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The Indian Space Research Organisation announced on Thursday that the Chandrayaan-3 mission is scheduled to be launched at 2.35 pm on July 14, with the lander expected to soft-land on the surface of the Moon on August 23 or 24. 

Chandrayaan-3 is a follow-on mission to Chandrayaan-2 to demonstrate end-to-end capability in safe landing and roving on the lunar surface.

The Chandrayaan-3 spacecraft, which will be launched by LVM3 (Launch Vehicle Mark-III) (earlier referred as GSLV Mk III), is a composite of three modules — propulsion, lander, and rover (which is housed inside the lander).

“LVM3-M4/Chandrayaan-3 Mission:The launch is now scheduled for July 14, 2023, at 2:35 pm IST from SDSC, Sriharikota”, the national space agency headquartered here said in a tweet.

Secretary of the Department of Space and ISRO Chairman Somanath S told reporters that the space agency would attempt soft-landing of the lander on August 23 or August 24.

ISRO officials noted that the mission life of the lander is one lunar day, which is equal to 14 Earth days.

“The date (for soft-landing) is decided based on when there is sunrise on the Moon. While landing, sunlight must be there. There is sunlight on the Moon for 14-15 days and for the next 14-15 days there is no sunlight,” they noted.

Chandrayaan-3 mission carries scientific instruments to study the thermo-physical properties of the lunar regolith, lunar seismicity, lunar surface plasma environment and elemental composition in the vicinity of the landing site.

While the scope of these scientific instruments on the lander and the rover would fit in the theme of “Science of the Moon”, another experimental instrument will study the spectro-polarimetric signatures of the Earth from the lunar orbit, which would fit in the theme of “Science from the Moon”, according to ISRO officials.’.

In March this year, the Chandrayaan-3 spacecraft successfully completed the essential tests that validated its capability to withstand the harsh vibration and acoustic environment that the spacecraft would encounter during its launch.

The propulsion module, which has Spectro-polarimetry of Habitable Planet Earth (SHAPE) payload to study the spectral and polarimetric measurements of Earth from the lunar orbit, will carry the lander and rover configuration till 100 km of lunar orbit.

Lander payloads are: ‘Chandra’s Surface Thermophysical Experiment’ to measure the thermal conductivity and temperature; ‘Instrument for Lunar Seismic Activity’ for measuring the seismicity around the landing site; and ‘Langmuir Probe’ to estimate the plasma density and its variations.

A passive Laser Retroreflector Array from the US space agency, National Aeronautics and Space Administration (NASA), is also accommodated for lunar laser ranging studies.

Rover payloads are: ‘Alpha Particle X-ray Spectrometer’ and ‘Laser Induced Breakdown Spectroscopy’ for deriving the elemental composition in the vicinity of the landing site.

The lander will have the capability to soft-land at a specified lunar site and deploy the rover which will carry out in-situ chemical analysis of the lunar surface during the course of its mobility.

The main function of the propulsion module is to carry the lander module from launch vehicle injection till final lunar 100 km circular polar orbit and separate it. Apart from this, the propulsion module also has one scientific payload as a value addition which will be operated post separation of the lander module, it was noted.


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Meteorite From Outer Solar System Challenges Planet Formation Timeline in Early Solar System

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Meteorite From Outer Solar System Challenges Planet Formation Timeline in Early Solar System

A minuscule meteorite seems to be rewriting the history of our solar system. The 50-gram Northwest Africa 12264 has brought a new understanding of when and how rocky worlds came together. Inner planets such as Earth and Mars were thought to have formed earlier than their more distant siblings, given temperatures and composition. But a new study of this meteorite, which originates from beyond the asteroid belt, suggests that the birth of planets throughout the solar system occurred tens of millions of years earlier than previously believed, narrowing the gap in time between the solar system’s inner and outer surfaces.

Outer Solar System Meteorite Reveals Rocky Planets Likely Formed Simultaneously Across the Galaxy

As per a study led by Dr Ben Rider-Stokes of The Open University and published in Communications Earth & Environment, the meteorite’s chemical makeup offers critical evidence. Its chromium and oxygen isotope ratios place its origin in the outer solar system. Most strikingly, lead isotope dating determined its age to be about 4.564 billion years, almost identical to basalt samples from the inner solar system that represent early planetary crusts.

These findings directly challenge the previous assumption that rocky planets beyond Jupiter formed two to three million years later due to their water-rich composition. Ice and water were thought to slow differentiation, the internal layering of planetary bodies. But this meteorite, with its outer solar birth and inner solar age, points to a far more synchronised process of rocky planet formation.

