The document discusses India's Mars Orbiter Mission (MOM), known as Mangalyaan, which was launched by the Indian Space Research Organisation (ISRO) in November 2013 with the goal of placing an orbiter around Mars to study its surface, atmosphere and climate. ISRO's MOM mission aims to demonstrate India's low-cost spaceflight capabilities and technological prowess. The orbiter successfully entered Mars' orbit in September 2014, making India the first nation to reach Mars on its first attempt and the first nation to successfully place an orbiter around Mars on its maiden interplanetary mission.
India (ISRO) accomplished a spectacular milestone by launching a satellite orbiting around Mars. The mission has critical significance in the history of Mars missions. These slides cover information about this mission including some awesome tricks used in the mission.
Mangalyaan india's first MOM at first attempt,
so over view of MOM, and brief explanation of instruments used in payload spacecraft, and phases of orbital transformation
India (ISRO) accomplished a spectacular milestone by launching a satellite orbiting around Mars. The mission has critical significance in the history of Mars missions. These slides cover information about this mission including some awesome tricks used in the mission.
Mangalyaan india's first MOM at first attempt,
so over view of MOM, and brief explanation of instruments used in payload spacecraft, and phases of orbital transformation
The Mars Orbiter Mission (MOM), also called Mangalyaan is a space probe orbiting Mars since 24 September 2014. It is India's first interplanetary mission and ISRO has also become the fourth space agency to reach Mars, after the Soviet space program, NASA, and the European Space Agency. It is the first Asian nation to reach Mars orbit, and the first nation in the world to do so in its first attempt.
INDIA'S FIRST MARS SPACE MISSION NAMED MARS ORBITER MISSION(MOM) SIMPLY KNOWN AS MANGALYAN. FOR MORE UPDATES AND SLIDES VISIT www.mechanizeinn.wordpress.com OR www.facebook.com/mechanizeinn
Mangalyaan ppt for vi bha student's forum vidarbha unitDr. BP Joshi
This is short presentation on Indias Mangalyaan mission, the orbiter which was launched last year and is about to reach its destination. These slides are for small presentation on the ISRO's mission. It is made with purpose of generating curiosity in students about the scientific milestone of India.
Mars Orbiter Mission ( MOM ) or Mangalyaan aman2227
India creates history as ISRO's first Mars orbiter Mangalyaan successfully enters red planet's orbit.
Indian country's space agency became the fourth to successfully put a satellite in orbit around Mars – and the first to manage it on its first try.
(download the following videos from youtube for working of videos:1. http://www.youtube.com/watch?v=OIKunbW-Ch4 2.https://www.youtube.com/watch?v=HHYsTvanNY4 3.https://www.youtube.com/watch?v=LWtLiLp_Bng)
Mars orbiter mission (Mangalyaan)The govt. of INDIAArchit Jindal
All details of the Mars orbiter mission of India. Also the details about ISRO who is carrying out this mission. Also Mp4 video of launch of PSLV-XL which was the launch vehicle for the spacecraft. I hope this presentation is useful for you.The video will work.
The Mars Orbiter Mission (MOM), also called Mangalyaan is a space probe orbiting Mars since 24 September 2014. It is India's first interplanetary mission and ISRO has also become the fourth space agency to reach Mars, after the Soviet space program, NASA, and the European Space Agency. It is the first Asian nation to reach Mars orbit, and the first nation in the world to do so in its first attempt.
INDIA'S FIRST MARS SPACE MISSION NAMED MARS ORBITER MISSION(MOM) SIMPLY KNOWN AS MANGALYAN. FOR MORE UPDATES AND SLIDES VISIT www.mechanizeinn.wordpress.com OR www.facebook.com/mechanizeinn
Mangalyaan ppt for vi bha student's forum vidarbha unitDr. BP Joshi
This is short presentation on Indias Mangalyaan mission, the orbiter which was launched last year and is about to reach its destination. These slides are for small presentation on the ISRO's mission. It is made with purpose of generating curiosity in students about the scientific milestone of India.
Mars Orbiter Mission ( MOM ) or Mangalyaan aman2227
India creates history as ISRO's first Mars orbiter Mangalyaan successfully enters red planet's orbit.
