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As anticipation grows for India’s planned Chandrayaan-3 lunar landing on Wednesday, an expert delves into the fascinating world of Moon exploration. The Moon has captivated human curiosity for centuries, and with each new mission, we uncover more about its geological history, composition, and potential for scientific discovery.

Dr. TV Venkateswaran, a scientist at Vigyan Prasar, an autonomous organisation under the Department of Science and Technology (DST), and a member of the public outreach committee of the Astronomical Society of India, answers key questions about the Moon’s geological evolution, the significance of its south pole, the presence of water and ice, and India’s ambitious plans for lunar exploration.

What is Moon’s geological history and evolution? In other words, how old it is, and when/how did it form?

The Moon is estimated to be about 4.5 billion years old, roughly the same age as the Earth. The leading theory about the Moon’s formation suggests that a Mars-sized celestial body collided with the young Earth, and the debris from this collision eventually coalesced to form the lunar body. However, current geological evidence from Moon suggests that it may be younger by just 60 million years compared to Earth.

How much do things weigh on the Moon, relative to Earth, and why?

The Moon’s gravitational pull is much weaker than Earth’s, approximately one-sixth of Earth’s gravity. As a result, objects on the Moon weigh significantly less than they do on Earth. This is due to the Moon’s smaller size and mass. For example, a person weighing 68 kilograms on the Earth would weigh only over 11 kg on the Moon.

Why do Indian scientists want to land on Moon’s south pole?

The lunar south pole has become a focal point for exploration due to its unique features and potential scientific value. It is believed to host a vast reservoir of water ice in permanently shadowed regions. The presence of water is of immense significance for future space exploration, as it can be converted into resources such as drinking water, oxygen, and hydrogen for rocket fuel. Also, the permanently sunlit area in the region has a temperature of around minus 50 to 10 degrees Celsius, which provide a better chemical condition for the electronics onboard the rover and lander to work properly.

What is in the lunar south pole? Is the terrain and geology there the same as elsewhere on the Moon or do we have no idea?

The terrain and geology at the Moon’s south pole are distinct from other regions. Permanently shadowed craters provide extremely cold conditions that allow water ice to accumulate and persist. The unique geography of the south pole also creates regions of perpetual sunlight, which can be harnessed for solar power. The terrain varies from rugged landscapes to relatively flat plains, offering a diverse range of scientific opportunities.

Why is a region of the lunar south pole permanently shadowed?

This depends on the Moon’s geology. The Moon’s axis is only slightly tilted relative to its orbit around the Earth. This results in certain areas near the poles being in permanent shadow. These shadows create extremely cold environments where temperatures can plummet to very low levels. These frigid conditions are conducive to preserving water ice for billions of years.

Does water/ice exist on the lunar south pole? Chandrayaan-1 seemed to have suggested it.

Yes, water ice has been confirmed to exist in the Moon’s south pole region. Data from various lunar missions, including India’s Chandrayaan 1, launched in 2008, have indicated the presence of water molecules in these permanently shadowed regions. This discovery has opened up exciting possibilities for sustained lunar exploration.

Is water/ice critical for future lunar exploration?

Water ice is a critical resource for future lunar exploration and even beyond. It can be converted into breathable air, drinking water, and most importantly, hydrogen and oxygen for rocket fuel. This could revolutionise space travel by reducing the need to transport these resources from Earth, making long-duration missions more feasible.

Does India plan to send a manned mission to the Moon in the future?

While ISRO has expressed its intention to send astronauts to space as part of its Gaganyaan mission, there are no plans yet to send human missions to the Moon in the near future.


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NASA Satellite Detects Tree Leaf Changes as Early Volcano Eruption Warning Signal

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NASA Satellite Detects Tree Leaf Changes as Early Volcano Eruption Warning Signal

NASA scientists might soon be able to forecast volcanic eruptions by monitoring how trees respond from space. Now, in a new collaboration with the Smithsonian Institution, they have discovered that tree leaves grow lusher and greener when previously dormant volcanic carbon dioxide seeps up from the ground — an early warning that a cone of magma is pushing upwards. Now, using satellites such as Landsat 8 and data from the recent AVUELO mission, scientists think this biological response could be visible remotely, serving as an added layer of early warning for eruptions in high-risk areas that currently menace millions worldwide.

NASA Uses Tree Greening as Satellite Clue for Early Volcano Eruption Warnings in Remote Regions

As per the research by NASA’s Earth Science Division at Ames Research Centre, greening occurs when trees absorb volcanic carbon dioxide released as magma rises. These emissions precede sulfur dioxide and are harder to detect directly from orbit.

While carbon dioxide does not always appear obvious in satellite images, its downstream effects — enhanced vegetation, for example — can help reinforce existing volcanic early warning systems, notes volcanologist Florian Schwandner. It could be important because, as the U.S. Geological Survey says, the country is still one of the most volcanically active.

