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NASA on Tuesday celebrated exceeding expectations during a mission to deflect a distant asteroid, in a sci-fi like test of humanity’s ability to stop an incoming cosmic object from devastating life on Earth.

The fridge-sized Double Asteroid Redirection Test (DART) impactor deliberately smashed into the moonlet asteroid Dimorphos on September 26, pushing it into a smaller, faster orbit around its big brother Didymos, NASA chief Bill Nelson announced.

That changed its orbital period by four percent, or 32 minutes — from 11 hour 55 minutes to 11 hours 23 minutes, bettering an expectation of 10 minutes.

“At some point in the future, if we find an asteroid that is threatening to hit Earth, and would be large enough to really do some damage, thank goodness that we will have had this successful test,” Nelson told AFP.

The asteroid pair loop together around our Sun every 2.1 years, and pose no threat to our planet.

But they are ideal for studying the “kinetic impact” method of planetary defense.

DART’s success as a proof-of-concept has made a reality what was once science fiction — notably films such as “Armageddon,” “Deep Impact,” and “Don’t Look Up.”

Never actually photographed before, Dimorphos, which is 530 feet (160 meters) in diameter or roughly the size of a big Egyptian pyramid, appeared as a speck of light around an hour before impact.

Its egg-like shape and craggy, boulder-dotted surface finally came into clear view in the last few moments, as DART raced toward it at roughly 14,500 miles (23,500 kilometres) per hour.

Pseudo-comet 

In the days that followed, astronomers rejoiced in stunning images of matter spreading out thousands of miles — pictures collected by Earth and space telescopes, as well as a tiny companion satellite that traveled to the zone with DART.

Thanks to its temporary new tail, Dimorphos has turned into a man-made comet.

But quantifying just how well the test worked required an analysis of light patterns from ground telescopes, which took a few weeks to become apparent.

The binary asteroid system, which was around 6.8 million miles (11 million kilometres) from Earth at impact, is visible only as a single dot from the ground.

The dot’s brightness changes as Dimorphos passes in front of Didymos, which is significantly bigger at half-a-mile wide.

Four optical telescopes were involved in measuring the orbital period — all in Chile and South Africa — while two US-based radar telescopes helped confirm the finding, said NASA planetary scientist Nancy Chabot.

The test also showed scientists that the asteroid is less like a solid rock, and more like a “rubbish pile” of boulders bound by mutual gravity.

If an asteroid is more solid, the momentum imparted by a spaceship will be limited. But if significant mass is pushed at high velocity in the opposite direction to impact, there will be an additional boost.

“It looks like the recoil from the ejecta blast off the surface was a substantial contributor to the overall push given to the asteroid,” said NASA scientist Tom Statler at a briefing.

The test will serve as an “anchor point” for simulations and calculations about the outcome of future impacts, he added.

Mass extinction

No known asteroid larger than 140 meters (460 feet) in size — big enough to devastate a city — has a significant chance to hit Earth for the next 100 years, according to NASA.

But wait long enough, and it will happen.

The geological record shows, for example, that a six-mile wide asteroid struck Earth 66 million years ago, plunging the world into a long winter that led to the mass extinction of the dinosaurs along with 75 percent of all species.

The agency plans to launch in 2026 a telescope called the Near-Earth Object (NEO) Surveyor to better characterize potentially hazardous 140-meter asteroids and comets that come within 30 million miles.

So far, less than half of the estimated 25,000 NEOs of 140 meters have been discovered.

Kinetic impact with a spaceship is just one way to defend the planet, albeit the only method possible with current technology.

Should an approaching object be detected early, a spaceship could be sent to fly alongside it for long enough to divert its path via using the ship’s gravitational pull, creating a so-called gravity tractor.

Another option would be launching nuclear explosives to redirect or destroy an asteroid.

NASA believes the best way to deploy such weapons would be at a distance, to impart force without blowing the asteroid to smithereens, which could further imperil Earth.


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Japan Launches Final H-2A Rocket with GOSAT-GW Satellite to Monitor Climate and Oceans

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Japan Launches Final H-2A Rocket with GOSAT-GW Satellite to Monitor Climate and Oceans

Japan launched a satellite which is a dual purpose, for monitoring greenhouse gases and sea temperature. On Saturday, June 28, 2025, the Japan Aerospace Exploration Agency (JAXA) held its 50th and final launch of the H-2A rocket, launching the GOSAT-GW satellite of dual purpose to space. This mission lifted off from Ypshinobu Launch Complex (LP-1) in Japan at Tenegashima Space Centre at 10:03 p.m. IST. These satellites have been sent by Japan to observe the changes in water cycles and greenhouse gases.

JAXA’s Dual Purpose Satellite Launch

According to JAXA, the Greenhouse Gas and Water Cycle Observation Satellite (GOSA-GW) is a very recent and significant effort of Japan to know about the effect of greenhouse gases and the changes in the cycle of rain. GOSAT-GW has joined the orbit of Earth with GCOM-W2, which is its predecessor, and was launched in 2012, known as SHIZUKU, whereas GOSAT-1, launched in 2009, is known as IBUKI. It is equipped with two main instruments.