Indian country's space agency became the fourth to successfully put a satellite in orbit around Mars – and the first to manage it on its first try.
(download the following videos from youtube for working of videos:1. http://www.youtube.com/watch?v=OIKunbW-Ch4 2.https://www.youtube.com/watch?v=HHYsTvanNY4 3.https://www.youtube.com/watch?v=LWtLiLp_Bng)
Mars orbiter mission (Mangalyaan)The govt. of INDIAArchit Jindal
All details of the Mars orbiter mission of India. Also the details about ISRO who is carrying out this mission. Also Mp4 video of launch of PSLV-XL which was the launch vehicle for the spacecraft. I hope this presentation is useful for you.The video will work.
Research & Development - Major Organisations of India , R&D Importance and RoleNaman Kumar
SPEECH
Naman: Good morning, respected teachers and my dear friends, today we the students of class Xi- C are going’ to explain the role and importance of Research and Development . Today in this presentation we will cover up on topics
• What is R&D
• Its role and importance
• Its components
• R&D in INDUSTRY
• R&D in India
• Expenditure analysis in different sectors of technology.
What is R&D?
Rohan: But friends do you really know what is research and development.
“Research and development (R&D) aims to create new technology or information that can improve the effectiveness of products or make the production of products more efficient.”
In layman’s language it’s a way to use our science to improve our standard of living.
Importance of R&D
Naman: Research and development is very crucial to find out solution to various problems of mankind and development of human beings. It is R&D with which the man could find solution to various diseases like discovery of penciline and various antibiotics. It is the research only with which we r enjoying various advanced technology
It is a continue process, to find specific solution to various new emerging needs of man. 13656286
Components of R&D
Rohan: To understand the R&D in depth we have to divide the R&D in to 2 major components:-
No. 1 Research and second is development.
Further research can be of two types Basic and Applied research
Basic research is just to find out the hidden truth of nature, may be in the field of physics, biology, botany, environment. Normally it is undertaken by advanced study centers of universities or corporates.
Second is Applied research - it is to find out a solution of a specific problem with the help of already discovered various principles or theories. Making an airplane of 5th generation.
Naman: Development is the stage in which we come out of the lab and try to make prototype application of the product , then go for trial in the field and modification and finally making a useful product.
R&D In Industry
There is always development and growth in industrial products. Few years back we were using CRTs for our computer monitors and TVs, now LED & LCD have taken their place. It is the role of R&D in Industry, we are experiencing a large variety of automobiles on roads as well as a wide range of electronic gadgets.
Rohan: After the independence India has put special importance to research activities for development of our industries. We have also established space research centers to explore various space technology like satellite communication. India’s main research centers are
1) CSIR for development of industrial sector
2) ISRO for development of space technology,
3) DRD
Mars Orbiter Mission (MOM), also called Mangalyaan With Mp4 Video..best pptNoman Jarang
The Mars Orbiter Mission (MOM), also called Mangalyaan ("Mars-craft" from Sanskrit मंगल mangala, "Mars" and यान yāna, "craft, vehicle"), is a spacecraft orbiting Mars since 24 September 2014. It was launched on 5 November 2013 by the Indian Space Research Organisation (ISRO)
The Indian space programmed had begun with no intentions of undertaking sophisticated initiatives like human spaceflight and extraterrestrial missions during the initial days. It was only after ISRO developed the capabilities of creating satellites and orbital launch vehicles like PSLV, that the possibilities of India's first extraterrestrial exploration mission to the Moon were being explored in the early 2000s.
Chandrayaan-2 is the second lunar exploration mission developed by the Indian Space Research Organisation, after Chandrayaan-1. It currently consists of a lunar orbiter, and also included the Vikram lander, and the Pragyan lunar rover, all of which were developed in India.
This pdf is about the Schizophrenia.
For more details visit on YouTube; @SELF-EXPLANATORY;
https://www.youtube.com/channel/UCAiarMZDNhe1A3Rnpr_WkzA/videos
Thanks...!
Introduction:
RNA interference (RNAi) or Post-Transcriptional Gene Silencing (PTGS) is an important biological process for modulating eukaryotic gene expression.
