Aditya-L1 (
Sanskrit
Sanskrit (; stem form ; nominal singular , ,) is a classical language belonging to the Indo-Aryan languages, Indo-Aryan branch of the Indo-European languages. It arose in northwest South Asia after its predecessor languages had Trans-cultural ...
: 'Sun', L1 '
Lagrange Point 1') is a
coronagraphy spacecraft for studying the
solar atmosphere
The Sun is the star at the centre of the Solar System. It is a massive, nearly perfect sphere of hot Plasma (physics), plasma, heated to incandescence by nuclear fusion reactions in its core, radiating the energy from its surface mainly as ...
, designed and developed by the
Indian Space Research Organisation
The Indian Space Research Organisation (ISRO ) is India's national List of government space agencies, space agency, headquartered in Bengaluru, Karnataka. It serves as the principal research and development arm of the Department of Space (DoS), ...
(ISRO) and various other Indian Space Research Institutes.
It is orbiting at about 1.5 million km from Earth in a
halo orbit around the
Lagrange point 1 (L1) between the
Earth
Earth is the third planet from the Sun and the only astronomical object known to Planetary habitability, harbor life. This is enabled by Earth being an ocean world, the only one in the Solar System sustaining liquid surface water. Almost all ...
and the
Sun
The Sun is the star at the centre of the Solar System. It is a massive, nearly perfect sphere of hot plasma, heated to incandescence by nuclear fusion reactions in its core, radiating the energy from its surface mainly as visible light a ...
, where it will study the solar atmosphere,
solar magnetic storms, and their impact on the environment around the Earth.
It is the first
Indian mission dedicated to observe the Sun.
Nigar Shaji is the project's director.
Aditya-L1 was launched aboard the
PSLV C57 at 11:50
IST on 2 September 2023.
It successfully achieved its intended orbit nearly an hour later, and separated from its
fourth stage at 12:57 IST.
It was inserted at the L1 point on 6 January 2024, at 4:17 pm IST.
In February 2024, Aditya-L1 observed a powerful flare erupt from Earth's sun from its vantage point–a distance of about 1 million miles (1.5 million kilometers).
Mission objectives
The main objectives of Aditya-L1 are:
* To observe the dynamics of the Sun's
chromosphere
A chromosphere ("sphere of color", from the Ancient Greek words χρῶμα (''khrôma'') 'color' and σφαῖρα (''sphaîra'') 'sphere') is the second layer of a Stellar atmosphere, star's atmosphere, located above the photosphere and below t ...
and
corona:
** To study
chromospheric and
coronal heating, the physics of
partially ionised plasma, of
coronal mass ejection
A coronal mass ejection (CME) is a significant ejection of plasma mass from the Sun's corona into the heliosphere. CMEs are often associated with solar flares and other forms of solar activity, but a broadly accepted theoretical understandin ...
s (CMEs) and their origins, of the coronal
magnetic field
A magnetic field (sometimes called B-field) is a physical field that describes the magnetic influence on moving electric charges, electric currents, and magnetic materials. A moving charge in a magnetic field experiences a force perpendicular ...
and
heat transfer
Heat transfer is a discipline of thermal engineering that concerns the generation, use, conversion, and exchange of thermal energy (heat) between physical systems. Heat transfer is classified into various mechanisms, such as thermal conduction, ...
mechanisms, and
flare
A flare, also sometimes called a fusée, fusee, or bengala, bengalo in several European countries, is a type of pyrotechnic that produces a bright light or intense heat without an explosion. Flares are used for distress signaling, illuminatio ...
exchanges.
* To observe the physical particle environment around its position.
* To determine the sequence of processes in multiple layers below the corona that lead to
solar eruptions.
* To study
space weather
Space weather is a branch of space physics and aeronomy, or heliophysics, concerned with the varying conditions within the Solar System and its heliosphere. This includes the effects of the solar wind, especially on the Earth's magnetosphere, ion ...
, and the origin, composition and dynamics of
solar wind
The solar wind is a stream of charged particles released from the Sun's outermost atmospheric layer, the Stellar corona, corona. This Plasma (physics), plasma mostly consists of electrons, protons and alpha particles with kinetic energy betwee ...
.
History

The mission was conceptualised in January 2008 by the Advisory Committee for Space Sciences (ADCOS). It was initially envisaged as a small, satellite in a
Low Earth Orbit
A low Earth orbit (LEO) is an geocentric orbit, orbit around Earth with a orbital period, period of 128 minutes or less (making at least 11.25 orbits per day) and an orbital eccentricity, eccentricity less than 0.25. Most of the artificial object ...