More About GOSAT-GW

GOSAT-GW is equipped with two main instruments, the first is called the Advanced Microwave Radiometer (AMSR), and the other is known as the Greenhouse Gases Observation Sensor (TANSO). The former one will measure water cycles and sea surface temperature fluctuations, while the latter one is for monitoring components such as carbon dioxide in Earth’s atmosphere for measuring climate change.

H-2A rocket of Japan has been capable of launching payloads into the geostationary orbit around Earth and also orbiting the Moon. JAXA also launched the Akatsuki spacecraft for studying Venus in 2010; however, the spacecraft failed to enter the orbit of Venus properly.

Japan’s Successful Launch Operations

JAXA launched H-2A for the first time in 2001. With its 25 years in operation, the rocket experienced only a single failure, giving the spacecraft a 98% success rate. After 50 missions, the launch vehicle is now being retired to make way for the H3 rocket of Japan, offering comparable performance at a very reasonable cost.

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SpaceX Launches 53 Starlink Satellites in One Day, Crossing 7,900 Active Units

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SpaceX Launches 53 Starlink Satellites in One Day, Crossing 7,900 Active Units

On June 28, 2025, two Falcon 9 rockets carrying the internet satellite broadband connection lifted off at 12:26 a.m. and 1:13 p.m. EDT. The first one was launched from Space Launch Complex 40 at Cape Canaveral Space Force Station, Florida, and another from Space Launch Complex 4 East at Vandenberg Space Force Base, California. The new addons for megaconsellation of SpaceX (Group 10-34 and Group 15-7) reached low orbit Earth about 9 minutes after leaving the ground and were deployed after an hour.

According to As per NASA, in the intervening time, the first stage of the Falcon rockets (boosters B1092 and B1088) flew back to the droneships. The landing was on “A Shortfall of Gravitas, “ completing the fifth flight of the boosters. The stage touched down on “Of Course I Still Love You”, with its eighth flight to space and back, in the Pacific Ocean.

The launch at early morning carries 27 Starlink Satellites and the afternoon liftoff lofted 26 more of the relay satellites, vasting the network of SpaceX to more than 7,900 active units, said by satellite tracker Jonathan Mc Dowell.

Broader Deployment Context

The launch in the morning was delayed earlier that day because of the severe weather alerts at Florida, but flew in the near perfect conditions at the visibility of 10 miles. Throughout 2025, SpaceX heald 42 Falcon 9 missions with 28 Starlink launched by June. by mid-June the batch of 26 satellites launched from Vandenberg (Booster B1081’s 15th flight) which contributed to more than 7,600 active satellites by June 12.

Both the missions are a part of an aggressive Starlink deployment, mainly for boosting the low Earth orbit constellation for the global broadband coverage. Now the network expands to approximately 7900 satellites, focusing on the biggest LEO broadband constellation ever.

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Astronomers Discover a Gigantic Supernova Remnant in the Large Magellanic Cloud

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Astronomers Discover a Gigantic Supernova Remnant in the Large Magellanic Cloud

Astronomers international team has employed various satellites and telescopes for performing multiwavelength observations of a supernova remnant known as SNR J0450.4-7050. The result that scientists got after an observational campaign, published on June 18, 2025, on the preprint server arXiv, gained new insights into the properties of this remnant, and observed that it is much larger than thought in the past. Supernova remnants (SNRs) are expanded structures resulting from the explosion of a supernova. It usually lasts for several hundred thousand years before the time it disperses into the interstellar medium.

Multiwavelength Observations Reveal New Details of SNR J0450.4-7050

As per the study by NASA, observations by the scientists indicate that SNRs contain the ejected expansion of material from the explosion and other interstellar material swept by the passage of the shockwave from the star that exploded. SNR studies beyond the Milky Way are important for comprehending the feedback in different evolutionary phases and gaining valuable insights into the local ISM. The Large Magellanic Cloud is the galaxy that has its SNR population explored in depth.

Importance of Studying Supernova Remnants Beyond the Milky Way

The recent observations reveal that SNR J0450.4-7050, a large supernova remnant in the LMC having physical dimensions of 332 by 244 light years, is estimated to have the remnants of around 45,000 years old. Scientists named it Veliki, which means large in Serbian. It also showcases the complex filamentary morphology with different inner and outer shell structures.

Discovery of Veliki: A Large, Aged Remnant in the Large Magellanic Cloud

An astronomer’s group led by Zachary J. Smeaton decided to take a closer observation of SNR J0450.4−7050 by the Australian Square Kilometre Array Pathfinder and MeerKAT radio telescope. The SNR showed a high radial surface brightness with one of the lowest average radio spectral indices, with similar remnants.

Unusual Radio Properties Suggest Veliki is a Fully Radiative SNR

These unusual features, according to the scientists, give the prediction that Veliki is mainly a radiative SNR with a high shock compression ratio. This states about the non-thermal spectrum and higher surface brightness and emissions. Further observations of the surrounding environment are needed to confirm the hypothesis with an understanding of the remnants’ nature in a better way.

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