It is highly conserved process of posttranscriptional gene silencing by which double stranded RNA (dsRNA) causes sequence-specific degradation of mRNA sequences.
dsRNA-induced gene silencing (RNAi) is reported in a wide range of eukaryotes ranging from worms, insects, mammals and plants.
This process mediates resistance to both endogenous parasitic and exogenous pathogenic nucleic acids, and regulates the expression of protein-coding genes.
What are small ncRNAs?
micro RNA (miRNA)
short interfering RNA (siRNA)
Properties of small non-coding RNA:
Involved in silencing mRNA transcripts.
Called “small” because they are usually only about 21-24 nucleotides long.
Synthesized by first cutting up longer precursor sequences (like the 61nt one that Lee discovered).
Silence an mRNA by base pairing with some sequence on the mRNA.
Discovery of siRNA?
The first small RNA:
In 1993 Rosalind Lee (Victor Ambros lab) was studying a non- coding gene in C. elegans, lin-4, that was involved in silencing of another gene, lin-14, at the appropriate time in the
development of the worm C. elegans.
Two small transcripts of lin-4 (22nt and 61nt) were found to be complementary to a sequence in the 3' UTR of lin-14.
Because lin-4 encoded no protein, she deduced that it must be these transcripts that are causing the silencing by RNA-RNA interactions.
Types of RNAi ( non coding RNA)
MiRNA
Length (23-25 nt)
Trans acting
Binds with target MRNA in mismatch
Translation inhibition
Si RNA
Length 21 nt.
Cis acting
Bind with target Mrna in perfect complementary sequence
Piwi-RNA
Length ; 25 to 36 nt.
Expressed in Germ Cells
Regulates trnasposomes activity
MECHANISM OF RNAI:
First the double-stranded RNA teams up with a protein complex named Dicer, which cuts the long RNA into short pieces.
Then another protein complex called RISC (RNA-induced silencing complex) discards one of the two RNA strands.
The RISC-docked, single-stranded RNA then pairs with the homologous mRNA and destroys it.
THE RISC COMPLEX:
RISC is large(>500kD) RNA multi- protein Binding complex which triggers MRNA degradation in response to MRNA
Unwinding of double stranded Si RNA by ATP independent Helicase
Active component of RISC is Ago proteins( ENDONUCLEASE) which cleave target MRNA.
DICER: endonuclease (RNase Family III)
Argonaute: Central Component of the RNA-Induced Silencing Complex (RISC)
One strand of the dsRNA produced by Dicer is retained in the RISC complex in association with Argonaute
ARGONAUTE PROTEIN :
1.PAZ(PIWI/Argonaute/ Zwille)- Recognition of target MRNA
2.PIWI (p-element induced wimpy Testis)- breaks Phosphodiester bond of mRNA.)RNAse H activity.
MiRNA:
The Double-stranded RNAs are naturally produced in eukaryotic cells during development, and they have a key role in regulating gene expression .
Professional air quality monitoring systems provide immediate, on-site data for analysis, compliance, and decision-making.
Monitor common gases, weather parameters, particulates.
The increased availability of biomedical data, particularly in the public domain, offers the opportunity to better understand human health and to develop effective therapeutics for a wide range of unmet medical needs. However, data scientists remain stymied by the fact that data remain hard to find and to productively reuse because data and their metadata i) are wholly inaccessible, ii) are in non-standard or incompatible representations, iii) do not conform to community standards, and iv) have unclear or highly restricted terms and conditions that preclude legitimate reuse. These limitations require a rethink on data can be made machine and AI-ready - the key motivation behind the FAIR Guiding Principles. Concurrently, while recent efforts have explored the use of deep learning to fuse disparate data into predictive models for a wide range of biomedical applications, these models often fail even when the correct answer is already known, and fail to explain individual predictions in terms that data scientists can appreciate. These limitations suggest that new methods to produce practical artificial intelligence are still needed.
In this talk, I will discuss our work in (1) building an integrative knowledge infrastructure to prepare FAIR and "AI-ready" data and services along with (2) neurosymbolic AI methods to improve the quality of predictions and to generate plausible explanations. Attention is given to standards, platforms, and methods to wrangle knowledge into simple, but effective semantic and latent representations, and to make these available into standards-compliant and discoverable interfaces that can be used in model building, validation, and explanation. Our work, and those of others in the field, creates a baseline for building trustworthy and easy to deploy AI models in biomedicine.
