
Earth's largest camera will sweep the sky like never before
A top a mountain in Chile, where the days are dry and nights are clear, a team of scientists and engineers is preparing for one of the most important astronomical missions in recent times. Among them is
Kshitija Kelkar
, whose life has taken an interesting turn.
Twenty years ago in Pune, the city she's originally from, Kelkar sent a photo of a lunar eclipse she had taken with a digital camera to Sky and Telescope , a popular astronomy magazine. The publication accepted the photo and released it on its website under 'Photo of the Week'.
Inspired, Kelkar would turn astronomy into a career, and after degrees from Fergusson College, Pune University, University of Nottingham and doctoral work on how galaxies transform in their clusters, she arrived in Chile on a grant to use telescopes for her research.
by Taboola
by Taboola
Sponsored Links
Sponsored Links
Promoted Links
Promoted Links
You May Like
Providers are furious: Internet access without a subscription!
Techno Mag
Learn More
Undo
Today, years after that photo she took on a tiny camera, she's an observing specialist at the Vera C
Rubin
Observatory, looking at the sky through the largest digital camera ever assembled.
On June 23, that camera released a set of photos that stunned astronomers. Caught in unprecedented detail were galaxy clusters, distant stars and nebulae. In one photo, the camera — the size of a car with a resolution of 3.2 gigapixels — snapped a nebula around 4,000 light years away.
The Rubin observatory could even save Earth. In May, within just 10 hours, it found 2,104 previously undetected asteroids. Since its telescope takes images in quick succession, it's able to catch moving objects from the crowd of stars in the background that tend to stay in place. If even one space rock is headed our way, chances are first alerts would come from Rubin.
Humanity does have other powerful telescopes. There's
James Webb
, for instance, 1.5 million kilometres away from Earth with its own very dark sky. But it's mainly for zooming into specific targets. There's James Webb's predecessor, Hubble, currently in orbit over 500km above Earth. In 1995, it took Hubble nearly a week of long exposure to generate the now-famous Hubble Deep Field image, which showed about 3,000 very distant galaxies.
The Rubin Observatory, during its first test run in April, generated an image that revealed 10 million galaxies, in a matter of hours.
Part of the reason why it could do that is its very mission. Unlike James Webb and Hubble, which take in small parts of the sky, Rubin is a survey telescope, which means it shows the entire big picture, not specific objects. An image it takes covers a swathe of sky equivalent to 40 full moons — Webb's cameras show a size lesser than a full moon. A single photo from Rubin is so large, one would need 400 ultra-HD TV screens to see it in its full glory.
Large is ideal, given Rubin's purpose. Its primary optical instrument, named Simonyi Survey Telescope, is set to embark on a 10-year project called the Legacy Survey of Space and Time (LSST), to map the visible sky in extraordinary detail. The telescope is more than 300 tonnes of steel and glass, which is regularly cleaned using CO 2 . Over the next decade, this telescope and the giant LSST camera will take photos of the southern hemisphere sky, every 3-4 nights, to create the largest time-lapse film of the
Universe
ever made.
Why time-lapse? Imagine you're on the terrace of your building with a camera pointed at your neighbourhood. Time-lapse would reveal the windows that opened, the lights that came on, the cars and curtains that moved and the doors that opened.
Rubin observatory will do that to the Universe, find new objects and previously unknown interactions between them. 'We're going to be continuously taking 30-second images all night in different filters,' said Kelkar. 'And since we'll be observing the night sky every 30 seconds, in two back-to-back images of 15 seconds each, we'll catch any object that has changed its position or brightness.'
These objects may be stars, asteroids, unnamed comets and even potential sources of gravitational waves. This is where Kelkar said it would be unfair to compare Earth's telescopes — they're meant to complement each other, not compete.
Scientists, amateur astronomers and space enthusiasts the world over can sink their teeth into this data. 'People once thought the Earth was at the centre of the system. But then someone came along and said 'no, it's the Sun'. Similarly, we may find something absolutely mind-boggling, even evidence of life elsewhere,' Arvind Paranjpye, director of Nehru Planetarium in Mumbai, said.
Kelkar has been at Rubin for over a year, living in the town of
La Serena
— a twohour drive away. Her commute to work is through scenic valleys and along the 'El Camino de las Estrellas', or the 'Route to the Stars', because of the number of astronomical observatories along the way.