(800 km) with a
coronagraph to study the
solar corona
In astronomy, a corona (: coronas or coronae) is the outermost layer of a star's Stellar atmosphere, atmosphere. It is a hot but relatively luminosity, dim region of Plasma (physics), plasma populated by intermittent coronal structures such as so ...
. An experimental budget of was allocated for the financial year 2016–2017.
The scope of the mission has since been expanded and it became a comprehensive solar and space environment
observatory
An observatory is a location used for observing terrestrial, marine, or celestial events. Astronomy, climatology/meteorology, geophysics, oceanography and volcanology are examples of disciplines for which observatories have been constructed.
Th ...
to be placed at
Lagrange point 1 (L1), hence the mission was renamed as ''Aditya-L1.'' , the mission has an allocated cost of , excluding launch costs.
The
European Space Operations Centre (ESOC), operated by the
European Space Agency
The European Space Agency (ESA) is a 23-member International organization, international organization devoted to space exploration. With its headquarters in Paris and a staff of around 2,547 people globally as of 2023, ESA was founded in 1975 ...
(ESA) is supporting the mission.
On 11 January 2024, ISRO successfully deployed a 6-meter
magnetometer
A magnetometer is a device that measures magnetic field or magnetic dipole moment. Different types of magnetometers measure the direction, strength, or relative change of a magnetic field at a particular location. A compass is one such device, ...
boom aboard the Aditya-L1 in the
Halo orbit at the Lagrange Point L1. After the liftoff, the boom had been stowed for 132 days. The in-orbit deployment period that was measured was roughly 9 seconds, which is well within the 8–12 second prediction range. The magnetometer boom will measure the low-intensity interplanetary magnetic field in space using two high-accuracy
fluxgate magnetometer sensors that are carried aboard. In order to reduce the impact of the spacecraft's
magnetic field
A magnetic field (sometimes called B-field) is a physical field that describes the magnetic influence on moving electric charges, electric currents, and magnetic materials. A moving charge in a magnetic field experiences a force perpendicular ...
on measurements, the sensors are placed 3 and 6 meters away from the craft. Using a dual sensor system also helps to cancel out the spacecraft's magnetic influence and facilitates accurate estimation. The
carbon-fiber-reinforced polymers (CFRP) was used in the construction of the boom segments. Through the use of spring-driven
hinge
A hinge is a mechanical bearing that connects two solid objects, typically allowing only a limited angle of rotation between them. Two objects connected by an ideal hinge rotate relative to each other about a fixed axis of rotation, with all ...
mechanisms, the five pieces are joined to enable folding in close proximity to the craft throughout the journey and opening up upon reaching the desired orbit. The hinges lock into place as the mechanism fans out. In the stowed position, two hold-downs firmly secure the boom in place. Information obtained via the
telemetry
Telemetry is the in situ collection of measurements or other data at remote points and their automatic transmission to receiving equipment (telecommunication) for monitoring. The word is derived from the Greek roots ''tele'', 'far off', an ...
switches validates the release of the hold-down, the initial motion, and the locking of every hinge.
Overview

The mission took 126 Earth days after launch to reach the
halo orbit around the L1 point, which is about from Earth. The spacecraft is planned to remain in the halo orbit for its mission duration while being maintained at a
stationkeeping Δv of 0.2–4 m/s per year. The satellite carries seven science payloads with various objectives, including instruments to measure
coronal heating,
solar wind
The solar wind is a stream of charged particles released from the Sun's outermost atmospheric layer, the Stellar corona, corona. This Plasma (physics), plasma mostly consists of electrons, protons and alpha particles with kinetic energy betwee ...
acceleration, coronal magnetometry, origin and monitoring of
near-UV solar radiation
Sunlight is the portion of the electromagnetic radiation which is emitted by the Sun (i.e. solar radiation) and received by the Earth, in particular the visible light perceptible to the human eye as well as invisible infrared (typically p ...
(which drives Earth's upper atmospheric dynamics and global climate), coupling of the solar photosphere to the chromosphere and corona, and
in-situ
is a Latin phrase meaning 'in place' or 'on site', derived from ' ('in') and ' ( ablative of ''situs'', ). The term typically refers to the examination or occurrence of a process within its original context, without relocation. The term is use ...
characterisations of the space environment around Earth by measuring energetic particle fluxes and magnetic fields of the solar wind, and
solar magnetic storms.
Aditya-L1 will provide observations of the Sun's
photosphere
The photosphere is a star's outer shell from which light is radiated. It extends into a star's surface until the plasma becomes opaque, equivalent to an optical depth of approximately , or equivalently, a depth from which 50% of light will esc ...