Bio
Dr. Michel Dumontier is the Distinguished Professor of Data Science at Maastricht University, founder and executive director of the Institute of Data Science, and co-founder of the FAIR (Findable, Accessible, Interoperable and Reusable) data principles. His research explores socio-technological approaches for responsible discovery science, which includes collaborative multi-modal knowledge graphs, privacy-preserving distributed data mining, and AI methods for drug discovery and personalized medicine. His work is supported through the Dutch National Research Agenda, the Netherlands Organisation for Scientific Research, Horizon Europe, the European Open Science Cloud, the US National Institutes of Health, and a Marie-Curie Innovative Training Network. He is the editor-in-chief for the journal Data Science and is internationally recognized for his contributions in bioinformatics, biomedical informatics, and semantic technologies including ontologies and linked data.
Slide 1: Title Slide
Extrachromosomal Inheritance
Slide 2: Introduction to Extrachromosomal Inheritance
Definition: Extrachromosomal inheritance refers to the transmission of genetic material that is not found within the nucleus.
Key Components: Involves genes located in mitochondria, chloroplasts, and plasmids.
Slide 3: Mitochondrial Inheritance
Mitochondria: Organelles responsible for energy production.
Mitochondrial DNA (mtDNA): Circular DNA molecule found in mitochondria.
Inheritance Pattern: Maternally inherited, meaning it is passed from mothers to all their offspring.
Diseases: Examples include Leber’s hereditary optic neuropathy (LHON) and mitochondrial myopathy.
Slide 4: Chloroplast Inheritance
Chloroplasts: Organelles responsible for photosynthesis in plants.
Chloroplast DNA (cpDNA): Circular DNA molecule found in chloroplasts.
Inheritance Pattern: Often maternally inherited in most plants, but can vary in some species.
Examples: Variegation in plants, where leaf color patterns are determined by chloroplast DNA.
Slide 5: Plasmid Inheritance
Plasmids: Small, circular DNA molecules found in bacteria and some eukaryotes.
Features: Can carry antibiotic resistance genes and can be transferred between cells through processes like conjugation.
Significance: Important in biotechnology for gene cloning and genetic engineering.
Slide 6: Mechanisms of Extrachromosomal Inheritance
Non-Mendelian Patterns: Do not follow Mendel’s laws of inheritance.
Cytoplasmic Segregation: During cell division, organelles like mitochondria and chloroplasts are randomly distributed to daughter cells.
Heteroplasmy: Presence of more than one type of organellar genome within a cell, leading to variation in expression.
Slide 7: Examples of Extrachromosomal Inheritance
Four O’clock Plant (Mirabilis jalapa): Shows variegated leaves due to different cpDNA in leaf cells.
Petite Mutants in Yeast: Result from mutations in mitochondrial DNA affecting respiration.
Slide 8: Importance of Extrachromosomal Inheritance
Evolution: Provides insight into the evolution of eukaryotic cells.
Medicine: Understanding mitochondrial inheritance helps in diagnosing and treating mitochondrial diseases.
Agriculture: Chloroplast inheritance can be used in plant breeding and genetic modification.
Slide 9: Recent Research and Advances
Gene Editing: Techniques like CRISPR-Cas9 are being used to edit mitochondrial and chloroplast DNA.
Therapies: Development of mitochondrial replacement therapy (MRT) for preventing mitochondrial diseases.
Slide 10: Conclusion
Summary: Extrachromosomal inheritance involves the transmission of genetic material outside the nucleus and plays a crucial role in genetics, medicine, and biotechnology.
Future Directions: Continued research and technological advancements hold promise for new treatments and applications.
Slide 11: Questions and Discussion
Invite Audience: Open the floor for any questions or further discussion on the topic.
A brief information about the SCOP protein database used in bioinformatics.
The Structural Classification of Proteins (SCOP) database is a comprehensive and authoritative resource for the structural and evolutionary relationships of proteins. It provides a detailed and curated classification of protein structures, grouping them into families, superfamilies, and folds based on their structural and sequence similarities.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
6. OBJECTIVES
• Design and realisation of a Mars orbiter with a capability to perform
Earth bound maneuvers, cruise phase of 300 days, Mars orbit
insertion / capture, and on-orbit phase around Mars.
