Space Offline-1
Space Offline-1
- HIMABINDU
Major events
1957: First artificial satellite Russian Sputnik 1 launched.
1962: Indian National Committee for Space Research (INCOSPAR) formed by the Department of Atomic Energy under the
leadership of Dr. Vikram Sarabhai
1969: Indian Space Research Organization (ISRO) formed under Department of Atomic Energy.
1972: Department of Space (DoS) established and ISRO brought under it.
1975: First Indian satellite, Aryabhata, launched into space April 19. It was completely designed in the country and
launched from a Russian facility.
1979: Bhaskara-I, an experimental remote sensing satellite for earth observations, launched from Russia into LEO.
1993: PSLV carried out its first mission, became the Indian space mission’s most reliable workhorse.
For the next 20 years, it launched various satellites for historic missions such as the Chandrayaan and Mangalyaan. PSLV
remains a favourite among various organizations as a launch service provider.
How Do Objects Stay in Orbit?
An object in motion will stay in motion unless something pushes or pulls on it. This
statement is called Newton's first law of motion. Without gravity, an Earth-orbiting
satellite would go off into space along a straight line. With gravity, it is pulled back
toward Earth. A constant tug-of-war takes place between the satellite's tendency to
move in a straight line, or momentum, and the tug of gravity pulling the satellite
back.
An object's momentum and the force of gravity have to be balanced for an orbit to
happen. If the forward momentum of one object is too great, it will speed past and
not enter into orbit. If momentum is too small, the object will be pulled down and
crash. When these forces are balanced, the object is always falling toward the
planet, but because it's moving sideways fast enough, it never hits the planet.
Orbital velocity is the speed needed to stay in orbit. At an altitude of 150 miles (242
kilometers) above Earth, orbital velocity is about 17,000 miles per hour. Satellites
that have higher orbits have slower orbital velocities.
Geo synchronous (GSO) / Geo stationary orbit (GEO)
• A low Earth orbit (LEO) is, as the name suggests, an orbit that is relatively
close to Earth’s surface.
• It is normally at an altitude of less than 1000 km but could be as low as 160
km above Earth – which is low compared to other orbits, but still very far
above Earth’s surface.
• Unlike satellites in GEO that must always orbit along Earth’s equator, Low
earth orbits can be tilted. This means there are more available routes for
satellites in LEO, which is one of the reasons why LEO is a very commonly
used orbit.
• LEO’s close proximity to Earth makes it useful for several reasons. It is the
orbit most commonly used for satellite imaging, as being near the surface
allows it to take images of higher resolution.
• It is also the orbit used for the International Space Station (ISS), as
it is easier for astronauts to travel to and from it at a shorter
distance.
• Satellites in this orbit travel at a speed of around 7.8 km per
second; at this speed, a satellite takes approximately 90 minutes to
circle Earth, meaning the ISS travels around Earth about 16 times a
day.
• However, individual LEO satellites are less useful for tasks such as
telecommunication, because they move so fast across the sky,
communications satellites in LEO often work as part of a large
combination or constellation, of multiple satellites to give constant
coverage.
Medium Earth orbit (MEO)
• Transfer orbits are a special kind of orbit used to get from one orbit to
another.
• A GTO is highly elliptic. Its perigee (closest point to Earth) is typically as
high as low Earth orbit (LEO), while its apogee (furthest point from Earth) is
as high as geostationary / geosynchronous orbit. That makes it a Hohmann
transfer orbit between LEO and GSO.
• Using this system, the satellite is placed into a low earth orbit with an altitude
of around 180 miles. Once in the correct position in this orbit rockets are
fired to put the satellite into an elliptical orbit with the perigee at the low
earth orbit and the apogee at the geostationary orbit as shown. When the
satellite reaches the final altitude the rocket or booster is again fired to retain
it in the geostationary orbit with the correct velocity.
Satellite Launchers
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1. Satellite Launch Vehicle-3:
• (SLV-3) was India's first experimental satellite launch vehicle,
which was an all solid, four stage vehicle weighing 17 tons with a
height of 22m and capable of placing 40 kg class payloads in Low
Earth Orbit (LEO).
• While building upon the experience gained from the SLV-3
missions, ISRO developed the “Augmented Satellite Launch
Vehicle” (ASLV), designed to augment the payload capacity to 150
kg for Low Earth Orbits (LEO). It is a five stage, all-solid
propellant vehicle.
Polar Satellite Launch Vehicle (PSLV):
• It is the third generation launch vehicle of India.
• It is the first Indian launch vehicle to be equipped with liquid stages.
• It is a four-staged launch vehicle with first and third stage using solid
rocket motors and second and fourth stages using liquid rocket
engines.
• It also uses strap-on motors to augment the thrust provided by the first
stage and depending on the number of these strap-on boosters, the PSLV
is classified into its various versions like core-alone version (PSLV-CA)
with no strap-on boosters, PSLV-G with six strap-on boosters (9 tons
each), and PSLV-XL variant with 6 strap-on boosters (12 tons each).
• New variants such as PSLV-DL (2 strap on motors) & PSLV-QL (4 strap
on motors) are also being used.
• PSLV is designed mainly to deliver the “remote-sensing”
satellites with lift-off mass of up to about 1750 Kg to Sun-
Synchronous circular polar orbits.
• After its first successful launch in October 1994, PSLV emerged as
the reliable and versatile workhorse launch vehicle of India by
launching the satellites of lower lift-off mass of up to about 1400 Kg
to GEO transfer orbit (GTO). Besides, the vehicle successfully
launched two spacecrafts – Chandrayaan-1 and Mars Orbiter
Spacecraft.
3. Geosynchronous Satellite Launch Vehicle (Fat boy):
• (GSLV) is the fourth generation launch vehicle developed by India. Two
versions of the GSLV are being developed by ISRO.
