Archivo de la etiqueta: Astronomy

New Timing for Stubble Burning in India

Every year for decades, long rivers of smoke and haze have spread across the Indo-Gangetic Plain in northern India from October to December. That’s when farmers in Punjab, Haryana, Uttar Pradesh, Madhya Pradesh, and other states burn off plant “stubble” after the rice harvest.

When winds are weak and the atmosphere becomes stagnant, the haze can push levels of air pollution several times higher than limits recommended by the World Health Organization. Smoke typically mixes with particles and gases from other sources, such as industry, vehicles, domestic fires (heating and cooking), fireworks, and dust storms, to form the haze, though scientists consider stubble burning to be a major factor.

In some ways, the seasonal timing of stubble fires in 2025 followed typical patterns. Air quality deteriorated in Delhi and several other cities for about a month after crop fires intensified during the last week of October, explained Hiren Jethva, a Morgan State University atmospheric scientist based at NASA’s Goddard Space Flight Center. For about a decade, Jethva has tracked the stubble burning season in India using satellites, and has made predictions about the intensity of the upcoming fire season based on vegetation observations.  

The MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Aqua satellite captured this image of a smoky haze darkening skies over much of the plain on November 11, 2025. According to news reports, it was the first of several days in 2025 when pollution levels exceeded 400 on India’s air quality index, the strongest rating on the scale. As in past years, the poor air quality prompted officials in some areas to close schools and institute more stringent air quality controls on construction.

However, the daily timing of burning departs from what Jethva has seen in the past. He started tracking the number of fires years ago by primarily tallying observations from MODIS—which pass over locations on Earth each morning and afternoon on the Terra and Aqua satellites, respectively. Then, most fires were lit in the early afternoon between 1 p.m. and 2 p.m. local time.

But in the past few years, stubble fires have occurred progressively later in the day, Jethva said. He identified the shift by analyzing observations from GEO-KOMPSAT-2A, a South Korean geostationary satellite launched in late 2018 that collects data every 10 minutes.

Most stubble fires now happen between 4 p.m. and 6 p.m., he said, meaning that fire-monitoring systems that rely solely on MODIS, or similar sensors like VIIRS (Visible Infrared Imaging Radiometer Suite), miss many of the fires. “Farmers have changed their behavior,” he said.

His analysis of GEO-KOMPSAT-2A observations indicates that the stubble burning activity in Punjab and Haryana was moderate in 2025 compared to other recent years. This year had higher numbers of fires compared to 2024, 2020, and 2019 but fewer fires than 2023, 2022, and 2021, he found.

Indian Space Research Organization researchers have also pointed out the shift in the timing of stubble burning. In a Current Science study published in 2025, one group reported that MSG (Meteosat Second Generation) satellite observations showed a shift in peak fire activity from about 1:30 p.m. in 2020 to about 5:00 p.m. in 2024. In December 2025, researchers with the International Forum for Environment, Sustainability, & Technology (iForest) released a multi-satellite analysis that came to a similar conclusion.

Meanwhile, parsing out precisely how much stubble fires contribute to poor air quality in Delhi compared to other sources of pollution remains a topic of active study and debate among scientists. “Studies report contributions ranging from 10 to 50 percent,” said Pawan Gupta, a NASA research scientist who specializes in air quality.

Gupta estimates that the stubble burning contribution ranges from 40 to 70 percent on a given day, dropping to 20 to 30 percent if averaged over a month or burning season, and under 10 percent if averaged annually. “Meteorological conditions—like a shallow boundary layer height and low temperature—during the burning season add extra complexity,” he said.

The timing of the fires may influence the degree to which stubble burning affects air quality. Some modeling research suggests that evening fires may lead to a stronger overnight buildup of particle pollution than early-afternoon fires because the planetary boundary layer, the lowest part of the atmosphere, tends to be shallower and have weaker winds at night, allowing pollutants to accumulate.