• Deep space communication, navigation, mission planning and
management.
• Incorporate autonomous features to handle contingency situations.
• The secondary objectives are scientific, and include the study of Mars
surface features, morphology, mineralogy and the Martian
atmosphere.
7. The Launch Vehicle - PSLV-C25 will inject the Spacecraft into an Elliptical
Parking Orbit with a perigee of 250 km and an apogee of 23,500 km. With six
Liquid Engine firing, the spacecraft is gradually maneuvered into a hyperbolic
trajectory with which it escapes from the Earth’s Sphere of Influence (SOI) and
arrives at the Mars Sphere of Influence.
When spacecraft reaches nearest point
of Mars (Peri-apsis), it is maneuvered
in to an elliptical orbit around Mars by
firing the Liquid Engine. The spacecraft
then moves around the Mars in an orbit
with Peri-apsis of 366 km and Apo-apsis
of about 80000 km.
11. Established in 1969, ISRO superseded the erstwhile Indian National Committee
for Space Research (INCOSPAR). Headquartered in Bangalore, ISRO is under
the administrative control of the Department of Space, Government of India.
Since its establishment, ISRO has achieved numerous milestones. It built
India's first satellite, Aryabhata, which was launched by the Soviet Union on 19
April in 1975. In 1980, Rohini became the first satellite to be placed in orbit by
an Indian-made launch vehicle, SLV-3. ISRO subsequently developed two
other rockets: the Polar Satellite Launch Vehicle (PSLV) for launching
satellites into polar orbits and the Geosynchronous Satellite Launch Vehicle
(GSLV) for placing satellites into geostationary orbits.
12.
13. The Mars Orbiter Mission (MOM), informally called Mangalyaan (Sanskrit:
मङ्गलयान, "Mars-Craft"), is a Mars orbiter launched into Earth orbit on 5
November 2013 by the Indian Space Research Organisation (ISRO). It has
entered orbit of Mars on 24 September 2014.
The mission is a
"technology
demonstrator" project
aiming to develop the
technologies required
for design, planning,
management, and
operations of an
interplanetary mission.
14. Travelling at a speed of 1.55 km per second, Mangalyan crossed half way to Mars
on 9 April 2014.
It is India's first interplanetary mission and, ISRO became the fourth space
agency to reach Mars, after the Soviet space program, NASA, and European
Space Agency.
The spacecraft is being currently monitored from the Spacecraft Control Centre
at ISRO Telemetry, Tracking and Command Network (ISTRAC) in Bangalore with
support from Indian Deep Space Network (IDSN) antennae at Byalalu.
15. LAUNCH AND ORBIT
• launch will place from sriharikota and the Mars Orbiter was placed into
Earth orbit, then six engine firings which raise the orbit to one with an
apogee of 215,000 km and a perigee of 600 km,where it remained for
about 25 days.
• A final firing in 30 November 2013 sent MOM onto an interplanetary
trajectory.
• Mars orbit insertion was done on 21 September 2014 and allowed the
spacecraft to enter a highly elliptical orbit of 372 km x 80,000 km around
Mars.
16. Electric power is generated by three solar array panels of 1.8 m × 1.4 m (5 ft. 11 in
× 4 ft. 7 in) each (7.56 m2 (81.4 sq. ft.) total), for a maximum of 840 W generation
in Martian orbit. Electricity is stored in a 36 Ah Li-ion battery.
Liquid fuel engine of 440 N thrust is used for orbit raising and insertion in Martian
orbit. The orbiter also has eight 22 N thrusters for attitude control or orientation.
Two 230 W TWTAs and two coherent transponders. The antenna array consists of
a low-gain antenna, a medium-gain antenna and a high-gain antenna. The High-
gain antenna system is based on a single 2.2-metre reflector illuminated by a feed
at S-band. It is used to transmit and receive the telemetry, tracking, commanding
and data to and from the Indian Deep Space Network.