• The first version, GSLV Mk-II, has the capability to launch satellites
of lift-off mass of up to 2,500 kg to the GTO and satellites of up to
5,000 kg lift-off mass to the LEO.
• GSLV MK-II is a three-staged vehicle with first stage using solid
rocket motor, second stage using Liquid fuel and the third stage,
called Cryogenic Upper Stage, using cryogenic engine.
• GSLV Mk III, chosen to launch Chandrayaan – 2 spacecraft and will
be used to carry Gaganyaan.
• For one of its recent launch, ISRO redesignated GSLV-MK III to LVM-
III (Launch Vehicle – Mark III)
• It is a three-stage heavy lift launch vehicle developed by ISRO. The
vehicle has two solid strap-on boosters (S200 strap-ons) on either side
of its core. Each carry 204 tons of composite solid propellant and their
ignition results in vehicle lift off. Considered as stage 1
• Stage 2 is L110 liquid stage
• It has a cryogenic upper stage (C25).
• It is designed to carry 4-ton class of satellites into Geosynchronous
Transfer Orbit (GTO) or about 10 tons to LEO, which is about twice the
capability of GSLV Mk II.
Small Satellite Launch Vehicle (SSLV)
• Low-cost alternate to launch small satellites
• Produced through New space India Limited (NSIL,Nodal agency for SSLV)
• 3-Stage Solid propulsion
• Pay load capacity of 300 kg to Sun synchronous orbit & LEO 500 kg to
Low earth orbit.
Planned launches:
• In March 2022, ISRO has successfully conducted ground testing of
SSLV's solid booster stage-SS1, completing the ground testing of all 3
stages.
• SSLV-D1 (demonstration) launch has taken place in August 2022, but
failed due to a sensor failure and placed Earth Observatory satellite
(EOS)-2 and a student satellite into a wrong orbit.
• The second developmental flight of SSLV, SSLV-D2 is successfully
launched.
AGNILET: World’s first single-piece 3D-printed rocket
• On 4th November 2022, Chennai-headquartered space-tech start-up Agnikul had
successfully test-fired its single-piece 3D-printed engine, Agnilet.
• It is the world’s first single-piece 3D-printed rocket engine fully designed
and manufactured in India, which was successfully first test-fired at IIT Madras in
2021.
• The current test was conducted at Thumba Equatorial Rocket Launching Station
(TERLS), at Vikram Sarabhai Space Center (VSSC), Thiruvananthapuram.
• The test was carried out as part of MOU signed between ISRO and Agnikul
Cosmos Pvt. Ltd. to provide opportunity for Indian space start-ups to use facilities
of ISRO through (Indian National Space Promotion and Authorization Centre)
IN-SPACe.
• This engine is going to be used in Agniban, a highly customizable two-stage
rocket with 100 kg payload capacity to orbits around 700 km high (low Earth
orbits). It is going to use semi cryogenic engine that run on Kerosene as fuel and
Liquid oxygen as oxidizer.
Vikram-S: India's first privately made rocket launched
(Mission Prarambh)
• Vikram is a family of small lift launch vehicles being developed by
Hyderabad based startup, Skyroot Aerospace.
• It became the first Indian company to be authorised for launching a rocket
by Indian National Space Promotion and Authorisation Centre (IN-
SPACe).
• Skyroot has been developing 4 variants of the Vikram rocket, named after Dr.
Vikram Sarabhai.
• Vikram-S, a sounging rocket (used for probing the upper atmospheric regions
and for space research with their suborbital flights). was launched by Skyroot
Aerospace on 16th Nov 2022, from the sounding rocket launch complex at
Satish Dhavan Space Centre. The Mission titled 'Prarambh’ carried three
payloads. It marks the first launch of launch vehicle built by a private
company in India. It reached an altitude of 89.5 km. It was fuelled by 3-
stage all solid engine.
• Vikram-I can carry 480 kilograms of payload to Low Earth Orbit.
• Vikram-II is equipped to lift off with 595 kilograms of cargo.
• Vikram-III can launch with an 815 kg to 500 km Low Inclination Orbit.
● Skyroot's first privately developed, fully cryogenic rocket engine, Dhawan-I, for its
Vikram II was successfully test fired in 2021.
● Skyroot Aerospace test-fired its 3D-printed Dhawan II engine. The engine was
developed by the company for its updated version of, Vikram II.
● Dhawan-II is completely indigenous and used a super alloy for 3D printing the engine,
which reduced the manufacturing time by 95%. It will use Liquid Natural gas (LNG)
and Liquid Oxygen (LoX) as propellants.
● LNG is more than 90% methane and is considered the rocket fuel of the future.
● The engine development was partly supported by NITI Ayog’s ANIC-ARISE program
which promotes technologies including the use of green rocket propellants.
Reusable Launch Vehicle (RLV)
• Cryogenic rocket stage is more efficient and provides more thrust for every
kilogram of propellant it burns compared to solid and liquid propellant rocket
stages.
• Liquid Hydrogen and Liquid Oxygen are commonly used as cryogenic
propellants.
• Cryogenic stage is technically a very complex system compared to solid or
liquid propellant stages due to its use of propellants at extremely low
temperatures and other designing requirements.
• Oxygen liquifies at -183 deg C and Hydrogen at -253 deg C.
COMMUNICATION SATELLITES
Indian Express
Why ISRO want to explore the Moon’s South Pole:
Water Resources: The south pole region is believed to have water molecules in substantial
amounts, possibly trapped as ice in the permanently shadowed craters. Exploring and
confirming the presence of water is essential for future human missions and the potential
utilization of lunar resources.
Scientific Discoveries: The extreme environment and the presence of permanently
shadowed regions provide a preserved record of the Moon’s history and the early Solar
System.
