Kharagpur fire, April 2026 Kharagpur, Dharhara, Barhat
The fire started on 1 April 2026 in Kharagpur, India, and satellites saw it burning for 5 days. Copernicus’s global GWIS system rebuilt a burnt perimeter of 7,004 hectares from heat detections, spread across 3 municipalities.
It is the 9th largest in Bihār since 2016 (of 11 with a page). Number 30 in India in 2026, of 58.
The power measured by the satellite is low (10.6 MW in the strongest hotspot), more typical of grass or stubble burning, or a slow surface fire, than of a large crown fire.
Compare with…
Suggestions: Kharagpur · 2022Barhat · 2017
- Burnt area
- 7,004ha
- GWIS perimeter (Copernicus)
- Duration
- 5days
- 1 Apr 2026 – 5 Apr 2026
- Municipalities hit
- 3
- subdistricts
- Started on
- 1 Apr
- 2026
- Heat detections
- 69
- in a single hotspot: 11 MW
- Danger at start
- 18
- Moderate · FWI index
- Average daily power
- 43MW
- detected power per day, on average
Where it burned
How it evolved, day by day
Fire radiative power detected each day, in megawatts, and number of hotspots. The magenta bar marks the peak day.
The weather it burned in
It had gone 3 days without rain (1 mm or more) when it started.
This area had burned before
94% of the perimeter overlaps earlier fires recorded since 2016: 3,018 ha in 2016, 4,159 ha in 2017, 1,136 ha in 2018, 2,730 ha in 2019, 1,208 ha in 2020, 915 ha in 2021, 5,442 ha in 2022, 675 ha in 2023, 464 ha in 2024, 3,133 ha in 2025. Part of it burned more than once, so the yearly figures add up to more than the 6,571 ha that had burned before.
How big is it?
London boundary: geoBoundaries · Office for National Statistics (Open Government Licence v3.0).
Paris boundary: geoBoundaries · Institut national de l'information géographique et forestière (IGN-F) (Etalab Open License 2.0).
Madrid boundary: geoBoundaries · Open Data ESRI, IGN Central Registry of Cartography Area (CC BY 4.0).
Berlin boundary: geoBoundaries · Federal Agency for Cartography and Geodesy (dl-de/by-2-0).
This compares size, not location: both shapes are at the same scale, north up, centred on each other.
What happened to each town
-
Kharagpur where it started4,506 ha reached on 1 Apr13 %
-
2,367 ha reached on 1 Apr8.1 %
-
160 ha reached on 2 Apr0.7 %
Burnt area inside each municipality, from crossing the GWIS perimeter with administrative boundaries. The distance runs from the point marking the centre of each area to the nearest fire: staying a kilometre away does not mean it reached the houses.
People and buildings inside the perimeter
GHSL 2025Inside the perimeter there were about 0.94 hectares of built-up land and about 650 residents (GHSL 2025, satellite-based estimate).
This is an estimate on 100 m cells, made from satellite imagery and census data: it does not mean that homes burned or that anyone was harmed. The perimeter also contains land that never burned. The GHSL 2025 epoch is a projection made from 2020 and earlier data.
Source: Global Human Settlement Layer (GHS-BUILT-S and GHS-POP R2023A), European Commission Joint Research Centre (JRC), © European Union, CC BY 4.0. Sum inside the perimeter computed by WorldFires. human-settlement.emergency.copernicus.eu
The weather day by day
ECMWF ERA5 reanalysis at the fire location, the standard reference for past weather, and the Canadian Fire Weather Index (the same system Copernicus uses), computed by WorldFires from that data. Days after the fire run until the first rain.
Open-Meteo.com (CC BY 4.0) · Copernicus Climate Change Service (ERA5)
| Day | High | Min. humidity | Peak gust | Rain | Danger (FWI) |
|---|---|---|---|---|---|
| 25 Mar | 33.4 °C | 27 % | 29 km/h | 0.0 mm | Moderate 18 |
| 26 Mar | 33.9 °C | 26 % | 24 km/h | 0.0 mm | Moderate 18 |
| 27 Mar | 34.7 °C | 29 % | 27 km/h | 0.4 mm | Moderate 20 |
| 28 Mar | 29.0 °C | 48 % | 26 km/h | 2.9 mm | Very low 4 |
| 29 Mar | 30.2 °C | 54 % | 26 km/h | 0.4 mm | Low 9 |
| 30 Mar | 32.7 °C | 51 % | 27 km/h | 0.0 mm | Moderate 12 |
| 31 Mar | 33.3 °C | 49 % | 30 km/h | 1.7 mm | Low 8 |
| 1 Apr | 35.2 °C | 34 % | 38 km/h | 1.2 mm | Moderate 17 |
| 2 Apr | 36.2 °C | 31 % | 41 km/h | 0.0 mm | High 25 |
| 3 Apr | 37.8 °C | 28 % | 50 km/h | 0.0 mm | High 30 |
| 4 Apr | 36.6 °C | 28 % | 44 km/h | 0.0 mm | High 31 |
| 5 Apr | 33.3 °C | 31 % | 53 km/h | 0.0 mm | High 32 |
| 6 Apr after | 32.7 °C | 33 % | 32 km/h | 0.4 mm | High 26 |
| 7 Apr after | 34.8 °C | 24 % | 33 km/h | 0.2 mm | High 30 |
| 8 Apr after | 30.8 °C | 44 % | 32 km/h | 12.5 mm | Very low 3 |