The route also needs light discipline, which means those driving there after dark cannot really use full-beam headlights. 'We usually have our hazard lights up,' said Kelkar. At the observatory, work begins shortly before sunset. After a check of all systems, by Kelkar and the rest of the observing specialists, they open Rubin's massive dome for night operations.
The observatory's placement atop the Cerro Pachón mountain puts it well above the localised turbulent layer where warm air mixes with cooler air from above, offering a clear view of the stars.
Right now, trials are on as crews perform final checks before Rubin, 20 years in the making with $800 million in construction costs, formally begins its survey later in 2025.
The Legacy Survey of Space and Time will be of unprecedented scale.
Remember that image Rubin released of 10 million galaxies? Well, they make up just 0.05% of nearly 20 billion galaxies the observatory will have imaged when LSST ends in a decade. Rubin may see millions of distant stars ending in supernovae and into new reaches of our own Milky Way galaxy.
Some 10 million alerts to scientists are expected from the observatory every night — whenever a change is detected in the series of photos it takes. Software will automatically compare new images with the stack of older ones. If an object has moved in those photos, flashed, exploded or streaked past, the software will detect the changes and dispatch an alert, all within minutes.
There's no other telescope that can do these things — detect real-time changes in the immediate sky and flashes of light from distant objects, and at such scale. In just one year, Rubin observatory will have detected more asteroids than all other telescopes combined.
There's more. The Simonyi Survey Telescope, set up on a special mount, is also fast. It can quickly swivel from one wide area of sky to another — within five seconds.
Nothing will miss this allseeing eye. Kelkar said word has already been sent out to experts worldwide to investigate the 2,104 newly detected asteroids. 'The telescope will be a game-changer,' she added, 'because we're giving a common dataset for all kinds of science at once. We don't need specialised observations. It's one data for all.'
Kelkar was in the control room at La Serena when the first images landed.
'Twenty years of people's professional lives had come down to that moment. We're about to make a 10-year movie of the night sky, with the fastest telescope and the biggest camera ever made. It's going to be fantastic,' she said.
LAST WEEK ' S QUICK QUIZ
Question on June 30: Challenging the belief that oxygen is produced only through photosynthesis, scientists have found polymetallic nodules deep in the ocean producing oxygen. What's this oxygen called? Answer: It's called 'dark' oxygen
Earth's Largest Camera Will Sweep The Sky Like Never Before
Hashtags

Try Our AI Features
Explore what Daily8 AI can do for you:
Comments
No comments yet...
Related Articles


Time of India
an hour ago
- Time of India
Scientists discover a 'second Earth' twice the size of our planet near a red dwarf star, 154 light-years away
In a significant step forward in the search for distant worlds, astronomers have discovered TOI-1846 b , a newly identified super-Earth exoplanet that may be rich in water. Located just 154 light-years away, this planet is nearly twice the size of Earth and orbits a cool red dwarf star . Though not considered habitable due to its high temperatures, TOI-1846 b's dense, water-rich composition and close orbit offer valuable insights into the formation and evolution of rocky planets beyond our solar system. The discovery was made using data from NASA's Transiting Exoplanet Survey Satellite (TESS) and confirmed with advanced ground-based observations. This planet adds to the growing catalogue of super-Earths that continue to reshape our understanding of planetary diversity in the galaxy. New super-Earth discovered orbiting red dwarf just 154 light-years away The new water-rich exoplanet , nearly twice the size of Earth, is orbiting a red dwarf star 154 light-years away. Named TOI-1846 b, this super-Earth may offer insights into the formation and evolution of rocky planets beyond our solar system. The discovery, detailed in a recent study published on the arXiv preprint server , was led by Abderahmane Soubkiou and his team at the Oukaimeden Observatory in Morocco. The planet was initially detected through NASA's Transiting Exoplanet Survey Satellite (TESS) and later confirmed using a combination of ground-based photometry, high-resolution imaging, and spectroscopy. by Taboola by Taboola Sponsored Links Sponsored Links Promoted Links Promoted Links You May Like Secure your family's future! ICICI Pru Life Insurance Plan Get Quote Undo TOI-1846 b: A water-rich super-Earth with extreme heat and close orbit According to the reports, TOI-1846 b has a radius of approximately 1.792 times that of Earth and is about 4.4 times more massive. It orbits its host star once every 3.93 days, indicating an extremely close and swift orbit. The planet's equilibrium temperature is estimated at 568.1 Kelvin (roughly 295°C), ruling out the possibility of surface habitability under known Earth-like conditions. Despite its high temperature, its