Clues to Earth’s History: The Moon is thought to have formed from debris generated by a
giant impact between a Mars-sized object and the early Earth. By studying the lunar south
pole, scientists can gain insights into the materials and conditions that existed during the
formation of the Earth-Moon system.
Technological Advancements: By undertaking missions to this region, ISRO can develop
and demonstrate innovative technologies for soft landing, navigation, resource utilization,
and long-duration operations that can be applied in future space missions.
HIMA BINDU
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Hindustan Times
CHANDRAYAAN-3
● Chandrayaan-3 is India’s third moon mission and is a follow-up of Chandrayaan-
2 (2019) which aimed to land a rover on the lunar South Pole.
● It aims to be the world’s first mission to soft-land near the lunar South Pole.
About the Mission:
The Mission will have three major modules-
a) The Propulsion module (will carry the lander and rover configuration till 100 km
lunar orbit).
b) Lander module (capability to soft land and deploy Rover).
c) Rover (will carry out in-situ chemical analysis of the lunar surface).
Unlike Chandrayaan-2, it will not have an orbiter and its propulsion module will
behave like a communications relay satellite.
Chandrayaan-3 payloads:
The propulsion module:
● It has Spectro-polarimetry of Habitable Planet Earth (SHAPE) payload to look
for changes that a life supporting atmosphere make to the star light that is passing
through it, there by analysing possibility of life in nearby planets.
The Lander payloads:
● Radio Anatomy of Moon Bound Hypersensitive ionosphere and Atmosphere
(RAMBHA) – to measure near surface plasma density and and its changes with
time.
● Chandra’s Surface Thermophysical Experiment (ChaSTE) to measure the
thermal conductivity and temperature.
● Instrument for Lunar Seismic Activity (ILSA) for measuring the seismicity
around the landing site.
● Langmuir Probe (LP) to estimate the plasma density and its variations.
● A passive Laser retroreflector array from NASA to help accurately measure the
distance between Earth and moon.
The Rover payloads:
● Alpha Particle X-ray Spectrometer (APXS) and Laser Induced Breakdown
Spectroscopy (LIBS) for deriving the elemental composition in the vicinity of the
landing site.
Chandrayaan - 3 landed on Moon on 23rd August. Rover separated. And lost contact after
14 days.
Global Collaborations:
● ISRO-NASA successfully confirmed the presence of water from the data taken by
Chandrayaan-1.
● Indo-Japan collaboration, LUPEX aims to send a lander and rover to the Moon’s
south pole around 2024.
Findings of Chandrayaan 3:
• Chandrayaan-3 ‘unambiguously confirmed’ the presence of sulphur in the lunar
surface near south pole. Other elements like Aluminum (Al), Calcium (Ca), Iron
(Fe), Chromium (Cr), Titanium (Ti), Manganese (Mn), Silicon (Si), and Oxygen (O)
are also detected. The space agency further added that the search for Hydrogen (H) is
underway.
• 2. 4-meter diameter crater on Moon's surface
• Temperature recorded on the Lunar surface is 50-700C and at a depth of 8cm (-)100C
• Vikram lander studied the Moon’s Ionosphere to provide insights into developing
future communication technology suitable for Moon.
• Vikram lander detected seismic activity which could be either due to a moon quake
or an Asteroid hit.
• Pragyan Rover covered 100 meters distance of Lunar terrain.
• Found that near surface plasma environment (Charged particles) to be relatively
sparce means it will not cause much disturbance to radio communication.
• Vikram lander performed a hop experiment indicating that the space craft could be
used to bring samples back in future.
RUSSIA’S LUNA 25
● The race to send a spacecraft to the moon
has taken an exciting turn as Russia's
Luna 25 mission, launched on a Soyuz
rocket on August 11, 2023, aims to soft-
land on Moon’s south pole a few days
before India's Chandrayaan-3.
● Luna 25 marks Russia's return to lunar
HM
I exploration after 47 years, aiming to
reclaim its reputation in space exploration.
● Russia's space agency, Roscosmos asserts
that Luna 25's landing would not impact
Chandrayaan-3, as their landing regions
are distinct.
Reason for Luna 25 reaching the Moon Earlier than Chandrayaan-3:
• Direct Trajectory Advantage for Luna 25
• Luna 25's lift-off mass of 1,750 kg is significantly lighter than Chandrayaan-3's
3,900 kg, facilitating a quicker journey.
● Luna 25 benefits from an earlier lunar dawn at its landing site, ensuring full Solar
panel power for its payloads during the lunar day (equal to 14 Earth days).
Soft landing to moon:
● Only three countries have managed to complete a soft landing on the Moon in history:
the United States, the Soviet Union, and China.
Other Differences between Luna 25 and Chandrayaan 3:
Luna 25 is lighter and lacks a rover, The lander has eight payloads to study the soil
composition, dust particles in the polar exosphere, and detect surface water.
Chandrayaan-3 carries a rover capable of moving 500 meters, aims to study lunar soil,
and has instruments to detect water-ice in shadowed craters near the lunar South Pole.
Luna 25 is designed for a year-long mission, equipped with heating mechanisms
and a non-solar power source. In contrast, Chandrayaan-3 is built for a single lunar day
due to lack of heating during lunar nights.
Status of India Russia Space Collaboration:
● India’s first satellite, Aryabhata was launched by the Soviet Union in 1975.
● Only one Indian citizen has ever flown to space- Rakesh Sharma flew to the
Salyut 7 space station on a Soyuz rocket in 1984 as part of the USSR’s
Interkosmos program (a program designed to help allies with crewed and uncrewed
missions).
● In 2004, the two countries signed a protocol to boost cooperation in space. This
included the development of the GLONASS navigation system and the launching
of Russian GLONASS satellites by Indian rockets.
● Chandrayaan-2 was initially supposed to be a collaboration between India
and Russia.