NASA Earth Observatory image by Michala Garrison, using MODIS data from NASA EOSDIS LANCE and GIBS/Worldview. Story by Adam Voiland.

References and Resources

• Biswal, A., et al. (2025) Emission time and amount of crop residue burning play critical role on PM_2.5 variability during October–November in northwestern India during 2022–2024. Environmental Science: Atmospheres, 11.
• Burki, T. (2025) Stubble: The Farmer’s Bane. The Lancet Respiratory Medicine, 13(2), 207.
• The Deccan Herald (2025, December 8) Punjab, Haryana farmers change stubble burning time window to avoid satellite detection. Accessed December 9, 2025.
• Down to Earth (2025, November 26) Why has Madhya Pradesh burnt more paddy stubble for the second year in a row? Accessed December 9, 2025.
• Jethva, H., et al. (2019) Connecting Crop Productivity, Residue Fires, and Air Quality over Northern India. Scientific Reports, 9, 16594.
• Ministry of Environment, Forest and Climate Change (2025, December 1) Paddy Harvesting Season 2025 concludes with significant Reduction in Farm Fire Incidents across Punjab and Haryana. Accessed December 9, 2025.
• NASA (2024, October 18) What is Air Quality? Accessed December 9, 2025.
• NASA Earth Observatory (2020, November 17) A Busy Season for Crop Fires in Northwestern India. Accessed December 9, 2025.
• NASA Earth Observatory (2025, January 22) Is Fire Activity Declining in Northwestern India? Accessed December 9, 2025.
• NDTV (2025, December 1) Stubble Burning Down By 90% In Punjab, Haryana, Centre Informs Parliament. Accessed December 9, 2025.
• NDTV (2025, December 9) Farm Fires Didn’t End, They Just Moved To Afternoon: Satellite Data Analysis. Accessed December 9, 2025.
• The New Indian Express (2025, November 11) AQI spikes to 428 in first ‘severe’ air day of this year, GRAP-III invoked in capital. Accessed December 9, 2025.
• Singh, N., et al. (2025) Evidence of shift in stubble burning timing over northwest India from geostationary satellite observations. Current Science, 129(10), 921-923.
• The Times of India (2025, December 6) Stubble burning cases jump by 18% in UP this year. Accessed December 9, 2025.

Downloads

November 11, 2025

JPEG (2.90 MB)

You may also be interested in:

Stay up-to-date with the latest content from NASA as we explore the universe and discover more about our home planet.

Widespread Smoke from Canadian Fires

3 min read

Fires burning in boreal forests created hazy skies across North America in summer 2025.

Article

Seeing the Monroe Canyon Fire in a New Light

5 min read

As wildland fires raged in the American West, NASA airborne technology was there to image it in incredible detail.

Article

B.C. Wildfires Send Smoke Skyward

2 min read

Lightning likely ignited several large fires that sent smoke pouring over the Canadian province in early September 2025.

Article

Keep Exploring

Discover More from NASA Earth Science

Subscribe to Earth Observatory Newsletters

Subscribe to the Earth Observatory and get the Earth in your inbox.

Earth Observatory Image of the Day

NASA’s Earth Observatory brings you the Earth, every day, with in-depth stories and stunning imagery.

Explore Earth Science

Earth Science Data

Powered by WPeMatico

Get The Details…

NASA Astronaut Jonny Kim to Discuss Eight-Month Space Station Mission

NASA astronaut Jonny Kim will recap his recent mission aboard the International Space Station during a news conference at 3:30 p.m. EST Friday, Dec. 19, from the agency’s Johnson Space Center in Houston.

Watch the news conference live on NASA’s YouTube channel. Learn how to stream NASA content through a variety of online platforms, including social media.

Media interested in participating in person must contact the NASA Johnson newsroom no later than 5 p.m. Thursday, Dec. 18, at 281-483-5111 or jsccommu@mail.nasa.gov.

