion stars in the Milky Way, and recent research has revealed that virtually every one of them is orbited by at least one planet. What's more, it's thought that roughly 22 percent of these stars are orbited by a rocky, roughly Earth-sized planet in the habitable zone. The number of stars in our neighborhood — within the range of our next-generation telescopes — means that we should be able to spot many of the coming decades, and analyze its atmosphere. There's one unknown variable: how prone life is to forming

After that, however, there's one big unknown variable: how prone life is to forming. It took about a billion years after the formation of Earth for life to first evolve, but after that it filled every niche and crevice on this planet's surface with remarkable speed. "We know life adapts really well to all kinds of conditions," Kaltenegger says. "The question is whether it needs very specific conditions to start."

There's also a caveat to consider: even if we spotted a candidate planet with what seemed to be a biosignature, it'd be extremely hard to know for sure that it resulted from life — both because we really don't know much about exoplanet geologies, and because alien life forms could be hugely different from any life we've ever seen on Earth.
And, even if we spotted a definite biosignature, we'd have no way of knowing what sort of life form produced it. It seems most likely that it'd be a microbe (for about half of Earth's history, after all, the only life forms were single-celled organisms), but it could be something more complex and we really wouldn't know.

So will we actually find aliens? Seager, Kaltenegger, and other scientists involved in the search are hopeful.
"I believe that in our lifetime, we will be able to take children to a dark sky, point to a star, and say 'that star has a planet with signs of life in its atmosphere.'" Seager said during a recent TEDx Talk, below, on her research

[video=youtube;NnM4SaGc8R0]https://www.youtube.com/watch?v=NnM4SaGc8R0&feature=player_embedded[/video]



I will now get back to bottling my Malbec
 

Miragedriver

Brigadier
mQxN5FC.jpg

The easily recognisable boot-shape of Italy, with Sicily at its toe, spread across this panorama taken by an astronaut aboard the International Space Station (ISS). On a clear night looking east, the pattern of night lights shows populations concentrated mainly along the coastlines, but also in the Po River Valley of northern Italy (L). Some of the brightest clusters of lights are Rome and nearby Naples, with island cities of Cagliari on Sardinia and Catania on Sicily. The small, dark, circular patch dangerously close to Catania marks the unpopulated slopes of the active volcano Etna. The island of Malta appears at the lower right. The airglow line is vivid in this night shot.
Picture: Nasa/AFP/Getty


I will now get back to bottling my Malbec
 

aksha

Captain
Please, Log in or Register to view URLs content!


Please, Log in or Register to view URLs content!



Please, Log in or Register to view URLs content!



India debuts GSLV Mk.III with prototype crew capsule
Please, Log in or Register to view URLs content!

The Indian Space Research Organisation has launched the first test flight of its newest rocket – the GSLV Mk.III – on Thursday, conducting a suborbital flight that also demonstrated a prototype crew capsule (CARE) for India’s proposed manned missions. Liftoff from the Satish Dhawan Space Centre occurred at 09:30 local time (04:00 UTC).

ISRO Launch:

India’s new rocket, which the Indian Space Research Organisation (ISRO) refers to by the names GSLV Mk.III and LVM3, is a completely new vehicle marking the third generation for India’s orbital launch systems.

The two-stage rocket is designed to place around 10 tonnes (9.8 Imperial tons, 11 US tons) of payload into low earth orbit or four tonnes (3.9 Imperial tons, 4.4 US tons) to a geosynchronous transfer orbit.

2014-12-18 01_00_29-LIVE_ GSLV Mk-3 1st test launch (X1) December 18, 2014 (ETD 0400UTC)For Thursday’s mission only the first stage and boosters were live, while the inert second stage was loaded with liquid nitrogen to simulate propellant.

India made its first attempt to launch a satellite on 10 August 1979, with its Satellite Launch Vehicle (SLV) carrying the Rohini Technology Payload, or RTP, in a launch from the Sriharikota Range (now known as the Satish Dhawan Space Centre).

Control of the rocket was lost following a valve failure in the second stage thrust vectoring system, with the rocket falling into the bay of Bengal.

India’s first successful launch came on 18 July in the following year, with the second Satellite Launch Vehicle orbiting the Rohini or RS-1 satellite.

In all, four Satellite Launch Vehicles were flown, with the third flight a failure and the fourth, in April 1983, a success.

With a capacity of only around 40 kilograms (90 lb) the SLV was unable to carry any significant payloads so an upgraded version, the Augmented Satellite Launch Vehicle (ASLV) was introduced.
2014-12-18-01_00_29-LIVE_-GSLV-Mk-3-1st-test-launch-X1-December-18-2014-ETD-0400UTC-311x350.jpg


Based around the SLV, the ASLV added two more solid motors, burning together as the rocket’s first stage, to the sides of the vehicle. A modified version of the four stage SLV served as the second, third, fourth and fifth stages of the ASLV.

The ASLV made its first flight from a new complex at Sriharikota, located close to the SLV pad, on 24 March 1987. The first two launches failed to achieve orbit, while the third left ISRO’s SROSS-C satellite in a lower-than-planned orbit.