size and density suggest a potentially water-rich composition, making it of interest to exoplanet researchers. This characteristic positions it among a growing class of rocky exoplanets that may contain substantial water content, possibly beneath thick atmospheres or layered beneath rocky crusts. How astronomers confirmed TOI-1846 b as a genuine super-Earth To validate the planet's existence, the team relied on a robust set of techniques: TESS data captured the planet's transits. Ground-based multicolor photometry helped refine its radius and orbital data. High-resolution imaging and spectroscopy confirmed that the transit signal was planetary in nature and not a false positive. These observations collectively confirmed that TOI-1846 b is a genuine super-Earth, orbiting a relatively small and cool red dwarf star. TOI-1846 b faces atmospheric study challenges due to low TSM score Researchers assessed the planet's Transmission Spectroscopy Metric (TSM) — a measure of how suitable a planet is for atmospheric study. TOI-1846 b scored a TSM of 47, which falls below the benchmark value of 90 typically used for sub-Neptune-sized planets. This suggests that its atmosphere may be challenging to analyze with current instruments. However, astronomers still consider TOI-1846 b a compelling candidate for future study, especially using radial velocity (RV) methods with high-precision instruments like MAROON-X. These observations could help refine its mass and reveal its internal structure and water content. TOI-1846 b vs HD 20794 d: How super-Earths differ in habitability and structure TOI-1846 b joins a growing catalog of recently discovered super-Earth exoplanets. For instance, earlier in 2025, astronomers identified HD 20794 d, a planet located just 20 light-years away, with a mass nearly six times that of Earth. Unlike TOI-1846 b, HD 20794 d lies within its star's habitable zone, although its elliptical orbit may complicate the possibility of stable surface water. While TOI-1846 b is too hot to support life, it remains a valuable case study for astronomers seeking to understand planetary composition , water retention, and the atmospheric evolution of rocky worlds. What TOI-1846 b could reveal about water-rich exoplanets Though not habitable, TOI-1846 b's possible water-rich interior, proximity to Earth, and detailed observational data make it a key object of interest. As telescope technology improves, particularly with next-gen observatories like the James Webb Space Telescope (JWST) and upcoming ground-based extremely large telescopes (ELTs), TOI-1846 b could play a role in shaping future models of planetary formation and composition. About the star orbiting around TOI-1846 The star around which TOI-1846 b orbits is a red dwarf, with just 42% the mass of our Sun and approximately 0.4 solar radii. It is estimated to be around 7.2 billion years old, making it older than the Sun. Its relatively cool effective temperature of 3,568 K is characteristic of low-mass stars, which are known to have long lifespans and stable radiation output — ideal for exoplanet detection missions. Also Read | Is your brain 15 seconds behind? Study reveals you're seeing the past, not the present


Time of India
2 hours ago
- Time of India
Forget about the dentist appointment: THIS vitamin can prevent tooth decay by 50%
A recent review of historical clinical trials reveals a significant link between vitamin D and a reduced incidence of tooth decay, showing a potential 50% reduction in dental caries. The research, analyzing studies from the 1920s to 1980s, highlights vitamin D's crucial role in dental health, particularly for children. Getting a dentist appointment these days is not easy, let alone the money you have to spend to fix issues. Tooth decay is one of the most common dental problems that affects children and adults alike. But the treatment does not have to cost you an arm and a leg. What if tooth decay could be prevented with a simple, affordable nutrient? A study has found a link between tooth decay and vitamin deficiency. A review of historical clinical trials found that a certain vitamin lowers the rate of tooth decay. The study is published in Nutrition Reviews . Link between tooth decay and vitamin D The review found that vitamin D was linked with a 50 percent reduction in the incidence of dental caries. To understand the link between vitamin D and tooth decay, the researchers reviewed 24 controlled clinical trials, spanning the 1920s to the 1980s, on approximately 3,000 children in several countries. These trials pointed out that vitamin D was associated with an approximately 50 percent reduction in the incidence of tooth decay. "My main goal was to summarize the clinical trial database so that we could take a fresh look at this vitamin D question," Dr. by Taboola by Taboola Sponsored Links Sponsored Links Promoted Links Promoted Links You May Like 2025 Top Trending local enterprise accounting software [Click Here] Esseps Learn More Undo Philippe Hujoel of the University of Washington, who conducted the review, said. What is vitamin D Vitamin D, also known as the 'sunshine vitamin,' is an essential nutrient. It is a fat-soluble nutrient that plays a crucial role in the body. From maintaining bone health, immune