Media wishing to participate by phone must contact the Johnson newsroom no later than two hours before the start of the event. To ask questions by phone, media must dial into the news conference no later than 15 minutes prior to the start of the call. NASA’s media accreditation policy is available online.

Kim returned to Earth on Dec. 9, along with Roscosmos cosmonauts Sergey Ryzhikov and Alexey Zubritsky. He logged 245 days as an Expedition 72/73 flight engineer during his first spaceflight. The trio completed 3,920 orbits of the Earth over the course of their nearly 104-million-mile journey. They also saw the arrival of nine visiting spacecraft and the departure of six.

During his mission, Kim contributed to a wide range of scientific investigations and technology demonstrations. He studied the behavior of bioprinted tissues containing blood vessels in microgravity for an experiment helping advance space-based tissue production to treat patients on Earth. He also evaluated the remote command of multiple robots in space for the Surface Avatar study, which could support the development of robotic assistants for future exploration missions. Additionally, Kim worked on developing in-space manufacturing of DNA-mimicking nanomaterials, which could improve drug delivery technologies and support emerging therapeutics and regenerative medicine. 

Learn more about International Space Station research and operations at:

http://www.nasa.gov/station

-end-

Jimi Russell
Headquarters, Washington
202-358-1100
james.j.russell@nasa.gov

Shaneequa Vereen
Johnson Space Center, Houston
281-483-5111
shaneequa.y.vereen@nasa.gov

Powered by WPeMatico

Get The Details…
Jessica Taveau

NASA’s Webb, Curiosity Named in TIME’s Best Inventions Hall of Fame

Two icons of discovery, NASA’s James Webb Space Telescope and NASA’s Curiosity rover, have earned places in TIME’s “Best Inventions Hall of Fame,” which recognizes the 25 groundbreaking inventions of the past quarter century that have had the most global impact, since TIME began its annual Best Inventions list in 2000. The inventions are celebrated in TIME’s December print issue.

“NASA does the impossible every day, and it starts with the visionary science that propels humanity farther than ever before,” said Nicky Fox, associate administrator, Science Mission Directorate, NASA Headquarters in Washington. “Congratulations to the teams who made the world’s great engineering feats, the James Webb Space Telescope and the Mars Curiosity Rover, a reality. Through their work, distant galaxies feel closer, and the red sands of Mars are more familiar, as they expanded and redefined the bounds of human achievement in the cosmos for the benefit of all.”

Decades in the making and operating a million miles from Earth, Webb is the most powerful space telescope ever built, giving humanity breathtaking views of newborn stars, distant galaxies, and even planets orbiting other stars. The new technologies developed to enable Webb’s science goals – from optics to detectors to thermal control systems – now also touch Americans’ everyday lives, improving manufacturing for everything from high-end cameras and contact lenses to advanced semiconductors and inspections of aircraft engine components.

Meanwhile on Mars, the unstoppable Curiosity rover, NASA’s car-size science lab, has spent more than a decade uncovering clues that the Red Planet once could have supported life, transforming our understanding of our planetary neighbor. These NASA missions continue to make breakthroughs that have reshaped our understanding of the universe and our place in it. Curiosity has also paved the way for future astronauts: Its Radiation Assessment Detector has studied the Martian radiation environment for nearly 14 years, and its unforgettable landing by robotic jetpack allowed heavier spacecraft to touch down on the surface — a capability that will be needed to send cargo and humans to Mars.

To compile this “Hall of Fame” list, TIME solicited nominations from TIME editors and correspondents around the world, paying special attention to high-impact fields, such as health care and technology. TIME then evaluated each contender on a number of key factors, including originality, continued efficacy, ambition, and impact.

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).

The Curiosity rover was built by NASA’s Jet Propulsion Laboratory, which is managed by Caltech in Pasadena, California. JPL leads the mission on behalf of NASA’s Science Mission Directorate in Washington as part of NASA’s Mars Exploration Program portfolio.