Scientists note that the discovery is also consistent with observations of exoplanetary systems. Based on this and past observations of disks of dust and gas around other stars, the evidence of planetesimals forming quickly and over large orbital separations adds to the argument that early solar system evolution may have been more universal than thought.

As trivial as the time difference might be in the context of a universe, the question is huge. A new timeline of planet formation is not only a retelling of Earth’s history but may also help determine how astronomers think about how planets form in the galaxy more generally, providing new hints about where and how in the galaxy Earth-like planets could take shape.

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NASA’s Hubble and Webb Discover Bursting Star Formation in Small Magellanic Cloud



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NASA’s Hubble and Webb Discover Bursting Star Formation in Small Magellanic Cloud

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NASA’s Hubble and Webb Discover Bursting Star Formation in Small Magellanic Cloud

Scientists from NASA observed the bursting expansion of gas, stars, and dust from the glittering territory of the dual star clusters using Hubble and Webb space telescopes. NGC 460 and NGC 456 stay in the Small Magellanic Cloud, which are open clusters, with dwarf galaxies and orbit the Milky Way. These clusters are part of the extensive star complex clusters and nebulae that are most likely to be linked to each other. Stars are born upon the collapse of clouds.

Hubble and Webb Reveal Explosive Star Births in Small Magellanic Cloud

As per a report from NASA, the open clusters are from anywhere from a few dozen to many young stars, which are loosely bound by gravity. The images captured by Hubble capture the glowing and ionised gas, which comes from stellar radiation and blows bubbles in the form of gas and dust, which is blue in colour. The infrared of Webb shows the clumps and delicate filament-like structures and dust, which is red in colour.

NGC 460 and NGC 456: A Window into Early Universe Star Formation

Hubble shows the images of dust in the form of a silhouette against the blocking light; however, in the images of Webb, the dust is warmed by starlight and glows with infrared waves. The blend of gas and dust between the stars of the universe is called the interstellar medium. The region holding these clusters is known as the N83-84-85 complex and is home to multiple, rare O-type stars. These are hot and extremely massive stars that burn hydrogen like the Sun.

Such a state mimics the condition in the early universe; therefore, the Small Magellanic Cloud gives a nearby lab to find out the theories regarding star formation and the interstellar medium of the cosmos’s early stage.

With these observations, the researchers tend to study the gas flow from convergence to divergence, which helps in refining the difference between the Small Magellanic Cloud and its dwarf galaxy, and the Large Magellanic Cloud. Further, it helps in knowing the interstellar medium and gravitational interactions between the galaxies.

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New Interstellar Object 3I/ATLAS Could Reveal Secrets of Distant Worlds

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New Interstellar Object 3I/ATLAS Could Reveal Secrets of Distant Worlds

The entry of a third known object into our solar system has been confirmed on July 1, 2025 by the astronomers. This object is named 3I/ATLAS, where 3I stands for “Third Interstellar”, having a highly hyperbolic (eccentricity ≈ 6.2) orbit, confirming it is not bound to the Sun but is a true interstellar visitor. Only two such visitors, 1I/ʻOumuamua (2017) and 2I/Borisov (2019), had been seen before. Notably, 3I/ATLAS appears to be the largest and brightest interstellar wanderer yet discovered.

Comparison with previous interstellars

According to NASA, astronomers from the ATLAS survey first spotted the object on July 1, 2025, using a telescope in Chile. It immediately drew attention for its unusual motion. Shortly after discovery, observers saw a faint coma and tail, leading to its classification as comet C/2025 N1 (ATLAS).

This comet-like appearance is shared with 2I/Borisov, the second interstellar visitor. Global observatories now track 3I/ATLAS. It poses no threat but offers a rare opportunity to study alien material. Since 1I/ʻOumuamua was observed only as it was leaving the solar system, it was difficult for astronomers to get enough data on it to confirm its exact nature — hence the crazy theories about it being an alien spaceship — though it’s almost certainly an asteroid or a comet.

Size and Significance

3I/ATLAS is much larger and brighter than earlier interstellar visitors. It is about 15 kilometers (km) [9 miles] in diameter, with huge uncertainty, compared to 100m for 1I/’Oumuamua and less than 1km for 2I/Borisov. This brightness and size makes it a a better target for study. Astronomers are planning to analyze its light for chemical signatures from its home system to get clues about the formation of distant planetary systems.

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