| 9 Apr after | 30.7 °C | 49 % | 28 km/h | 0.6 mm | Low 8 |
| 10 Apr after | 32.3 °C | 22 % | 45 km/h | 0.0 mm | High 28 |
| 11 Apr after | 34.0 °C | 25 % | 32 km/h | 0.0 mm | High 25 |
| 12 Apr after | 36.0 °C | 23 % | 41 km/h | 0.0 mm | High 33 |
| 13 Apr after | 36.2 °C | 30 % | 32 km/h | 0.0 mm | High 30 |
| 14 Apr after | 36.0 °C | 19 % | 28 km/h | 0.0 mm | High 31 |
| 15 Apr after | 37.1 °C | 28 % | 34 km/h | 0.0 mm | High 36 |
| 16 Apr after | 32.7 °C | 61 % | 38 km/h | 0.0 mm | Moderate 20 |
| 17 Apr after | 36.2 °C | 41 % | 28 km/h | 0.0 mm | High 22 |
| 18 Apr after | 37.0 °C | 42 % | 33 km/h | 0.1 mm | High 27 |
| 19 Apr after | 35.6 °C | 49 % | 40 km/h | 0.0 mm | High 27 |
| 20 Apr after | 38.9 °C | 33 % | 33 km/h | 0.8 mm | High 32 |
Before and after, from space
Drag the line to compare the same ground before the fire and after it.
If the day is cloudy, change the date: each satellite passes once a day. In false colour the burnt ground looks brown or red.
The smoke
CAMS · CopernicusOn 30 March 2026 the air beside the fire reached 102 µg/m³ of PM2.5. That day averaged 78: 5.2 times the WHO daily guideline (15).
Particles from the Copernicus CAMS model at the centre of the perimeter; these are not measurements in each town. The pale bar is the worst hour, the solid one the daily average.
Open-Meteo.com (CC BY 4.0) · Copernicus Atmosphere Monitoring Service (CAMS)
Detections table · 69Every satellite heat detection, one by one, with time, satellite, power and coordinates.
| Date and time | Satellite | FRP (MW) | Lat | Lon |
|---|
Other fires nearby
Frequently asked questions
- How long did the Kharagpur fire last?
- GWIS (Copernicus) dates it between 1 April 2026 and 5 April 2026: 5 days between the first and last heat detection of the perimeter.
- How much area did it burn?
- The perimeter GWIS (Copernicus) rebuilt from heat detections is 7,004 hectares (70.0 km²). It is an estimate: official national figures may differ.
- Which municipalities burned?
- The fire entered 3 municipalities: Kharagpur (4,506 ha, 13 %); Dharhara (2,367 ha, 8.1 %); Barhat (160 ha, 0.7 %).
- What was the weather like?
- During the fire the temperature reached 37.8 °C, humidity dropped to 22 % and gusts hit 53 km/h. The fire danger index (FWI) reached 32, class High.
- Where does this data come from?
- From the GWIS (Copernicus) burnt perimeter, NASA FIRMS VIIRS hotspots and the administrative boundaries of India (geoBoundaries). It is not an official report.
Where to verify it
A satellite detection is not an official report. Final figures and the fire’s status are published by each country’s emergency service.
Emergency number: 112 · Emergency number and official warnings
Satellite cross-check
History of this page Changes in area, dates, name, official record or merged pages, compared every night since 24 October 2026.
No changes since 24 October 2026.
Does something look wrong on this page?
This page is built from satellite data and official records, and it sometimes gets things wrong: the wrong dates, the wrong town, two fires merged into one, or something that was not a wildfire at all. If you know this fire first-hand (you live nearby, saw it, fought it or reported on it), tell us what really happened and we will check it.
Report an error
How we know this
- Perimeter: GWIS (Copernicus), rebuilt from heat detections rather than mapped on imagery.
- Dates from the perimeter: the VIIRS detections inside it did not change them. 69 Suomi-NPP VIIRS detections on those dates.
- We have not matched this page with any official record.
- Weather: Copernicus ERA5 reanalysis at the fire location, in cells of about 25 km.
- Built-up area and population come from the JRC Global Human Settlement Layer (epoch 2025, 100 m cells), summed inside the perimeter: an estimate of what was there, not a damage count.
Where this data comes from
The perimeter comes from the Copernicus Global Wildfire Information System (GWIS), which rebuilds it from MODIS and VIIRS heat detections and publishes it under CC BY 4.0. It is not measured on imagery as in Europe, so it is an estimate. Heat detections come from the VIIRS sensors aboard Suomi-NPP and NOAA-20, distributed by NASA FIRMS at 375 m resolution. Municipal boundaries come from geoBoundaries ADM3 (Open Data Commons Open Database License 1.0). The area per municipality is computed by WorldFires by crossing the perimeter with those boundaries, so it may differ from each country’s official figure.