To learn more about NASA’s science missions, visit:

https://science.nasa.gov

Keep Exploring

Discover More Topics From NASA

Explore NASA Science Activities

James Webb Space Telescope

Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…

Mars Science Laboratory: Curiosity Rover

Part of NASA’s Mars Science Laboratory mission, at the time of launch, Curiosity was the largest and most capable rover…

Science Missions

Powered by WPeMatico

Get The Details…

A Rare Gourd

NASA’s Hubble Space Telescope captured an uncommon sight – the death of a low-mass star – in this image of the Calabash Nebula released on Feb. 3, 2017.

Here, we can see the star going through a rapid transformation from a red giant to a planetary nebula, during which it blows its outer layers of gas and dust out into the surrounding space. The recently ejected material is spat out in opposite directions with immense speed — the gas shown in yellow is moving close to a million kilometers an hour.

Astronomers rarely capture a star in this phase of its evolution because it occurs within the blink of an eye – in astronomical terms. Over the next thousand years the nebula is expected to evolve into a fully-fledged planetary nebula.

Powered by WPeMatico

Get The Details…
Gary Daines

NASA Announces Plan to Map Milky Way With Roman Space Telescope

NASA’s Nancy Grace Roman Space Telescope team has released detailed plans for a major survey that will reveal our home galaxy, the Milky Way, in unprecedented detail. In one month of observations spread across two years, the survey will unveil tens of billions of stars and explore previously uncharted structures.

“The Galactic Plane Survey will revolutionize our understanding of the Milky Way,” said Julie McEnery, Roman’s senior project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “We’ll be able to explore the mysterious far side of our galaxy and its star-studded heart. Because of the survey’s breadth and depth, it will be a scientific mother lode.”

The Galactic Plane Survey is Roman’s first selected general astrophysics survey — one of many observation programs Roman will do in addition to its three core surveys and Coronagraph technology demonstration. At least 25% of Roman’s five-year primary mission is reserved for astronomers worldwide to propose more surveys beyond the core programs, fully leveraging Roman’s capabilities to conduct groundbreaking science. Roman is slated to launch by May 2027, but the team is on track for launch as early as fall 2026.

While ESA’s (European Space Agency’s) retired Gaia spacecraft mapped around 2 billion Milky Way stars in visible light, many parts of the galaxy remain hidden by dust. By surveying in infrared light, Roman will use powerful heat vision that can pierce this veil to see what lies beyond.

“It blows my mind that we will be able to see through the densest part of our galaxy and explore it properly for the first time,” said Rachel Street, a senior scientist at Las Cumbres Observatory in Santa Barbara, California, and a co-chair of the committee that selected the Galactic Plane Survey design.

The survey will cover nearly 700 square degrees (a region of sky as large as about 3,500 full moons) along the glowing band of the Milky Way — our edge-on view of the disk-shaped structure containing most of our galaxy’s stars, gas, and dust. Scientists expect the survey to map up to 20 billion stars and detect tiny shifts in their positions with repeated high-resolution observations. And it will only take 29 days spread over the course of the mission’s first two years.

Cosmic Cradles

Stars are born from parent clouds of gas and dust. Roman will peer through the haze of these nesting grounds to see millions of stellar embryos, newborn stars still swaddled in shrouds of dust, tantrumming toddler stars that flare unpredictably, and young stars that may have planetary systems forming around them. Astronomers will study stellar birth rates across a wide range of masses and stitch together videos that show how stars change over time.

“This survey will study such a huge number of stars in so many different stellar environments that we’ll be sampling every phase of a star’s evolution,” Street said.

Observing so many stars in various stages of early development will shed light on the forces that shape them. Star formation is like a four way tug-of-war between gravity, radiation, magnetism, and turbulence. Roman will help us study how these forces influence whether gas clouds collapse into full-fledged stars, smaller brown dwarfs — in-between objects that are much heavier than planets but not massive enough to ignite like stars — or new worlds.