17. 1. Geo Centric Phase
The spacecraft is injected into an Elliptic Parking Orbit by the launcher. With six
main engine burns, the spacecraft is gradually maneuvered into a departure
hyperbolic trajectory with which it escapes from the Earth’s Sphere of Influence
(SOI) with Earth’s orbital velocity + V boost. The SOI of earth ends at 918347 km
from the surface of the earth beyond which the perturbing force on the orbiter is
mainly due to the Sun. One primary concern is how to get the spacecraft to Mars,
on the least amount of fuel. ISRO uses a method of travel called a Hohmann
Transfer Orbit – or a Minimum Energy Transfer Orbit – to send a spacecraft from
Earth to Mars with the least amount of fuel possible.
18. 2. Helio Centric Phase
The spacecraft leaves Earth in a direction tangential to Earth’s orbit and
encounters Mars tangentially to its orbit. The flight path is roughly one half of an
ellipse around sun. Eventually it will intersect the orbit of Mars at the exact
moment when Mars is there too. This trajectory becomes possible with certain
allowances when the relative position of Earth, Mars and Sun form an angle of
approximately 44o. Such an arrangement recur periodically at intervals of about
780 days. Minimum energy opportunities for Earth-Mars occur in November
2013, January 2016, May2018 etc.
19. 3. Martian Phase
The spacecraft arrives at the Mars Sphere of Influence (around 573473 km
from the surface of Mars) in a hyperbolic trajectory. At the time the
spacecraft reaches the closest approach to Mars (Periapsis), it is captured
into planned orbit around mars by imparting ∆V retro which is called the
Mars Orbit Insertion (MOI) manoeuvre. The Earth-Mars trajectory is shown
in the above figure. ISRO plans to launch the Mars Orbiter Mission during
the November 2013 window utilizing minimum energy transfer opportunity.
20. The MOM mission concept began with a feasibility study in 2010, after
the launch of lunar satellite Chandrayaan-1 in 2008. The government of
India approved the project on 3 August 2012, after the Indian Space
Research Organisation completed ₹1.25 billion (US $21 million) of
required studies for the orbiter. The total project cost may be up to
₹4.54 billion (US $77 million). The satellite costs ₹1.53 billion (US$26
million) and the rest of the budget has been attributed to ground
stations and relay upgrades that will be used for other ISRO projects.
The space agency had initially planned the launch on 28 October 2013
but was postponed to 5 November 2013 following the inability of
ISRO's spacecraft tracking ships to take up pre-determined positions
due to poor weather in the Pacific Ocean. Launch opportunities for a
fuel-saving Hohmann transfer orbit occur about every 26 months, in
this case, 2016 and 2018. The Mars Orbiter's on-orbit mission life will
be between six and ten months.
21. Mars Orbiter Mission spacecraft being prepared for a prelaunch
test at Satish Dhawan Space Centre SHAR, Srihairkota.
22. The lift-off mass was 1,350 kg (2,980 lb), including 852 kg (1,878 lb)
of propellant mass.
Cuboid in shape of approximately 1.5 m (4 feet 11 inches).
23. The spacecraft's bus is a modified I-1 K structure and propulsion hardware
configurations similar to Chandrayaan 1, India's lunar orbiter that operated from
2008 to 2009, with specific improvements and upgrades needed for a Mars
mission.[31] The satellite structure is of aluminium and composite fibre
reinforced plastic (CFRP) sandwich construction.
24.
25. Assembly of the PSLV-XL launch vehicle, designated C25, started on 5
August 2013. The mounting of the five scientific instruments was
completed at ISRO Satellite Centre, Bangalore, and the finished
spacecraft was shipped to Sriharikota on 2 October 2013 for
integration to the PSLV-XL launch vehicle.
The satellite's development was fast-tracked and completed in a
record 15 months. Despite the US federal government shutdown,
NASA reaffirmed on 5 October 2013 it would provide communications
and navigation support to the mission. ISRO chairman stated in
November 2013 that if the MOM and NASA's orbiter MAVEN were
successful, they would complement each other in findings and help
understand Mars better.
27. LAP Lyman-Alpha Photometer 1.97 kg
MSM Methane Sensor For Mars 2.94 kg
MENCA Mars Exospheric Neutral Composition Analyser 3.56 kg
TIS Thermal Infrared Imaging Spectrometer 3.20 kg
MCC Mars Colour Camera 1.27 kg
The 15 kg (33 lb) scientific payload consists of five instruments:
28. • The 15 kg (33 lb) scientific
payload consists of five
instruments:
• Atmospheric studies Lyman-
Alpha Photometer (LAP) ——
Measuring the
deuterium/hydrogen ratio will
allow to estimate the process
of water loss to outer space.