● However, Russia withdrew from designing the lander-rover for
Chandrayaan-2 leading India to develop it independently.
● Also, four astronauts who will be part of India’s first crewed space
mission: Gaganyaan have been trained in Russian facilities.
Source: IE, 16 Aug 2023.
China’s Chang’e-4 Mission
• On January 2 nd , 2019, China has successfully landed a robotic
spacecraft on the far side of the Moon, the first ever such landing.
• Previous Moon missions have landed on the Earth-facing side, but this is
the first successfully landing on the unexplored far side.
• It is carrying instruments to analyse the unexplored region's geology, as
well to conduct biological experiments.
• The area where the probe has landed faces away from Earth, meaning it is
free from radio frequencies. As a result, it is not possible for a lunar rover
to communicate directly with ground control.
• Hence, China launched a dedicated satellite (Queqiao) orbiting to relay
information from the rover to Earth.
Tidal locking: The moon takes about 29 days to
complete one revolution around the Earth, the same
time it takes to make one rotation on its own axis. As
a result, we see the same side of the moon irrespective
of when and where on Earth we look at it from.
BepiColombo
European & Japanese collaborative mission to Mercury. Launched in
October 2018 and expected to reach Mercury in 2025.
Akatsuki
Japan’s first interplanetary mission actively studying Venus’s atmosphere.
Juno
NASA’s mission exploring Jupiter (Reached Jupiter in 2016).
VOYAGER TWIN SPACECRAFT
• The twin Voyager 1 and 2 spacecrafts launched in 1977 are continuing to explore where
nothing from Earth has flown before.
• The primary mission, Voyager 1 was the exploration of Jupiter and Saturn.
• Voyager 2 went on to explore Uranus and Neptune and is still the only spacecraft to
have visited those outer planets.
• In August 2012, Voyager 1 made the historic entry into interstellar space (the region
between stars), crossing the Heliopause (The boundary between solar wind and
interstellar wind). The interstellar space is filled with material ejected by the death of
nearby stars millions of years ago.
• Voyager 2 entered interstellar space on November 5, 2018 and scientists hope to learn
more about this region.
• Voyager’s power supply comes from a radioisotope thermoelectric generator (RTG)
which turns heat from the decay of radioactive material into electricity to power the
space craft.
• Twin Voyagers are likely to run out of power within 5 years.
ISRO, BARC JOIN HANDS TO DEVELOP
NUCLEAR ENGINES FOR ROCKETS
● Recently, the Bhabha Atomic Research Center (BARC) and the Indian Space
Research Organization (ISRO) began working together to develop radio
thermoelectric generators (RTGs), a novel strategy meant to overcome the
limitations of traditional chemical engines for interplanetary travel.
● Chemical engines work well for satellite thrusters, but they are inadequate for
deep space travel due to fuel limitations and lack of solar power in distant regions.
● RTGs have been successfully employed by US spacecraft such as the Voyager,
Cassini and Curiosity, to power missions with exceptional achievements.
Radio Thermoelectric Generators (RTGs):
● Radioisotope Heater Unit (RHU) utilize radioactive materials, such as
Plutonium-238 or Strontium-90, to emit heat as they decay over time.
● This heat is harnessed and converted into electricity by the RTG component.
● This conversion takes place through a thermocouple, a material that generates
voltage when subjected to a temperature gradient.
● The voltage produced by the thermocouple is utilized to charge batteries
onboard the spacecraft.
● These batteries, in turn, power various systems, including propulsion mechanisms,
enabling interplanetary travel.
Advantages of RTGs for Space Missions:
Independence from Solar Proximity:
● Unlike solar-powered systems, RTGs operate effectively regardless of the
spacecraft's distance from the sun.
● This characteristic eliminates constraints related to launch windows and
planetary alignment.
Reliability and Consistency:
● RTGs offer a consistent and reliable source of power, essential for
sustaining prolonged deep space missions.
● The gradual decay of radioactive materials ensures a continuous supply of
heat and electricity.
Bhabha Atomic Research Centre:
● BARC is India’s premier nuclear research facility based in Mumbai,
Maharashtra.
● It is a multi-disciplinary research center with core mandate to sustain
peaceful applications of nuclear energy, primarily for power generation.
Source: BL, 16 July 2023.
NUCLEAR-POWERED ROCKET
● NASA collaboration with the United States Defense Advanced Research Projects
Agency (DARPA) is seeking a nuclear propulsion system, a nuclear reactor that
utilizes the energy derived from the fission of uranium atoms that could
potentially cut down the travel time to Mars by half.
● This ambitious initiative, known as the Demonstration Rocket for Agile Cislunar
Operations (DRACO) and the launch is scheduled for late 2025 or early 2026.
Significance:
Minimized Exposure: The potential risks associated with extended space travel, such
as radiation exposure and isolation, could be mitigated through quicker journeys.
Military Applications: Nuclear propulsion can facilitate rapid maneuvers of
military satellites in Earth's orbit.
Concern:
• Safety Concerns: Accidents or malfunctions could release radioactive material
into space or back to Earth. Such incidents could have severe environmental and
health consequences.
• Launch Risks: There is always a chance of a launch failure or explosion, leading to
the dispersion of radioactive material over a wide area.
Historical Context of Nuclear Propulsion:
● Projects like Orion, Rover, and NERVA explored nuclear-powered propulsion
systems, although these initiatives were not fully realized.
● Notably, Project Orion considered using atomic bomb explosions for acceleration,
while Project NERVA aimed to develop a nuclear-thermal engine akin to the
DRACO engine.
DRACO’S advancement over its predecessors:
• Fuel Enrichment: Unlike Project NERVA, which used weapons-grade
uranium, DRACO employs a less-enriched form of uranium. This shift
enhances safety and minimizes the risks.
• In-Space Activation: The nuclear reactor within the DRACO engine
remains dormant until it reaches space. This mitigates the potential for
radioactive accidents during launch or on Earth.
