Peshrar fire, March 2017 Peshrar, Bishunpur, Latehar
The fire started on 27 March 2017 in Peshrar, India, and satellites saw it burning for 9 days. Copernicus’s global GWIS system rebuilt a burnt perimeter of 12,816 hectares from heat detections, spread across 3 municipalities.
Number 4 in India in 2017, of 27.
The power measured by the satellite is low (26.5 MW in the strongest hotspot), more typical of grass or stubble burning, or a slow surface fire, than of a large crown fire.
- Burnt area
- 12,816ha
- GWIS perimeter (Copernicus)
- Duration
- 9days
- 27 Mar 2017 – 4 Apr 2017
- Municipalities hit
- 3
- subdistricts
- Started on
- 27 Mar
- 2017
- Heat detections
- 487
- in a single hotspot: 27 MW
- Danger at start
- 28
- High · FWI index
- Energy released
- 1.9GW
- sum of detected power
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 10 days without rain (1 mm or more) when it started. Rain came after the fire: 1.1 mm on 21 Apr.
This area had burned before
20% of the perimeter overlaps earlier fires recorded since 2016: 2,536 ha in 2016.
What happened to each town
-
Peshrar where it started6,711 ha reached on 27 Mar19 %
-
5,377 ha reached on 27 Mar8.8 %
-
791 ha reached on 30 Mar1.6 %
Burnt area inside each municipality, from crossing the GWIS perimeter with administrative boundaries. The distance is from the town centre to the nearest fire: staying a kilometre away does not mean it reached the houses.
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) |
|---|---|---|---|---|---|
| 22 Mar | 30.1 °C | 26 % | 43 km/h | 0.0 mm | High 28 |
| 23 Mar | 32.1 °C | 24 % | 45 km/h | 0.0 mm | High 30 |
| 24 Mar | 33.3 °C | 23 % | 46 km/h | 0.0 mm | High 32 |
| 25 Mar | 34.5 °C | 21 % | 42 km/h | 0.0 mm | High 34 |
| 26 Mar | 33.2 °C | 19 % | 46 km/h | 0.0 mm | High 37 |
| 27 Mar | 33.6 °C | 20 % | 40 km/h | 0.0 mm | High 35 |
| 28 Mar | 33.9 °C | 24 % | 52 km/h | 0.0 mm | Very high 40 |
| 29 Mar | 34.9 °C | 18 % | 56 km/h | 0.0 mm | Very high 44 |
| 30 Mar | 36.4 °C | 15 % | 52 km/h | 0.0 mm | Very high 47 |
| 31 Mar | 36.0 °C | 18 % | 44 km/h | 0.0 mm | Very high 43 |
| 1 Apr | 35.8 °C | 16 % | 53 km/h | 0.0 mm | Very high 49 |
| 2 Apr | 35.9 °C | 17 % | 45 km/h | 0.0 mm | Very high 46 |
| 3 Apr | 35.3 °C | 18 % | 40 km/h | 0.0 mm | Very high 46 |
| 4 Apr | 36.2 °C | 19 % | 34 km/h | 0.0 mm | Very high 42 |
| 5 Apr after | 35.6 °C | 23 % | 41 km/h | 0.0 mm | Very high 46 |
| 6 Apr after | 35.9 °C | 25 % | 31 km/h | 0.0 mm | Very high 42 |
| 7 Apr after | 37.1 °C | 18 % | 29 km/h | 0.0 mm | Very high 39 |
| 8 Apr after | 36.5 °C | 22 % | 34 km/h | 0.0 mm | Very high 44 |
| 9 Apr after | 33.7 °C | 18 % | 36 km/h | 0.0 mm | Very high 44 |
| 10 Apr after | 32.4 °C | 12 % | 47 km/h | 0.0 mm | Extreme 52 |
| 11 Apr after | 33.3 °C | 12 % | 47 km/h | 0.0 mm | Extreme 53 |
| 12 Apr after | 34.7 °C | 12 % | 38 km/h | 0.0 mm | Very high 49 |
| 13 Apr after | 36.1 °C | 13 % | 32 km/h | 0.0 mm | Very high 48 |
| 14 Apr after | 36.1 °C | 13 % | 35 km/h | 0.0 mm | Very high 49 |
| 15 Apr after | 35.8 °C | 14 % | 54 km/h | 0.0 mm | Extreme 58 |
| 16 Apr after | 34.0 °C | 20 % | 45 km/h | 0.0 mm | Extreme 51 |
| 17 Apr after | 35.2 °C | 26 % | 29 km/h | 0.0 mm | Very high 42 |
| 18 Apr after | 36.7 °C | 24 % | 41 km/h | 0.0 mm | Very high 46 |
| 19 Apr after | 38.2 °C | 13 % | 44 km/h | 0.5 mm | Extreme 54 |
| 20 Apr after | 36.0 °C | 16 % | 41 km/h | 0.0 mm | Extreme 54 |
| 21 Apr after | 37.3 °C | 19 % | 49 km/h | 1.1 mm | Very high 46 |
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.
Detections table · 487Every 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 Peshrar fire last?
- GWIS (Copernicus) dates it between 27 March 2017 and 4 April 2017: 9 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 12,816 hectares (128.2 km²). It is an estimate: official national figures may differ.
- Which municipalities burned?
- The fire entered 3 municipalities: Peshrar (6,711 ha, 19 %); Bishunpur (5,377 ha, 8.8 %); Latehar (791 ha, 1.6 %).
- What was the weather like?
- During the fire the temperature reached 37.1 °C, humidity dropped to 12 % and gusts hit 56 km/h. The fire danger index (FWI) reached 53, class Extreme.
- 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
Satellite cross-check
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
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.