,
chromosphere
A chromosphere ("sphere of color", from the Ancient Greek words χρῶμα (''khrôma'') 'color' and σφαῖρα (''sphaîra'') 'sphere') is the second layer of a Stellar atmosphere, star's atmosphere, located above the photosphere and below t ...
and
corona. Its scientific payloads must be placed outside the interference from the
Earth's magnetic field
Earth's magnetic field, also known as the geomagnetic field, is the magnetic field that extends from structure of Earth, Earth's interior out into space, where it interacts with the solar wind, a stream of charged particles emanating from ...
, and hence, could not have been useful in the low Earth orbit, as proposed in the original mission concept back in 2008.
One of the major unsolved problems in the field of
solar physics
Solar physics is the branch of astrophysics that specializes in the study of the Sun. It intersects with many disciplines of pure physics and astrophysics.
Because the Sun is uniquely situated for close-range observing (other stars cannot be re ...
is coronal heating. The upper atmosphere of the Sun has a temperature of , whereas the lower atmosphere is just . In addition, it is not understood exactly how the Sun's radiation affects the dynamics of the Earth's atmosphere on a shorter as well as a longer time scale. The mission will obtain near-simultaneous images of the different layers of the Sun's atmosphere, which will reveal the ways in which energy is channeled and transferred from one layer to another. Thus, the mission will enable a comprehensive understanding of the dynamical processes of the Sun and address some of the outstanding problems in solar physics and
heliophysics
Heliophysics (from the prefix "wikt:helio-, helio", from Attic Greek ''hḗlios'', meaning Sun, and the noun "physics": the science of matter and energy and their interactions) is the physics of the Sun and its connection with the Solar System. ...
.
Payloads

The instruments of Aditya-L1 are tuned to observe the solar atmosphere, mainly the chromosphere and corona. In-situ instruments will observe the local environment at the L1 point. There are seven payloads on board, with four for
remote sensing
Remote sensing is the acquisition of information about an physical object, object or phenomenon without making physical contact with the object, in contrast to in situ or on-site observation. The term is applied especially to acquiring inform ...
of the Sun and three for in-situ observation. The payloads have been developed by different laboratories in the country with close collaborations of various ISRO centres.
Visible Emission Line Coronagraph (VELC)
The Visible Emission Line Coronagraph (VELC) is a key instrument on the
Aditya spacecraft. The VELC is an internally
occulted reflective coronagraph designed to fulfil specific observation needs. The instrument allows for high spatial resolution imaging 1.25-2.5
arcseconds of the Sun's corona, simultaneous observations in three modes (Imaging, Spectroscopy and
Spectro-polarimetry), and even utilizes artificial intelligence to aid in the detection of coronal mass ejections (CMEs). The instrument was developed by
Indian Institute of Astrophysics,
Bangalore
Bengaluru, also known as Bangalore (List of renamed places in India#Karnataka, its official name until 1 November 2014), is the Capital city, capital and largest city of the southern States and union territories of India, Indian state of Kar ...
.
Solar Ultraviolet Imaging Telescope (SUIT)
The SUIT is an ultraviolet imaging telescope designed to study the solar spectral radiation in the
ultraviolet
Ultraviolet radiation, also known as simply UV, is electromagnetic radiation of wavelengths of 10–400 nanometers, shorter than that of visible light, but longer than X-rays. UV radiation is present in sunlight and constitutes about 10% of ...
range, using narrowband and broadband spectral filters in the range of 200-400 nm with the hope of developing a better understanding between solar activity and the atmospheric dynamics of Earth. The SUIT provides near-simultaneous coverage of the solar atmosphere, from lower photosphere to the upper chromosphere. The instrument was developed by
Inter University Centre for Astronomy & Astrophysics,
Pune
Pune ( ; , ISO 15919, ISO: ), previously spelled in English as Poona (List of renamed Indian cities and states#Maharashtra, the official name until 1978), is a city in the state of Maharashtra in the Deccan Plateau, Deccan plateau in Western ...
, in collaboration with ISRO.
Solar Low Energy X-ray Spectrometer (SoLEXS)
The SoLEXS is an X-ray spectrometer designed to continuously measure the solar
soft X-ray flux (1 keV-22 keV) from the Sun-Earth Lagrangian point L1. These measurements can be used to better understand the properties of the Sun's corona, in particular, why the temperature of the corona is so high. The SoLEXS will observe solar flares, and in conjunction with data provided by the VELC, will help study the complex thermal properties of the Sun's outer layers. The instrument was developed by
U R Rao Satellite Centre,
Bangalore
Bengaluru, also known as Bangalore (List of renamed places in India#Karnataka, its official name until 1 November 2014), is the Capital city, capital and largest city of the southern States and union territories of India, Indian state of Kar ...