Source: IE, 6 Aug 2023.
SOLAR PROBES
Aditya L1 Mission
• Expected launch: 2023
• A 400-Kg Space craft will be launched using PSLV-XL in an orbit around the
Lagrange point 1 (L1) of the Sun-Earth system.
• Lagrange points are the positions where the centrifugal force due to the velocity
of orbiting satellite & the gravitational force / centripetal forces of two large
bodies, Sun and earth balance each other. There are 5 such points in Sun-Earth
system.
• It is placed at 1.5 million kms away from earth to provide continuous view of the
Sun without any occultation due to eclipses.
• It aims to study
➢ Solar corona (Visible and near infrared rays), Sun's Photosphere (soft and hard
X-ray) & Chromosphere (UV) solar emissions.
➢ Solar winds and flares, Coronal mass ejections ( significant release of plasma
and accompanying magnetic field from solar corona)
➢ Round the clock imaging of sun
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HIMA BINDU
Parker Probe
‘Parker Mission’ is a probe launched by NASA to study the Sun.
• Launched using Delta-IV Heavy rocket in August 2018. Cost: $ 1.5 bn
• Over the course of seven years, Parker will make 24 loops around the Sun-
getting as close as about 6 million km away from the Sun of 150 million km.
• First-ever mission to "touch" the Sun (as per NASA, the probe in December
2021 flown through the Sun’s upper atmosphere – the corona – and sampled
particles and magnetic fields).
• This probe is considered to be the fastest man made object with speeds around
190 km/s.
Key objectives:
• in situ measurements and imaging.
• Understanding of the corona and expanding our knowledge of the origin and
evolution of the solar wind.
• To forecast changes in Earth's space environment that affect life on Earth.
The European Space Agency’s (ESA) Vigil mission
(formerly known as Lagrange)
• It’s the first of its kind mission, with the aim of monitoring the unpredictable and
active Sun and help protect the Earth from its outbursts.
• Solar flares, coronal mass ejections, geomagnetic storms, and other space weather
incidences will be monitored by ESA Vigil.
• Monitoring of the space incidences will help in predicting the timing of its arrival
on Earth and any effect it might have on infrastructure.
• This mission plans to position two spacecraft in the L1 and L5 Lagrangian points.
• The spacecraft at L1 is to provide observations of the solar wind speed, density,
temperature and dynamic pressure, charged particle environment and the direction
and strength of the interplanetary magnetic field.
• The spacecraft at L1 would also monitor the solar
corona and measure solar energetic particles that may
be associated with solar flares and the onset
of coronal mass ejections.
• The spacecraft at L5 would complement
measurements made from L1 by providing a side-
view of the propagation of plasma clouds emitted by
the Sun toward Earth.
• The spacecraft at L5 would monitor of the solar disk
and corona and carry out measurements of
the interplanetary medium.
SOLAR STORMS
• The Solar magnetic cycle that works in the deep
interior of the Sun creates regions that rise to the surface
and appear like dark spots. These are sunspots.
• Solar magnetic cycle: Every 11 years or so, the Sun's
magnetic field completely flips. This means that the
Sun's north and south poles switch places.
• One way to track the solar cycle is by counting the
number of sunspots. The beginning of a solar cycle is
a solar minimum, or when the Sun has the least
sunspots. Over time, solar activity—and the number of
sunspots—increases.
• They typically consist of a dark region called the
‘umbra’, which is surrounded by a lighter region called
the ‘penumbra’.
● Solar flares are highly energetic phenomena that happen when the energy
stored in the sun’s magnetic structures called sunspots is converted into light
and heat energy. This causes the emission of high energy electromagnetic
waves like radio waves, x-ray radiation, Gamma rays. They travel at a speed
of light. Takes 8 mins to reach Earth.
● There are five categories of solar flare according to their brightness in the x-
ray wavelengths, which include A, B, C, M, and X; each class is at least ten
times more potent than the one before it.
● (Current: Recently, the Sun emitted an X1.0 -class solar flare, disrupting
radio communications over parts of the United States and the Pacific Ocean).
● The solar wind is a stream of charged particles released from the
outer most layer of the Sun’s atmosphere called the corona. This
mostly consists of electrons, protons and alpha particles with kinetic
energy between 0.5 and 10 keV.
● A coronal mass ejections (CME) are significant release
of plasma and accompanying magnetic field from
the Sun's corona into the solar wind. They can harbour energies
exceeding that of a million atomic bombs. Take 1-3 days to reach
Earth.
● Solar flares occur in active regions and are often, but not always,
accompanied by coronal mass ejections.
• Geomagnetic storm: Major disturbance of Earth's magnetosphere due to the
heliospheric magnetic field (HMF) that is dragged out from the solar corona
by the solar wind. They are categorised as G1, G2,G3,G4,G5 in the increasing order
of their intensity.
• Solar storms occur when sun emits huge bursts of energy in the form of solar flares
and Coronal mass ejections. Solar storms can last only a few minutes to
several
hours, but the effects of geomagnetic storms can linger in the Earth's
magnetosphere and atmosphere for days to weeks. They are categorised as
S1,S2,S3,S4,S5 in the increasing order of their intensity
• (Note: Magnetosphere is that area of space, around a planet, that is controlled
by
the planet’s magnetic field.
• The interplanetary magnetic field (IMF) or heliospheric magnetic field (HMF), is
the component of the solar magnetic field that is dragged out from the
solar corona by the solar wind flow to fill the Solar System.)
Effect of Solar storms:
• Judging by data from the NASA DSCOVR satellite, the scientists observed a
steep jump in transverse magnetic fields, density and speeds of the plasma
wind that are tell-tale signatures of the arrival of a coronal mass ejection shock
front. (The shock wave of travelling mass)
• The energy, radiation and high energy particles emitted by flares can affect Earth
bound objects and life on Earth – it can affect the electronics within satellites and
affect astronauts. International Space station ISS could also have been affected.