• Methane Sensor For Mars
(MSM) to check for methane
in the atmosphere of Mars, if
any, and map its sources.
29. • Mars Exospheric Neutral
Composition Analyzer (MENCA) — is
a quadrupole mass analyzer capable
of analyzing the neutral composition
of particles in the exosphere.
• Surface imaging studies Thermal
Infrared Imaging Spectrometer (TIS)
— will measure the temperature
and emissivity of the Martian
surface, this can allow mapping
surface composition and mineralogy
of Mars.
• Mars Colour Camera (MCC) — will
provide images in the visual
spectrum, providing context
information for the other science
instruments
32. TRACKING
• The Indian Deep Space Network will
perform navigation and tracking
operations of this mission, and
NASA's Deep Space Network
provided support services during
the non-visible period of the Indian
Deep Space Network. The signals
from the orbiter take as much as 20
min to reach earth
• Also some of the ships positioned in
south pacific ocean tracked and
coordinate the spacecraft
33. PSLV-C25 carrying the Mars Orbiter Mission spacecraft was launched from
Sriharikota on 5 November 2013.
As originally conceived, ISRO would have launched MOM on its new
Geosynchronous Satellite Launch Vehicle (GSLV), but the GSLV has failed
twice in two space missions in 2010, ISRO is still sorting out issues with its
cryogenic engine, and it was not advisable to wait for the new batch of
rockets since that would have delayed the MOM project for at least three
years. ISRO had to make a choice between delaying the Mars Orbiter Mission
and switching to the less-powerful PSLV.
They opted for the latter. There is no way
to launch on a direct-to-Mars trajectory
with the PSLV as it does not have the
power. Instead, ISRO launched it into
Earth orbit first and slowly boosted it
into an interplanetary trajectory with
the help of gravity assist manoeuvres.
37. The Polar Satellite Launch Vehicle, usually known
by its abbreviation PSLV is the first operational
launch vehicle of ISRO. PSLV is capable of
launching 1600 kg satellites in 620 km sun-
synchronous polar orbit and 1050 kg satellite in
geo-synchronous transfer orbit. In the standard
configuration, it measures 44.4 m tall, with a lift
off weight of 295 tonnes. PSLV has four stages
using solid and liquid propulsion systems
alternately. The first stage is one of the largest
solid propellant boosters in the world and carries
139 tonnes of propellant. A cluster of six strap-
ones attached to the first stage motor, four of
which are ignited on the ground and two are air-
lit.
38. These rockets have launched numerous
communications satellites and earth
observation satellite. On 22 October in 2008,
Chandrayaan-1, India sent its first mission to
the Moon. Over the years, ISRO has
conducted a variety of operations for both
Indian and foreign clients. ISRO's satellite
launch capability is mostly provided by
indigenous launch vehicles and launch sites.
In 2008, ISRO successfully launched its first
lunar probe, Chandrayaan-1, while future
plans include indigenous development of
GSLV, manned space missions, further lunar
exploration, mars exploration and
interplanetary probes. ISRO has several field
installations as assets, and cooperates with
the international community as a part of
several bilateral and multilateral agreements.
5 November 2013, ISRO launched its Mars
Orbiter Mission, which is currently en route to
Mars.
39. The reliability rate of PSLV has been superb. There had been 25
continuously successful flights of PSLV, till April 2014 . With its
variant configurations, PSLV has proved its multi-payload, multi-
mission capability in a single launch and its geosynchronous launch
capability. In the Chandrayaan-mission, another variant of PSLV
with an extended version of strap-on motors, PSOM-XL, the
payload haul was enhanced to 1750 kg in 620 km SSPO. PSLV has
rightfully earned the status of workhorse launch vehicle of ISRO.
1. Lift-off weight 295 tonne
2. Pay Load 1600 kg in to 620 km Polar Orbit,
1060 kg in to Geosynchronous Transfer Orbit (GTO)
3. Height 44 metre
Typical Parameters of PSLV