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When Indian space agency scientists set out to design the Chandrayaan-3 moon mission, they knew they had one more chance to make history with a landing on the lunar south pole after a failed attempt four years ago.

They also had to do it on a shoestring budget and ended up spending only Rs. 6.15 billion on the mission.

From managing costs on rockets to developing a built-in-India supply base, the Indian Space Research Organisation’s (ISRO) success with the Chandrayaan-3 moon landing shows how it has honed a system of doing more for less, officials, suppliers and analysts say.

ISRO’s record for frugal innovation will be tested by upcoming missions, including a project to study the sun set to launch next month and a plan to put astronauts in orbit.

Although India’s government allocated the equivalent of $1.66 billion (nearly Rs. 13,700 crore) for the department of space for the fiscal year ending in March, it spent around 25 percent less. The budget for the current fiscal year is $1.52 billion (nearly Rs. 12,560 crore).

By contrast, NASA has a $25 billion (nearly Rs. 2,06,585 crore) budget for the current year. Put another way, the annual increase in NASA’s budget — $1.3 billion (nearly Rs. 10,750 crore) — was more than what ISRO spent in total.

“No one in the world can do it like we do,” said S Somanath, ISRO chairman and a veteran aerospace engineer, who was celebrating Chandrayaan’s successful touchdown on Wednesday.

“I won’t disclose all secrets, otherwise everyone else (can) become cost effective,” he said at a news conference.

One example of how ISRO contained costs on Chandrayaan-3: it opted to take a longer route to the moon, allowing it to use less powerful – and cheaper – propulsion systems. Chandrayaan-3 took more than 40 days to reach the moon, looping through widening orbits to use the Earth’s gravitational force as a slingshot.

By contrast, Russia’s Luna-25 mission, which crashed before its own attempted landing on the moon’s south pole, had been on a more direct course to the moon. Russia has not disclosed what it spent on the failed mission.

“To take a direct route takes more power, more fuel, and is far more expensive,” said Somak Raychaudhury, an astrophysicist and vice chancellor of Ashoka University. 

ISRO also developed some of the lander components itself, including the cameras, altimeter and hazard avoidance sensors. It used Indian suppliers for vehicle assembly, transportation and electronics to keep costs low. And it limited the number of design prototypes to save time and money.

“With local sourcing of equipment and design elements, we are able reduce the price considerably. A similar set up by an international vendor would cost four to five times,” Amit Sharma, CEO of Tata Consulting Engineers, which was a vendor to ISRO for the Chandrayaan-3 project, told Reuters.

Stretching every rupee

Many of the ISRO scientists who worked on the failed Chandrayaan-2 attempt to land on the lunar south pole in 2019 stayed on for the current mission. 

ISRO is gearing up to launch the Aditya-L1 spacecraft, a space-based solar observatory, in September. It has plans to send astronauts to space in a mission ISRO’s Somanath has said could come by 2025. 

ISRO’s success is also expected to provide a lift for the country’s private-sector space start-ups at a time when Prime Minister Narendra Modi’s government is looking to open the sector to foreign investment, suppliers say.

Ankit Patel, founder and director of Ankit Fasteners, which has been supplying nuts, bolts and other fasteners to ISRO since 1994, said there were times when parts had to be hand carried to a launchpad to meet a deadline.

“The unsung heroes of ISRO are the engineers who are pushing their suppliers every day to achieve the set timeline,” Patel told Reuters.

He added: “ISRO has been very frugal with its expenditure. ISRO needs to think out of the box to stretch every rupee.” 

© Thomson Reuters 2023


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NASA Reveals a Fracture in Huge Cosmic Bone: Everything You Need to Know

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NASA Reveals a Fracture in Huge Cosmic Bone: Everything You Need to Know

X-ray is a very common method that almost every individual is well aware of. However, ever wondered what an X-ray of the Milky Way would look like? Or is that even possible? Well, yes, it is. Recently, NASA’s Chandra X-Ray Observatory has carried out an image of a recent scan, which revealed a fractured bone. As specified in Space.com, the bone-like structure, which was witnessed in the X-ray image, was derived from the radio data obtained by the MeerKAT Radio Array in South Africa and the National Science Foundation’s Very Large Array in New Mexico.

About the Cause of Fracture

According to the data obtained from Chandra’s X-ray, the fracture, also known as the galactic center filament, was caused by the impact from a pulsar. A pulsar is a spinning neutron star that emits radiation constantly at regular intervals. Revealed in Space.com, the scientists are highly skeptical about the speed of the pulsar, during slamming, would have been between one to two million miles per hour.

What is a Galactic Center Filament

Milky Way, undoubtedly, does not consist of bone. However, what looks like a real bone is a Galactic Center Filament, which is an amalgamation of structures crafted by the radio waves interwoven with the magnetic fields, right at the center of the Milky Way.