• Intermittent satellite navigation (GPS) problems.
• Very powerful Earth-directed coronal mass ejections can cause failure of power
grids and affect oil pipelines and deep-sea cables.
• They can also cause spectacular aurorae in the high-latitude and polar
countries.
• The last major blackout due to a coronal mass ejection recorded was in 1989.
Predicting Solar Storms:
• The process of prediction takes place in two steps: First the researchers
analyse the possibility of a strong solar flare from an active region –
that is, clusters of sunspots using a machine learning algorithm which
has been developed in CESSI, IISER Kolkata.
• The second step is estimating the time of arrival on Earth of coronal
mass ejections and forecasting the geomagnetic storm.
• If there is an associated flare, its position on the Sun is used to extract
the location of origin of the CME. The location of the source of the
CME and the velocity are used as inputs in a model called the Drag
Based Ensemble Model to calculate the CME arrival times and
speed.
7)If a major Solar storm (Solar flare) reaches the Earth, which of the following are
the possible effects on the Earth? (UPSC 2022)
HIMA BINDU
• LIGO project operates three gravitational-wave (GW) detectors. Two are at Hanford
in the state of Washington, USA, and one is at Livingston in Louisiana, USA.
• Currently these observatories are being upgraded to their advanced configurations
(called Advanced LIGO).
• The proposed LIGO-India project aims to move one Advanced LIGO detector
from Hanford to India.
• LIGO-India project is envisaged as an international collaboration between the
LIGO Laboratory and Indigo (A consortium of Indian gravitational wave
physicists).
• The Union cabinet on 6th April 2023 approved the project at an estimated cost of
Rs 2600 crores. The facility’s construction is expected to be completed by 2030.
• LIGO India will cork in tandem with the twin LIGO observatories in USA.
• LIGO lab would provide the complete design and all the key detector components.
Indian scientists would provide the infrastructure to install the detector at a suitable
site in India and would be responsible for commissioning it.
• VIRGO detector is a 3 km interferometer in Italy.
• The KAGRA observatory is an underground 3 km interferometer in
Japan.
• They are managed by VIRGO collaboration and KAGRA collaboration,
respectively.
• LIGO-VIRGO-KAGRA (LVK) collaboration: These detectors need to be
operating simultaneously around the globe to localize a source of
gravitational waves anywhere in the sky.
• LIGO's success has led to ESA's plans of a future mission possibly by 2034.
The project is called Evolved Laser Interferometry Space Antenna / New
Gravitational Wave Observatory (eLISA/NGO) - or just LISA for short.
• The first step to ESA's space-based observatory has been taken. LISA
Pathfinder, which was a test-phase mission, ends on July 18, 2017, having
shown its technology works in space.
Laser Interferometer Space Antenna (LISA)
• The Laser Interferometer Space Antenna (LISA) is a proposed space
probe to detect and accurately measure gravitational waves from
astronomical sources.
• LISA would be the first dedicated space-based gravitational wave
detector.
• The LISA concept has a constellation of three spacecraft arranged in an
equilateral triangle with sides 2.5 million km long, flying along an Earth-
like heliocentric orbit.
• LISA will observe gravitational waves by measuring differential changes
in the length of its arms, as sensed by laser interferometry. (work by
merging two or more sources of light to create an interference pattern,
which can be measured and analysed.) Each of the three LISA spacecraft
contains two telescopes, two lasers and two test masses
• (each a 46 mm, roughly 2 kg, gold-coated cube of gold/platinum),
arranged in two optical assemblies pointed at the other two spacecraft
• Studying gravitational waves gives enormous potential for
discovering the parts of the universe that are invisible by other means,
such as black holes, the and other yet unknown, objects. LISA will
complement our knowledge about the beginning, evolution and
structure of our universe.
• The LISA project started out as a joint effort between NASA and
the European Space Agency (ESA). However, in 2011, NASA
announced that it would be unable to continue its LISA partnership
with the European Space Agency due to funding limitations.
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MANNED MISSIONS AND
SPACE STATIONS
GAGANYAAN
• First-ever manned space mission of India – announced on 15th Aug,2018.
• Expected launch - in 2023
• Budget: 10,000 cr.
• India to become fourth country in the world to send manned missions to
space after USA, Russia and China.
• Planning to send 3 astronauts (using GSLV Mk-III) into LEO (300-400km).
They can see India from space while conducting experiments on
microgravity.
• Two unmanned test missions (delayed to 2023) will be launched before the
final manned mission.
• A humanoid robot (Vyom mitra) will be part of unmanned missions.
• Recently, ISRO has successfully integrated Vyom mitra with a computer
‘brain’ to enable it to ‘read’ control panels aboard the unmanned test flights
and communicate with its voice with the ISRO ground stations.
HIMA BINDU
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• ISRO has begun work on the manned mission in 2004.
• Many of the critical technologies required for human spaceflight have
already been validated through various tests
✓ Space Capsule Recovery Experiment (from water bodies)
✓ Crew Module Atmospheric Re-Entry Experiment (CARE) in Dec-2014.
✓ Pad Abort Test (An ISRO launch escape system test of its crew module).
• Four Indian Air Force fighter pilots completed training in Moscow
Gagarin Research & Test Cosmonaut Training Center (GCTC) (Glavkosmos)
• Spacesuits are being made by Defence Bioengineering and Electromedical
Laboratory (DEBEL), an Indian defence laboratory under the DRDO.
SPACE STATION FOR INDIA
• ISRO is planning to setup its own space station in about a decade.
• It would be similar to the International Space Station (ISS) but smaller in
size weighing about 20 tonnes.
• It would be placed in a low earth orbit (~ 400 km).