.
High Energy L-1 Orbiting X-ray Spectrometer (HEL1OS)
Developed by the Space Astronomy Group, URSC, the HEL1OS (pronounced ''helios)'' is an x-ray spectrometer designed to study solar flares in the x-ray spectrum, in particular, energy bands of 10-150 Kev (
kilo-electron volts). Using a twin-pair of
Cadmium Telluride (CdTe) and
Cadmium Zinc Telluride (CZT) detectors, the instrument aims to study the acceleration and movement of electrons in the Sun's corona, as well as to study the
cut-off energy between thermal and non-thermal solar emissions.
Aditya Solar Wind Particle Experiment (ASPEX)
The ASPEX is an instrument composed of low and
high energy particle spectrometers, designed to conduct measurements of the Sun's solar wind particles. Solar Wind Ion Spectrometer (SWIS), the low energy spectrometer, contains two analysers, each designed to study particles entering the device in different planes. Supra Thermal Energetic Particle Spectrometer (STEPS), the high energy spectrometer, also consists of two parts, STEPS 1 and STEPS 2, both designed to separate protons and
alpha particle
Alpha particles, also called alpha rays or alpha radiation, consist of two protons and two neutrons bound together into a particle identical to a helium-4 nucleus. They are generally produced in the process of alpha decay but may also be produce ...
s and measure the integrated
flux
Flux describes any effect that appears to pass or travel (whether it actually moves or not) through a surface or substance. Flux is a concept in applied mathematics and vector calculus which has many applications in physics. For transport phe ...
. The instrument was developed by the
Physical Research Laboratory,
Ahmedabad
Ahmedabad ( ), also spelled Amdavad (), is the most populous city in the Indian state of Gujarat. It is the administrative headquarters of the Ahmedabad district and the seat of the Gujarat High Court. Ahmedabad's population of 5,570,585 ...
.
Plasma Analyser Package for Aditya (PAPA)
The PAPA is an instrument on board the Aditya-L1 designed to study the temperature, distribution and velocity of the solar winds. The instrument contains two sensors; the Solar Wind Electron Energy Probe (SWEEP) and the Solar Wind lon Composition Analyser (SWICAR). The detectors are used in conjunction to analyse the energy levels of electrons and ions within the solar wind. The instrument was developed by the Space Physics Laboratory of the
Vikram Sarabhai Space Centre,
Thiruvananthapuram
Thiruvananthapuram ( ), also known as Trivandrum, is the Capital city, capital city of the Indian state of Kerala. As of 2011, the Thiruvananthapuram Municipal Corporation had a population of 957,730 over an area of 214.86 sq. km, making it the ...
.
Digital magnetometers
On board the Aditya-L1 spacecraft are a pair of magnetic sensors on a deployable boom, one positioned in the middle and the other at the tip. The purpose of these sensors is to gather information about the magnitude and direction of the Interplanetary Magnetic Fields (IMF), as well as to study other events such as Coronal Mass Ejections (CME). Data from the magnetic sensors will be used to supplement that of the PAPA and ASPEX sensors.
Mission profile
Launch
On 2 September 2023, at 11:50
IST, the
Polar Satellite Launch Vehicle (PSLV-C57) accomplished a successful launch of the ''Aditya-L1'' from the
Second Launch Pad of the
Satish Dhawan Space Centre (SDSC) located in
Sriharikota.
''Aditya-L1'', following a flight duration of 63 minutes and 20 seconds, achieved a successful
injection into an
elliptical orbit
In astrodynamics or celestial mechanics, an elliptical orbit or eccentric orbit is an orbit with an orbital eccentricity, eccentricity of less than 1; this includes the special case of a circular orbit, with eccentricity equal to 0. Some or ...
around the Earth at 12:54
IST.
''Aditya-L1'' underwent a series of four Earth-bound
orbital maneuvres prior to its injection to a transfer orbit towards the
Lagrange point
In celestial mechanics, the Lagrange points (; also Lagrangian points or libration points) are points of equilibrium for small-mass objects under the gravitational influence of two massive orbiting bodies. Mathematically, this involves t ...
(L1). It reached its designated orbit at the L1 point 126 days after its launch on 6 January 2024 at 4:17 IST.