function, and mood regulation, vitamin D helps in many vital functions. Our body can naturally produce vitamin D when exposed to sunlight. When the skin is exposed to sunlight, it naturally makes vitamin D from cholesterol. The sun's ultraviolet B (UVB) rays interact with the cholesterol in skin cells and trigger the process of vitamin D synthesis. You can also get this nutrient from foods such as fatty fish (salmon, mackerel), egg yolks, and fortified foods (milk, orange juice). Vitamin D's role in preventing caries (Pic courtesy: iStock) Though vitamin D's role in supporting bone health has not been disputed, there has been a significant disagreement over its role in preventing caries, Hujoel noted. In 1950, the American Medical Association and the US National Research Council concluded that vitamin D was beneficial in managing dental caries. Later in 1989, the National Research Council, despite new evidence supporting vitamin D's caries-fighting benefits, called the issue 'unresolved. ' "Such inconsistent conclusions by different organizations do not make much sense from an evidence-based perspective," Hujoel said. The trials the team reviewed had increased vitamin D levels in children through UV radiation or by diet (cod liver oil or other products containing the vitamin). The trials they reviewed were conducted in the United States, Great Britain, Canada, Austria, New Zealand, and Sweden, and were held in institutional settings, schools, medical and dental practices, or hospitals. The participants were children or young adults between the ages of 2 and 16 years, with a weighted mean age of 10 years. 'Pretty Little Baby' Singer Connie Francis Hospitalised, Family Gives Health Update The findings from the University of Washington reaffirm the importance of vitamin D for dental health. Children who are vitamin D deficient have poor and delayed teeth eruption and are prone to dental caries,' Dr. Michael Hollick, professor of medicine at the Boston University Medical Center said. Studies have also found that Vitamin D deficiency is linked to dental caries in young children. "Whether this is more than just a coincidence is open to debate. In the meantime, pregnant women or young mothers can do little harm by realizing that vitamin D is essential to their offspring's health. Vitamin D does lead to teeth and bones that are better mineralized," Hujoel said. "One has to be careful with the interpretation of this systematic review. The trials had weaknesses which could have biased the result, and most of the trial participants lived in an era that differs profoundly from today's environment,' Hujoel added.


Time of India
6 hours ago
- Time of India
Earth's largest camera will sweep the sky like never before
The LSST Camera A top a mountain in Chile, where the days are dry and nights are clear, a team of scientists and engineers is preparing for one of the most important astronomical missions in recent times. Among them is Kshitija Kelkar , whose life has taken an interesting turn. Twenty years ago in Pune, the city she's originally from, Kelkar sent a photo of a lunar eclipse she had taken with a digital camera to Sky and Telescope , a popular astronomy magazine. The publication accepted the photo and released it on its website under 'Photo of the Week'. Inspired, Kelkar would turn astronomy into a career, and after degrees from Fergusson College, Pune University, University of Nottingham and doctoral work on how galaxies transform in their clusters, she arrived in Chile on a grant to use telescopes for her research. by Taboola by Taboola Sponsored Links Sponsored Links Promoted Links Promoted Links You May Like Providers are furious: Internet access without a subscription! Techno Mag Learn More Undo Today, years after that photo she took on a tiny camera, she's an observing specialist at the Vera C Rubin Observatory, looking at the sky through the largest digital camera ever assembled. On June 23, that camera released a set of photos that stunned astronomers. Caught in unprecedented detail were galaxy clusters, distant stars and nebulae. In one photo, the camera — the size of a car with a resolution of 3.2 gigapixels — snapped a nebula around 4,000 light years away. The Rubin observatory could even save Earth. In May, within just 10 hours, it found 2,104 previously undetected asteroids. Since its telescope takes images in quick succession, it's able to catch moving objects from the crowd of stars in the background that tend to stay in place. If even one space rock is headed our way, chances are first alerts would come from Rubin. Humanity does have other powerful telescopes. There's James Webb , for instance, 1.5 million kilometres away from Earth with its own very dark sky. But it's mainly for zooming into specific targets. There's James Webb's predecessor, Hubble, currently in orbit over 500km above Earth. In 1995, it took Hubble nearly a week of long exposure to generate the now-famous Hubble Deep Field image, which showed about 3,000 very distant galaxies. The Rubin Observatory, during its first test run in April, generated an image that revealed 10 million galaxies, in a matter of hours. Part of the reason why it could do that is its very mission. Unlike James Webb and Hubble, which take in small