• The preliminary plan for the space station is to accommodate astronauts for
up to 15-20 days in space to conduct microgravity experiments.
• It may take about 5 to 7 seven years to construct, details will only emerge
after the Gaganyaan Mission is complete.
• China is also planning a large space station in the Lower Earth Orbit.
MISSIONS AND SATELLITE
LAUNCHES IN NEWS
JAMES WEBB SPACE TELESCOPE
• Next Generation Telescope - successor to the Hubble Space Telescope.
• Developed by NASA—in collaboration with the Canadian Space
Agency and the European Space Agency (Cost: $9.7 billion).
• It will be the largest and most powerful telescope ever built for use in
space.
• Launched on 25th December 2021 by the Ariane 5 rocket from European
Space Agency's Spaceport in French Guiana.
• Maximum Life span estimated to be 10 years.
• After a 29 day-long journey, the spacecraft will arrive at Lagrangian point
2 (nearly 1.5 million km from Earth).
• The gravitational forces of the Sun and the Earth can nearly hold a
spacecraft at this point, so that it takes relatively little rocket thrust to keep
the spacecraft in orbit around L2.
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• It will have a much larger primary
mirror than Hubble (2.7 times larger
in diameter & 6 times larger in area), giving
it more light-gathering power.
• It has infrared instruments with longer
U
wavelength coverage and greatly
improved sensitivity than Hubble.
• Biggest feature is a tennis court sized five-
layer sunshield that attenuates heat
from the sun more than a million times.
• The telescope recently captured a clear
image of the planet Uranus and its rings.
(April 2023)
NASA's DART (Double Asteroid Redirection) Test
• On September 27, 2022, NASA conducted DART (Double Asteroid Redirection
Test).
• It is a mission to demonstrate Kinetic impact/Kinetic kick method to deflect
an asteroid by changing its motion.
• For this test, NASA targeted Asteroid pair Didymos and its moonlet
Dimorphos.
• LICIACube (Light Italian CubeSat for Imaging Asteroids) was launched
from earth along side the DART impactor to take pictures of the Asteroid
before & after the collision.
• DART collided with the Dimorphos (just 160 meters wide) at a speed of 23,760
kilometers per hour, and changed its angular momentum and moved it in to
a closer orbit to Didymos – causing deflection.
• This method is expected to save the world in future by safely deflecting a
killer asteroid on its course towards earth.
PSLV-C44 mission
• PSLV C-44 served as a test for a new variant of the launch vehicle, the
PSLV-DL, which has two strap-on motors.
• It will make use of the final stage of rocket as an experimental orbital
platform for Kalamsat, world’s smallest student satellite, built by
Chennai based school students. It will continue orbiting the earth at a
distance of 450km above it for six months, maybe more.
• PSLV C44 also carried an imaging and surveillance satellite called
Microsat for the Defence Research and Development Organisation
(DRDO).
• Microsat was targeted in Anti-satellite test (ASAT), Mission Shakti.
FUTURE MISSIONS OF ISRO
X-ray Polarimeter Satellite (XPoSat):
• It is a satellite that ISRO plans to launch on a Small Satellite launch
vehicle 2023.
• It will be placed in the Low Earth Orbit.
• It will measure polarisation of X-rays released from cosmic sources.
(Polarisation: An electromagnetic wave such as light consists of a
coupled oscillating electric field and magnetic field which are always
perpendicular to each other; by convention, the "polarization" of
electromagnetic waves refers to the direction of the electric field).
• X-ray polarisation measurements help understand the nature of
their source, including strength, distribution of its magnetic
field and the nature of other radiation around it ( As the
polarization of X-rays affect these factors).
The payloads to be carried:
• Polarimeter Instrument in X-rays (POLIX), developed by
Bengaluru-based Raman Research Institute.
• XSPECT (X-ray Spectroscopy and Timing).
NISAR Mission
• NASA-ISRO Synthetic Aperture Radar.
• It will be the first satellite mission to use two different radar
frequencies (L-band and S-band) to measure changes in our planet’s surface.
• NASA will provide the mission’s L-band Synthetic Aperture Radar and
ISRO will provide S-band Synthetic Aperture Radar.
• This allows the mission to observe a wide range of changes, from the flow
rates of glaciers and ice sheets to the dynamics of earthquakes and volcanoes,
biomass, natural hazards, sea level rise, and groundwater etc.
• Likely to be launched by GSLV in 2024 from India after final assembly at UR
RAO Space centre into a sun synchronous orbit from Satish Dhawan
Space Centre .
SPACE DEBRIS
• Space debris is the collection of defunct man-made objects in space — old
satellites, spent rocket stages and fragments from disintegration and collisions.
• It is estimated that there are about half a million pieces of man-made
substances orbiting the Earth.
• These space debris can really be dangerous as they travel at high speeds, which
turns even tiny pieces of junk into deadly shrapnel that can damage satellites,
space shuttles and even space stations.
• Kessler effect/syndrome: Proposed by NASA scientist Donald J. Kessler in
1978 - proposed that a chain reaction of exploding space debris can end up
making space activities and the use of satellites impossible for generations.
Space debris – Steps taken by ISRO
• ISRO is a member of “Inter-Agency Space Debris Coordination
Committee” (IADC), which makes global efforts to reduce man-made and
natural space debris. They exchange information on space debris among
member space agencies and alert a respective space agency when any
satellite of that space agency is in danger due to space debris.”
• ISRO also banks on its sophisticated “Multi-Object Tracking Radar
(MOTR)”, operational since 2015, to track space debris.
• In 2019, ISRO initiated ‘Project NETRA’ (NEtwork for space object
TRacking and Analysis) – an early warning system in space to detect debris
and other hazards to Indian satellites.
