TRISHNA Satellite Mission 2027: ISRO-France Mission, Objectives and Features
The Thermal Infra-Red Imaging Satellite for High-resolution Natural Resource Assessment (TRISHNA) is an international Earth observation satellite program being jointly developed by India’s ISRO and CNES of France. The satellite will be launched from Sriharikota and will be capable of studying surface temperature, evapotranspiration, vegetation status and water stress with high spatial and temporal resolutions. The data obtained through it is anticipated to help in agriculture monitoring, water resource management and climate studies.
TRISHNA is the Thermal Infra-Red Imaging Satellite for High-resolution Natural Resource Assessment.
It was created to provide high spatial and temporal resolution Earth surface data.
It is designed to observe the energy and water budgets of the continental biosphere, which will allow the estimation of terrestrial water stress and usage.
Some of the major scientific and environmental objectives of the mission are as follows,
Such observation could be useful for climatic studies, agriculture, water management, and disaster studies.
The satellite will be equipped with two main instruments that will be the result of the collaboration between ISRO and CNES, France’s space agency
1. Thermal Infrared (TIR) Instrument
2. Visible-Near Infrared-SWIR Instrument
Developed by ISRO
The satellite will be placed into a sun-synchronous orbit, 761 kilometers above the Earth.
The planned spatial resolution will be,
The mission will have a design life of five years.
TRISHNA’s high-resolution thermal observations may be useful in addressing emerging issues like water shortages, agriculture, urban heating and glacier melting.
It will also be a contributor to some of the international initiatives that include GEOGLAM, UN Sustainable Development Goals and Global Water Watch.
Some of the mission products are anticipated to act as Essential Agricultural Variables (EAVs) and Essential Climate Variables (ECVs).
Sun-synchronous orbit refers to a near-polar orbit that allows the satellite to pass over the same place at a similar local solar time each day.
This gives the same lighting condition every day, making image comparisons possible.
TRISHNA is expected to have an operational altitude of about 761 kilometers, with a local equator-crossing time of 12:30 noon.
This frequent revisit capability will help scientists observe changes in surface temperature and vegetation.
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