Funding for the ASLV was cut in favour of the more capable Polar Satellite Launch Vehicle which by then under development, with the final ASLV launch on 4 May 1994 successfully carrying SROSS-C2 into orbit.

2014-12-18 01_01_23-ISRO PSLV - Google SearchThe PSLV began a new generation for India’s rockets; the only significant commonality PSLV and its predecessors was the use of S-9 motors – which had made up the first stage of the SLV and the first and second stages of the ASLV – as boosters attached to its first stage.

Far larger than its predecessors, the PSLV introduced a large solid first stage, with liquid second and fourth stages and another solid for the third stage. In its standard configuration it can place up to 3,700 kilograms (8,200 lb) of payload into low Earth orbit.

Having made 28 launches since September 1993, the PSLV has been used for two thirds of India’s orbital launches to date. In addition to being India’s most-flown rocket it is also the country’s most reliable, having suffered only one failure – during its maiden flight – and one partial failure in two decades of service.

Two additional configurations, the PSLV-CA (or Core Alone) and PSLV-XL have been developed to accommodate smaller and larger payloads respectively. The Core Alone configuration eliminates the boosters from the first stage, while the PSLV-XL replaces them with larger S-12 motors.

The most recently-developed orbital launch system in India’s fleet is the Geosynchronous Satellite Launch Vehicle, or GSLV. This vehicle was introduced in 2001 with the aim of enabling India to deploy its own communications satellites without relying on foreign rockets – providing a payload capacity of up to 2,200 kilograms (4,900 lb) to geosynchronous transfer orbit.

Based on the PSLV, it replaces the solid rocket boosters with larger liquid boosters and introduces a cryogenically-fuelled third stage. Early flights of the GSLV Mk.I used a Russian KVD-1M engine on the third stage, however the Mk.II configuration, first flown in April 2010, has an Indian-built engine in its place.

Despite ISRO’s hopes for the vehicle, the GSLV has proven unreliable with a success rate of only 37.5 percent. Only three of its eight launches to date have reached their planned orbits, with one additional launch reaching a usable, though lower-than-planned, orbit. January’s successful deployment of GSAT-14 was the GSLV’s first flawless mission in almost ten years.

2014-12-18 00_52_40-index.php (521×901)The LVM-3 or GSLV Mk.III is completely new development, a two stage rocket with twin solid boosters augmenting an all-liquid core vehicle.

The first stage, or L110, is powered by two Vikas engines, derived from France’s Viking series used on Ariane rockets between 1979 and 2004. Burning Unsymmetrical dimethylhydrazine (UDMH) propellant oxidised by dinitrogen tetroxide (N2O4), the L110 will be air-lit almost two minutes after the rocket lifts off under the power of its two booster rockets.

Each of the two S200 boosters will burn 207 tonnes (204 Imperial tons, 228 US tons) of solid propellant – a mixture of ammonium perchlorate, aluminium and hydroxyl-terminated polybutadiene (HTPB).

The rocket’s second stage, which was not tested on Thursday’s mission, is designated the C25. It was powered by a CE20 engine burning liquid hydrogen and liquid oxygen; however for the maiden flight the second stage was inert, loaded with liquid nitrogen to simulate propellant.

The name of the new rocket remains unclear, with ISRO continuing to refer to the rocket as both the LVM3 and GSLV Mk.III.

The payload for Thursday’s maiden launch was the Crew Module Atmospheric Reentry Experiment (CARE), which demonstrated the crew capsule which ISRO has been developing for its manned programme. The primary objective of CARE’s mission wa to validate the reentry and recovery of the prototype spacecraft.

The 3,735-kilogram (8,234 lb) spacecraft flew without the service module that will eventually accompany it on manned missions; instead it was attached to the second stage of its carrier rocket upside-down, inside the payload fairing.
2014-12-18-00_52_40-index.php-521%C3%97901-211x350.jpg


By launching upside-down, ISRO hope to simplify the CARE mission and increase the chances of success; eliminating the risk of having to modify the capsule’s heat shield to interface with the rocket and removing the need for the spacecraft to manoeuvre to reentry attitude following launch.

With the CARE mission, ISRO’s manned vehicle becomes the second such spacecraft to undergo a flight test this month; on 5 December NASA launched its Exploration Flight Test 1 mission to demonstrate its Orion spacecraft.

Although a more sophisticated flight than CARE, with the Orion spacecraft making two orbits of the Earth and entering at greater velocity from a higher apogee, EFT-1 had similar objectives to India’s mission – testing the spacecraft’s performance during reentry and validating recovery procedures.
2014-12-18-00_55_37-LIVE_-GSLV-Mk-3-1st-test-launch-X1-December-18-2014-ETD-0400UTC-350x225.jpg

The GSLV Mk.III launched from the Second Launch Pad (SLP) at the Satish Dhawan Space Centre, a complex constructed in the early 2000s for the PSLV and GSLV Mk.I. Thursday’s was the thirteenth launch from the pad, which was first used for the May 2005 launch of CartoSat-1 on a PSLV.