• On 14th December 2020, ISRO inaugurated a dedicated space
situational awareness (SSA) Centre at ISRO Telemetry, Tracking
and Command Network (ISTRAC) in Bangalore under project
NETRA.
• The project NETRA with an estimated to cost of ₹400 crore, will give
India its own capability in space situational awareness (SSA) like
the other space powers — which is used to ‘predict’ threats from
debris to Indian satellites.
• Under “NETRA”, ISRO is planning to set up several observational
facilities: connected radars, telescopes; data processing units and
a control Centre.
Initial focus seems to be on debris in the Low Earth Orbit,
eventually ISRO wants to track the debris in GEO where the
communication satellites operate.
Need:
• Currently there are 15 functional Indian communication satellites
in the GEO, 13 remote sensing satellites in LEO & 8 navigation
satellites in MEO. Protecting them is important for India.
• This would make India a part of international efforts towards
tracking, warning about and mitigating space debris.
SPACE DEBRIS –
INTERNATIONAL EFFORTS TO CLEANUP
1. “RemoveDEBRIS” has been deployed from the International Space Station
(ISS) that can capture and deorbit the debris.
2. European Space Agency with Swiss startup company “Clear Space” is
building a spacecraft equipped with four robotic arms to capture debris and
drag it into Earth’s atmosphere. This mission, known as ClearSpace-1, is
expected to launch by 2025.
3. NASA's Space Debris Sensor orbits the Earth on the International Space
Station.
4. The United Nations has established the Committee on the Peaceful Uses of
Outer Space (COPUOS).
PRIVATIZING SPACE
ACTIVITIES
• Department of Space announced Cabinet approval on reforms to boost private
participation in space activities on 24 June, 2020.
• GOI announced the establishment of a new autonomous body - Indian National
Space Promotion and Authorization Centre (IN-SPACe) that will take "decisions
to regulate and permit activities in the space sector - a facilitator, and also a
regulator.
❖ ISRO will be the main body for all the missions.
❖ IN-SPACE acts as a channel between private and government space sectors.
❖ NSIL works as marketing arm for ISRO
• Private companies can now produce their own satellites and rockets and use
ISRO’s launch facility to launch them for a fee.
• A large part of manufacturing and fabrication of rockets and satellites has also
begun in the private sector through NSIL.
NSIL & ANTRIX corporation
• An agreement between Antrix corporation and Bengaluru based startup Devas
multimedia was signed in 2005 under which Antrix agreed to build, launch and
operate two satellites and lease our 90% of satellite transponder capacity to Devas
which had planned to use it to offer hybrid satellite and terrestrial communication
services throughout India.
• The deal included 70MHz of S-band spectrum (Restricted for the use by security
forces and government telecom entities like MTNL and BSNL) which was
priced at 1000 crore. A media expose claimed that incurred heavy loss to the
national exchequer (Treasurer or the treasury itself).
• The controversial deal was cancelled later.
• The long legal battle between Antrix and Devas ended up in the supreme court in 1st
Jan 2022 which ordered the winding up of the startup.
• NSIL is considered to be a move to protect the space industry in India from the
consequences of the Devas-Antrix mess.
New Space India Limited
• It is a new commercial arm of ISRO, incorporated on 6 March 2019 (under the
Companies Act, 2013) is a wholly owned Government of India company, under the
administrative control of Department of Space (DOS).
• NSIL will have role in the following:
➢ Production of Polar Satellite Launch Vehicle (PSLV) and Small Satellite Launch
Vehicle (SSLV) through industry;
➢ Building of Satellites (both Communication and Earth Observation) as per user
requirements.
➢ Transfer of technology developed by ISRO centres/ units and constituent
institutions of Dept. of Space;
➢ Marketing spin off technologies and products/ services emanating out of ISRO
activities
ISRO is also willing to provide place for private players to build their own launchpad
within the Sriarikota launch station.
SPACE X
• Space Exploration Technologies Corporation (Space X) is an American
aerospace manufacturer and space transportation services company.
•It was founded in 2002 by Elon Musk.
Crew Dragon spacecraft
• Space X has contract with NASA for Cargo and crew transportation to and
from the International Space Station.
• On 30th May 2020, Crew dragon Demo-2 mission took Two NASA astronauts
to ISS. It was the first crewed test flight of the crew dragon space craft and the
falcon 9 rocket.
• SpaceX Crew -1 mission: On 16th November 2020, SpaceX launched four
astronauts (3 Americans + 1 Japanese) to the International Space Station in the
first operational crewed flight of a “Crew dragon, resilience ”, spacecraft on a
Falcon 9 rocket. It was the first full-fledged taxi flight for NASA by a private
company.
• SpaceX broke the world record of the greatest number of satellites
carried by a single rocket as by sending 143 payloads into space
on 24th Jan 2021.
• With this it broke the record of ISRO’s 104 satellites being launched
in one go in February 2017.
• The reusable Falcon 9 rocket carried 133 commercial and
government spacecraft and 10 Starlink satellites to space - part of
the company’s Small Satellite Rideshare Programme.
• (Note: Starlink is a satellite internet constellation being constructed
by SpaceX providing satellite internet access)
Space Race
SpaceX
(Elon Musk)
Inspiration-4
1.PSLV launch the satellites useful for earth sources monitoring where as GSLVs
are designed mainly to launch communication satellites.
2.Satellites launched by PSLV appear to remain permanently fixed in the same
position in the sky, as viewed from a particular location on Earth.
3. GSLV Mk III is four-staged launch vehicle with the first and third stages using
solid rocket motors; and second and fourth stages using liquid rocket engines.
Which of the statements given above is/are correct?
a) 1 only
b) 2 and 3 only
c) 1 and 2 only
d) 3 only
4) In which of the following areas can GPS technology be used? (UPSC 2018)
a) Voyager-2
b) New Horizons
c) LISA Pathfinder
d) Evolved LISA