parts of the sky, Rubin is a survey telescope, which means it shows the entire big picture, not specific objects. An image it takes covers a swathe of sky equivalent to 40 full moons — Webb's cameras show a size lesser than a full moon. A single photo from Rubin is so large, one would need 400 ultra-HD TV screens to see it in its full glory. Large is ideal, given Rubin's purpose. Its primary optical instrument, named Simonyi Survey Telescope, is set to embark on a 10-year project called the Legacy Survey of Space and Time (LSST), to map the visible sky in extraordinary detail. The telescope is more than 300 tonnes of steel and glass, which is regularly cleaned using CO 2 . Over the next decade, this telescope and the giant LSST camera will take photos of the southern hemisphere sky, every 3-4 nights, to create the largest time-lapse film of the Universe ever made. Why time-lapse? Imagine you're on the terrace of your building with a camera pointed at your neighbourhood. Time-lapse would reveal the windows that opened, the lights that came on, the cars and curtains that moved and the doors that opened. Rubin observatory will do that to the Universe, find new objects and previously unknown interactions between them. 'We're going to be continuously taking 30-second images all night in different filters,' said Kelkar. 'And since we'll be observing the night sky every 30 seconds, in two back-to-back images of 15 seconds each, we'll catch any object that has changed its position or brightness.' These objects may be stars, asteroids, unnamed comets and even potential sources of gravitational waves. This is where Kelkar said it would be unfair to compare Earth's telescopes — they're meant to complement each other, not compete. Scientists, amateur astronomers and space enthusiasts the world over can sink their teeth into this data. 'People once thought the Earth was at the centre of the system. But then someone came along and said 'no, it's the Sun'. Similarly, we may find something absolutely mind-boggling, even evidence of life elsewhere,' Arvind Paranjpye, director of Nehru Planetarium in Mumbai, said. Kelkar has been at Rubin for over a year, living in the town of La Serena — a twohour drive away. Her commute to work is through scenic valleys and along the 'El Camino de las Estrellas', or the 'Route to the Stars', because of the number of astronomical observatories along the way. The route also needs light discipline, which means those driving there after dark cannot really use full-beam headlights. 'We usually have our hazard lights up,' said Kelkar. At the observatory, work begins shortly before sunset. After a check of all systems, by Kelkar and the rest of the observing specialists, they open Rubin's massive dome for night operations. The observatory's placement atop the Cerro Pachón mountain puts it well above the localised turbulent layer where warm air mixes with cooler air from above, offering a clear view of the stars. Right now, trials are on as crews perform final checks before Rubin, 20 years in the making with $800 million in construction costs, formally begins its survey later in 2025. The Legacy Survey of Space and Time will be of unprecedented scale. Remember that image Rubin released of 10 million galaxies? Well, they make up just 0.05% of nearly 20 billion galaxies the observatory will have imaged when LSST ends in a decade. Rubin may see millions of distant stars ending in supernovae and into new reaches of our own Milky Way galaxy. Some 10 million alerts to scientists are expected from the observatory every night — whenever a change is detected in the series of photos it takes. Software will automatically compare new images with the stack of older ones. If an object has moved in those photos, flashed, exploded or streaked past, the software will detect the changes and dispatch an alert, all within minutes. There's no other telescope that can do these things — detect real-time changes in the immediate sky and flashes of light from distant objects, and at such scale. In just one year, Rubin observatory will have detected more asteroids than all other telescopes combined. There's more. The Simonyi Survey Telescope, set up on a special mount, is also fast. It can quickly swivel from one wide area of sky to another — within five seconds. Nothing will miss this allseeing eye. Kelkar said word has already been sent out to experts worldwide to investigate the 2,104 newly detected asteroids. 'The telescope will be a game-changer,' she added, 'because we're giving a common dataset for all kinds of science at once. We don't need specialised observations. It's one data for all.' Kelkar was in the control room at La Serena when the first images landed. 'Twenty years of people's professional lives had come down to that moment. We're about to make a 10-year movie of the night sky, with the fastest telescope and the biggest camera ever made. It's going to be fantastic,' she said. LAST WEEK ' S QUICK QUIZ Question on June 30: Challenging the belief that oxygen is produced only through photosynthesis, scientists have found polymetallic nodules deep in the ocean producing oxygen. What's this oxygen called? Answer: It's called 'dark' oxygen Earth's Largest Camera Will Sweep The Sky Like Never Before