Orbit raising burns
; First orbit raising burn
On 3 September 2023, the ''Aditya-L1'' performed its first Earth-bound maneuvre, raising its orbit to a into orbit.
; Second orbit raising burn
On 5 September 2023, ''Aditya-L1'' performed its second Earth-bound maneuvre, raising its orbit to a into orbit.
; Third orbit raising burn
On 10 September 2023, ''Aditya-L1'' performed its third Earth-bound maneuvre, raising its orbit to a into orbit.
; Fourth orbit raising burn
On 15 September 2023, ''Aditya-L1'' performed its fourth Earth-bound maneuvre, raising its original orbit to a into orbit. This was the last of such maneuvers, being directly followed by the Trans-Lagrangian 1 Injection, which took place on 19 September.
; Trans-Lagrangian 1 Injection
On 19 September 2023, ''Aditya-L1'' performed its last maneuvre around Earth to escape its orbit and headed towards the Lagrange 1 point, taking at least four months to further reach its destination, 1.5 million kilometers away.
On 30 September 2023, ''Aditya-L1'' had escaped the Earth's sphere of influence and was on the way to the Lagrange point 1.
During this journey a week before Orbital Insertion, the SUIT instrument captured an X-class solare flare and a CME on December 31st 2023.This was the first observations of a solar flare using
near-UV light.
;Trajectory correction maneuver
On 6 October 2023, ''Aditya-L1'' performed a Trajectory Correction maneuvre (TCM1). It was needed to correct the trajectory evaluated after tracking the Trans-Lagrangian Point 1 Insertion (TL1I) maneuvre performed on 19 September 2023.
;Halo orbit insertion
On 6 January 2024, ''Aditya-L1'' was successfully injected on the
Halo orbit of Lagrange point 1 (HOI), at 4:17 pm IST.
Orbit
Aditya-L1 completed its first
halo orbit around L1 point on July 2, 2024. It takes it approximately 178 days to complete each orbit. It underwent two station-keeping maneuvers on February 22 and June 7, and later one on July 2.
Science phase
Following commissioning and checkout, Adiya L1 began Science observations about three months into the mission. The PAPA instrument on the spacecraft was operationalised on December 12, 2023, and made its first observation on February 10 and 11, 2024.
In conjunction with the
Udaipur Solar Observatory and research stations at
Thumba, ISRO mobilised all its observation platforms and systems to record the signatures of a Massive Solar Flare in May 2024. Aditya-L1,
Chandrayaan-2's orbiter and
XPoSat have made observations and observed signatures have been analysed. Aditya-L1 used ASPEX, SOLEX, HEL1OS an its
magnetometer
A magnetometer is a device that measures magnetic field or magnetic dipole moment. Different types of magnetometers measure the direction, strength, or relative change of a magnetic field at a particular location. A compass is one such device, ...
instruments to record data. On July 16, 2024, the VELC instrument was used to measure a large Coronal Mass ejection from the Sun. It also studied an accompanying solar flare and the motion of solar particles within the Sun.
Marking its first year of science observation, ISRO released the maiden set of the scientific data from the Aditya L1 to the global scientific community on January 6, 2025, at the ISRO Headquarters in Bengaluru. ISRO presented the second set on 14 February 2025. On February 22, 2024, Aditya L1 captured the first-ever image of a ''X6.3-class''
solar flare ‘kernel’ occurring in the
photosphere
The photosphere is a star's outer shell from which light is radiated. It extends into a star's surface until the plasma becomes opaque, equivalent to an optical depth of approximately , or equivalently, a depth from which 50% of light will esc ...
and the
chromosphere
A chromosphere ("sphere of color", from the Ancient Greek words χρῶμα (''khrôma'') 'color' and σφαῖρα (''sphaîra'') 'sphere') is the second layer of a Stellar atmosphere, star's atmosphere, located above the photosphere and below t ...
. The image was taken alongside operations of SUIT, SoLEXS and HEL1OS instruments in the
Near-Ultraviolet band. Scientist from IIA reported observations of a flareless coronal mass ejection from reading taken by VELC in March 2025.
Gallery
Images of the sun taken from SUIT (Solar Ultraviolet Imaging Telescope) instrument of Aditya-L1 in different wavelengths.
Team
*
Nigar Shaji - Project director
*
Sankarasubramanian K - Principal scientist of the mission
See also
*
*
Solar space missions
**
**
**
**
**
*
References
External links
ISRO page for Aditya-L1
{{Orbital launches in 2023
Satellites of India
Spacecraft launched by India in 2023
Missions to the Sun
September 2023 in India
Space probes launched in 2023