Globally, about 1,350 potentially active volcanoes exist, many in remote or hazardous locations. On-site gas measurement is costly and dangerous, prompting volcanologists like Robert Bogue and Nicole Guinn to explore tree-based proxies.

Guinn’s study of tree leaves around Sicily’s Mount Etna found a strong correlation between leaf colour and underground volcanic activity. Satellites such as Sentinel-2 and Terra have proven capable of capturing these subtle vegetative changes, particularly in forested volcanic areas.

To confirm this method, climate scientist Josh Fisher led NASA-Smithsonian teams in March 2025 to Panama and Costa Rica, collecting tree samples and measuring gas levels near active volcanoes. Fisher sees this interdisciplinary research as key to both volcano forecasting and understanding long-term tree response to atmospheric carbon dioxide, which will reveal future climate conditions.

The benefits of early carbon dioxide detection have been demonstrated in the 2017 eruption of Mayon volcano in the Philippines, where it allowed mass evacuations and saved more than 56,000 lives. It has its limitations, like bad terrain or too much environmental noise, but it could be a game-changer.

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Russian Researchers Discover 11 New AGNs in All-Sky X-ray Survey

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Russian Researchers Discover 11 New AGNs in All-Sky X-ray Survey

11 new active galactic nuclei were detected in an all-sky X-ray source survey conducted by researchers from the Russian Academy of Sciences. A team led by Grigory Uskov has been on an inspection of the X-ray sources found in the ART-XC telescope of the Spektr-RG (SRG) space observatory. So far, their studies have resulted in the identification of more than 50 AGNs and several cataclysmic variables. A deeper dive into the physical properties and radiation nature of those galaxies will be crucial for a wide range of studies such as statistical insights, refining and testing cosmological models, classification studies etc.

Classification of newly found AGN

According to the recent study published in Astronomy letters, the newly discovered active galactic nuclei from the ARTSS1-5 catalog are categorised as the Seyfert galaxies, seven type 1 (Sy 1), three type 1.9 (Sy 1.9) and one type 2 (Sy 2).

AGN or active galactic nuclei are considered as the most luminous persistent sources of electromagnetic radiation in the universe. These compact regions at the centre of a galaxy are extremely energetic due to accretion onto a supermassive black hole or star formation activity at the galaxy’s center.

Based on their luminosity, AGNs are categorised as Seyfert Galaxies and Quasars. Seyfert galaxies are lower-luminosity AGNs where the host galaxy is clearly visible and emit a lot of infrared radiation, and have broad optical emission lines.

Research findings

The published paper states the 11 newly found galaxies are located relatively nearby, at redshifts of 0.028-0.258. The X-ray luminosities of these sources are within the range of 2 to 300 tredecillion erg/s, therefore typical for AGNs at the present epoch.

The spectrum of one of the new AGNs, designated SRGA J000132.9+240237, is described by a power law with a slope smaller than 0.5, which suggests a strong absorption and a significant contribution of the radiation reflected from the galaxy’s dusty torus. The authors of the paper noted that longer X-ray observations are required to determine the physical properties of this AGN.

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New Study Reveals Recent Ice Gains in Antarctica, But Long-Term Melting Continues

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New Study Reveals Recent Ice Gains in Antarctica, But Long-Term Melting Continues

Global warming and climate change have been subjects of major concern for a long time. One of the key indicators of this phenomenon is the melting of ice in the polar regions. Researchers from Tongji University in Shanghai have been using NASA satellite data to track changes in Antarctica’s ice sheet over more than two decades. Their newest study states that despite the increase in global temperature, Antarctica has gained ice in recent years. However, it cannot be considered as a miraculous reversal in global warming because over these two decades, the overall trend is substantial ice loss. Most of the gains have been caused by unusual increased precipitation over Antarctica.

About the New study

According to the new study , NASA’s Gravity Recovery And Climate Experiment (GRACE) and GRACE Follow-On satellites have been monitoring this ice sheet since 2002. The ice sheet covering Antarctica is the largest mass of ice on Earth

The satellite data revealed that the sheet experienced a sustained period of ice loss between 2002 and 2020. The ice loss accelerated in the latter half of that period, increasing from an average loss of about 81 billion tons (74 billion metric tons) per year between 2002 and 2010, to a loss of about 157 billion tons (142 billion metric tons) between 2011 and 2020, according to the study. However, the trend then shifted.

The ice sheet gained mass from 2021 to 2023 at an average rate of about 119 billion tons (108 metric tons) per year. Four glaciers in eastern Antarctica also flipped from accelerated ice loss to significant mass gain.

General Trend in global warming

Climate change doesn’t mean that everywhere on Earth will get hotter at the same rate, so a single region will never tell the whole story of our warming world.

Historically, temperatures over much of Antarctica have remained relatively stable, particularly compared to the Arctic. Antarctica’s sea ice has also been much more stable relative to the Arctic, but that’s been changing in recent years.

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