The second pad has been used for all GSLV launches since its completion, along with a handful of PSLV launches. The majority of PSLV missions are conducted from the nearby First Launch Pad.

For launches from the second pad, rockets are assembled vertically atop a mobile platform in an integration building about a kilometre southwest of the launch pad. The GSLV Mk.III prototype was rolled out a week ahead of launch to allow testing and rehearsals to be conducted in advance of liftoff.

Despite its name, the Second Launch Pad was not the second pad to be constructed at the centre; the numbering system does not take into account the two disused complexes which once hosted the Satellite Launch Vehicle and Augmented Satellite Launch Vehicle, nor does it include several sounding rocket pads.

2014-12-18 00_57_40-satish dhawan space centre - Google SearchThe Satish Dhawan Space Centre, which was formerly known as the Sriharikota Range, is named after former ISRO chairman Satish Dhawan. The facility was renamed in 2002 following the death of Dhawan in January of that year. It has been the site for all of India’s orbital launches. A third launch pad is currently under construction at the site to accommodate future missions, particularly for India’s manned space programme.

The rocket that flew Thursday’s mission has been designated GSLV Mk.III X1, or LVM3-X1. It flew in what ISRO consider a typical GSLV Mk.III flight profile up to the end of first stage flight, after which a series of simulated flight events will occur and the CARE spacecraft will be deployed for its reentry experiment.

The launch began when the countdown reaches zero, with ignition of the two S200 solid rocket motors. The rocket climbed away from its launch pad, flying on an azimuth of 120 degrees.

The first stage engines ignited 114.71 seconds after liftoff, at an altitude of 43.43 kilometres (26.99 miles, 23.45 nautical miles). The boosters burned together with the first stage until the 148.98 second mark in the launch, at which point they separated from the vehicle. Each booster was fitted with six separation motors which fired to take it clear of the core vehicle.

Three minutes and 52.7 seconds after liftoff the payload fairing separated from around the CARE spacecraft. The GSLV Mk.III used a fairing with a diameter of five metres (16 feet) designed to encapsulate the payload and protect it from atmospheric friction during its ascent to space.

First stage flight ended with the Vikas engines shutting down five minutes and 17.62 seconds after liftoff. The spent first stage separated from the second stage mockup 2.8 seconds later. Eleven tenths of a second after staging, the second stage simulated its own shutdown and spacecraft separation occurred four seconds later.

The GSLV accelerated CARE to a velocity of around 5.3 kilometres per second (3.3 miles per second, 12,000 mph) and a projected apogee of 126 kilometres (78 miles, 68 nautical miles), plus or minus one kilometre, which was achieved around the time of stage separation.

Immediately after separating from the rocket, CARE activated its control systems, consisting of six reaction control system thrusters each capable of delivering 100 newtons of thrust. The RCS was used to provide three-axis control, guiding the spacecraft for the first two minutes and eleven seconds of free flight, before being deactivated around the time of entry interface as the spacecraft performed an unguided ballistic descent.
2014-12-18-00_56_34-LIVE_-GSLV-Mk-3-1st-test-launch-X1-December-18-2014-ETD-0400UTC-350x235.jpg


Following entry interface, deployment of CARE’s drogue parachutes occurred nine minutes and 40 seconds into the mission, at an altitude of 15.4 kilometres. The drogue chutes slowed the capsule as it continued its descent, until the main parachutes were deployed around 202 seconds later with the spacecraft three kilometres above the Indian Ocean.

Splashdown occurred around 180 kilometres south of the Andaman and Nicobar Islands, where CARE will be recovered by the Indian Coast Guard. In all the mission lasted nineteen minutes from liftoff to splashdown.

Thursday’s mission concluded ISRO’s launch activities for 2014, following four successful orbital launches earlier in the year. The Geosynchronous Satellite Launch Vehicle began the year on 5 January with the deployment of GSAT-14 – the first successful launch of the GSLV Mk.II and the first for any GSLV configuration since 2004, ending a string of four consecutive launch failures.

PSLV launches in April and October deployed IRNSS navigation satellites, while a further PSLV launch in June orbited France’s SPOT-7 imaging satellite along with several miniature satellites.

India’s first launch next year will be of a PSLV-XL with another IRNSS spacecraft. This will be the first of several IRNSS launches in 2015, with missions to deploy a trio of British imaging satellites and ISRO’s AstroSat astronomy spacecraft also tentatively planned.

A development flight of the GSLV Mk.II is scheduled for around the end of the first quarter, carrying the GSAT-6 military communications satellite.

The GSLV Mk.III is not expected to fly again until 2016 or early 2017, when the rocket will make its first orbital flight – designated D1 – with the GSAT-19E spacecraft.
2014-12-18-00_53_45-LIVE_-GSLV-Mk-3-1st-test-launch-X1-December-18-2014-ETD-0400UTC-350x232.jpg


Please, Log in or Register to view URLs content!



[video=youtube;pD0RtxuGxug]https://www.youtube.com/watch?v=pD0RtxuGxug[/video]
 
Last edited:
Top