What did scientists discover?

As conveyed to Space.com, this is one of the brightest and longest galactic center filaments that have been detected so far. The distances of these filaments are 26,000 light-years and 230 light-years long. The bone has been named as G359.13142-0.20005.

The Scientist’s Verdict

Narrated to Space.com, the scientists suggest that the collision with the neutron stars would have dismantled the filament’s magnetic field, which further resulted in the fracture. The scientists are hopeful that the fracture will heal itself.

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NASA Telescopes Reveal Hidden Properties of X-Ray Pulsar RX J0032.9-7348

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NASA Telescopes Reveal Hidden Properties of X-Ray Pulsar RX J0032.9-7348

Pulsars are neutron stars rotating rapidly, emitting electromagnetic radiation in various wavelengths, including radio waves, optical, X-ray, and gamma-ray. Identified as a X ray transient source in the Small Magellanic Cloud (SMC) about 30 years ago, RX J0032.9-7348 has been classified as an X-ray Pulsar after detecting X-ray pulsations with a period of approximately 7.02 seconds after experiencing an X-ray brightening in October 2024.To take a closer look at it, astronomers have incorporated two NASA X-ray telescope, NICER and NuSTAR.

Discovery and Observational Campaign

According to Handbook of X-ray and Gamma ray Astrophysics, Accretion-powered X-ray pulsars (XRPs) are neutron stars within binary systems that emit X-rays in regular pulses, powered by the accretion of matter from a companion star. However, although RX J0032.9-7348 has been known for decades, very little is known regarding its properties and its optical counterpart has not been identified. Therefore, a team of astronomers led by Birendra Chhotaray of the Physical Research Laboratory (PRL) in Ahmedabad, India, decided to take a closer look at this pulsar with NuSTAR and NICER.
Dr Chhotaray and his team were able to verify the X-ray pulsation period of RX J0032.9-7348 through their observations and they also discovered that this pulsar has a double-peak pulse profile throughout a wide energy range, with small changes in the form of energy dependence.

Findings

Results of the observational campaign, published on the arXiv preprint server, gives insight of the spin dynamics and luminosity of this pulsar. The accretion processes during the X-ray brightening phase increases its angular momentum. It results into a spin-up of approximately -0.00033 seconds per day.
The luminosity of the pulsar varied from 8.2 undecillion to 37 undecillion erg/s during the monitoring campaign. The researchers report that no evidence of iron emission line or cyclotron resonance scattering features was found in the energy spectrum of this source.

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Soviet Venus Probe Kosmos 482 Set to Re-Enter Earth After 53 Years in Single Piece



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Soviet Venus Probe Kosmos 482 Set to Re-Enter Earth After 53 Years in Single Piece

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Soviet Venus Probe Kosmos 482 Set to Re-Enter Earth After 53 Years in Single Piece

Kosmos 482, under the USSR Venera program, was launched into space in 1972 to land on the second planet. However, the rocket malfunctioned and in Earth’s orbit, and it’s still revolving there ever since. Its rugged design lets it stay there and tolerate the atmosphere of Venus. This durability implies that it could survive reentry into Earth and remain intact with no impact. It is supposed to land either on 9 or 10 May without actually breaking anything up. The Aerospace Corporation is tracking it through the radar data provided by the U.S Space network surveillance.

When and Where Might It Land?

As per the current forecasts, ESA reports that the lander will re-enter the Earth’s atmosphere on Saturday, May 10, 12:37 PM EST, with an error margin of ±20.6 hours. Due to an orbital inclination of 52 degrees, it is possible that it could land between the vast regions including Australia, South America and Africa, and in water covering these areas. On the map, it is between 52 degrees North and 52 degrees south. It may fall into the ocean, as 70% of the Earth is water.

What Happens If It Survives Reentry?

If Kosmos 482 reaches the Earth in one piece, the speed would be 150-250 km per hour. The structure would be the same, that is, around 1 meter in diameter and 495 kgs in weight. The scientists predict that the parachute system must have no longer been there after 53 years in space.

Exact Timing Become Challenging

Solar activities, such as storms, are adding complexity to the radar data sometimes which in turn is impacting the reentry timings. Langbroek says, The Sun does whatever it wants to do, making it difficult to analyse the exact hours until the last moment.

Risk to the Public Is Low

Scientists say that the risk to humans is minimal, with a 0.4% chance of death or even injury. It will come down as a single object, with no debris risk. However, if anyone happens to encounter is should stay away and not touch it, simply report to the local authorities.

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NASA’s SPHEREx Telescope Begins 3D Infrared Mapping of the Universe



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