Some stars are born in enormous litters called clusters. Roman will study nearly 2,000 young, loosely bound open clusters to see how the galaxy’s spiral arms trigger star formation. The survey will also map dozens of ancient, densely packed globular clusters near the center of the galaxy that could help astronomers reconstruct the Milky Way’s early history.

Comparing Roman’s snapshots of clusters scattered throughout the galaxy will enable scientists to study nature versus nurture on a cosmic scale. Because a cluster’s stars generally share the same age, origin, and chemical makeup, analyzing them allows astronomers to isolate environmental effects very precisely.

Pulse Check

When they run out of fuel, Sun-like stars leave behind cores called white dwarfs and heavier stars collapse to form neutron stars and black holes. Roman will find these stellar embers even when they’re alone thanks to wrinkles in space-time.

Anything that has mass warps the underlying fabric of the universe. When light from a background star passes through the gravitational well around an intervening object on its journey toward Earth, its path slightly curves around the object. This phenomenon, called microlensing, can temporarily brighten the star. By studying these signals, astronomers can learn the mass and size of otherwise invisible foreground objects.

A separate survey — Roman’s Galactic Bulge Time-Domain Survey — will conduct deep microlensing observations over a smaller area in the heart of the Milky Way. The Galactic Plane Survey will conduct repeated observations over a shorter interval but across the whole center of the galaxy, giving us the first complete view of this complex galactic environment. An unobscured view of the galaxy’s central bar will help astronomers answer the question of its origin, and Roman’s videos of stars in this region will enable us to study some ultratight binary objects at the very ends of their lives thanks to their interactions with close companions.

“Compact binaries are particularly interesting because they’re precursors to gravitational-wave sources,” said Robert Benjamin, a visiting professor at the University of Wisconsin-Whitewater, and a co-chair of the committee that selected the Galactic Plane Survey design. When neutron stars and black holes merge, the collision is so powerful that it sends ripples through the fabric of space-time. “Scientists want to know more about the pathways that lead to those mergers.”

optical

infrared

opticalinfrared

optical

infrared

Optical vs infrared

Two Views

CurtainToggle2-Up

Image Details

The Galactic Plane Survey by NASA’s Nancy Grace Roman Space Telescope will scan the densest part of our galaxy, where most of its stars, gas, and dust reside — the most difficult region to study from our place inside the Milky Way since we have to look through so much light-blocking material. Roman’s wide field of view, crisp resolution, and infrared vision will help astronomers peer through thick bands of dust to chart new galactic territory. Credit: NASA, ESA, and STScI

Roman’s repeated observations will also monitor stars that flicker. Ground-based surveys detect thousands of bright stellar outbursts, but often can’t see the faint, dust-obscured stars that produce them. Roman will pinpoint the culprits plus take high-resolution snapshots of the aftermath.

Some stars throb rhythmically, and the speed of their pulsing is directly linked to their intrinsic brightness. By comparing their true brightness to how bright they appear from Earth, astronomers can measure distances across the galaxy. Roman will find these blinking stars farther away than ever before and track them over time, helping astronomers improve their cosmic measuring sticks.

“Pairing Roman’s Galactic Plane Survey with other Milky Way observations will create the best portrait of the galaxy we’ve ever had,” Benjamin said.

Download additional images and video from NASA’s Scientific Visualization Studio.

For more information about the Roman Space Telescope, visit:

https://www.nasa.gov/roman

By Ashley Balzer
NASA’s Goddard Space Flight Center, Greenbelt, Md.

Media contact:

Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, Md.
301-286-1940

Explore More

6 min read

NASA’s Roman Mission Shares Detailed Plans to Scour Skies

Article


8 months ago

8 min read

NASA Completes Nancy Grace Roman Space Telescope Construction

Article


1 week ago

7 min read

One Survey by NASA’s Roman Could Unveil 100,000 Cosmic Explosions

Article


5 months ago

Powered by WPeMatico

Get The Details…
Ashley Balzer