Essentials of 
Mangalyaan 
OR 
Mars Orbiter Mission ( MOM ) 
An Overview presented by: 
Shashikant Salvi
MANGALYAAN ( मंगलयान ) 
मंगल + यान 
Mangal + Yaan 
Mars + Vehicle 
Indian Satellite for the exploration of Mars 
MARS ORBITER MISSION ( MOM )
Mars is the 4th planet in Solar System.
Physical characteristics of Mars and Earth 
Parameter Mars Earth 
Radius 3390 kms 6371 Kms 
Mass 0.64E24 kg 5.98E24 
Gravitational Acceleration 3.7 m/s2 9.8 m/s2 
Orbital period around Sun 687 days 365 days 
Length of a Day 24Hrs 39 Min 24Hrs 
Tilt of rotation axis 25 deg 23.5deg 
Weight on Mars and Earth 37.7 Kg 100 Kg
Why Mars? 
– Neighbour planet with Earth like features 
– Mars has an atmosphere ( although thin ) 
– Surface features like impact craters, volcanoes, valleys, 
deserts, and polar ice caps 
– Tilt in rotational axis that produces the seasons 
– Mountains and canyons. 
– Two moons, Phobos and Deimos 
Therefore it was explored by spacecrafts and probes from 60s. 
So India’s choice of 1st interplanetary spacecraft was for Mars ( after 
Moon mission, Chandrayaan in 2008 )
TIMING of MOM mission 
In November 2013, two missions started their journey 
from Earth to Mars 
MAVEN of USA on 18th Nov 
MOM of India on 8th Nov ( 1st Dec ) 
They Reached Mars on 22nd and 24th Sept 2014 
Both started from Earth in Nov 2013 time and reached 
Mars in Sept 2014. 
Was it just a coincidence?
Mars is farther from Sun than Earth 
Kepler’s laws state that it has to take more time to make a 
revolution than Earth 
( 687 days for Mars and 365 days for Earth ) 
They come near each other once in 780 days (2 yr 50 days ) 
This year’s situation is shown in next few slides. 
Notice how the Earth-Mars distance varies every month .. In 
right top corner of each slide 
Next possibility after 12th April 2014 is 30th May 2016
1st Feb 14 
Watch this space .. Every month’s 
distance is plotted for comparison 
1st Feb 2014
1st Feb 14 
1st Mar ‘14 
1st March 2014 
Distance between 
Earth and Mars
1st Feb 14 
1st Mar ‘14 
1st Apr ‘14 
1st April 2014 
Distance between 
Earth and Mars
1st Feb 14 
1st Mar ‘14 
1st Apr ‘14 
14th Apr ‘14 
14th April 2014 
Distance between 
Earth and Mars
1st Feb 14 
1st Mar ‘14 
1st Apr ‘14 
14th Apr ‘14 
1st May ‘14 
1st May 2014 
Distance between 
Earth and Mars
- Mars and Earth are nearest on 14th April 2014. 
(≈ 0.5 AU , 92 million kms ) 
- They were in Opposition on 8th April 2014 
- So MOM was launched such that its position on 8th 
April is exactly midway ( 343 million kms done and 343 
million kms remaining ) 
343 
686 
800 
700 
600 
500 
400 
300 
200 
100 
0 
2013-Dec-02 
2013-Dec-17 
2014-Jan-01 
2014-Jan-16 
2014-Jan-31 
2014-Feb-15 
2014-Mar-02 
2014-Mar-17 
2014-Apr-01 
2014-Apr-16 
2014-May-01 
2014-May-16 
2014-May-31 
2014-Jun-15 
2014-Jun-30 
2014-Jul-15 
2014-Jul-30 
2014-Aug-14 
2014-Aug-29 
2014-Sep-13
Transportation of satellite from one planet to the 
other using Sun is known as Hohemann Transfer 
MOM and MAVEN travelled from Earth to Mars on 
two slightly different elliptical paths with Sun as 
one of the focus
MOM aboard PSLV C25 Rocket 
MOM 
Heat 
shield 
4th 
Stage 
Heat shield 
open 
Heat 
shield 
Closed 
Feed Line 
for MOM
1st 
Stage 
Mobile 
Service Tower 
( MST ) 
Launch 
Pedestal 
Umbilical 
Tower 
Feed lines 
How Big is the PSLV? 
Compare with people on the MST 
Feed lines for liquid propellants , 
high-pressure gases, checkout 
cables, chilled air
MOM is basically a Demonstration Mission 
• Scientific Objectives 
- Usage of indigenous scientific Instruments for 
Martian Study 
• Technological Objectives 
Demonstrate the ability to 
- Design a satellite to survive Martian conditions 
- Design Interplanetary orbit and later 
- Achieve and operate Mars orbit
Scientific Objectives 
Demonstrate the usage of indigenous 
scientific instruments for Exploration of 
- Mars surface features 
- morphology 
- mineralogy and 
- Martian atmosphere
Technological Objectives of MOM 
- Design an orbiter to survive Martian conditions 
- Design cruise phase of 300 days 
- Achieve and operate Mars orbit 
- Establish and evaluate 
navigation 
Deep space communication 
mission planning and management 
- Incorporate autonomous features to handle 
contingency situations.
80238 Kms 
3807 Kms 
Orbit of MOM around Mars 
418 Kms 
76847 Kms 
Apoapsis 
Major Axis 
Periapsis
Measuring Instruments on MOM 
Mars Orbiter Mission carries 
- camera ( MCC ) 
- two spectrometers ( MENCA and TIS ) 
- radiometer ( MSM ) 
- photometer ( LAP ) 
These instruments are used to study 
- Martian surface 
- atmosphere and 
- exosphere extending up to 80,000 kms 
to understand evolution of that planet and 
geologic and biogenic processes ( if possible )
Location of various Components 
Propellant Tank 
High Gain 
Antenna 
Feed Horn 
High Gain 
Antenna 
Reflector 
Reaction 
Wheel 
TTC Antenna 
PITCH 
YAW 
ROLL
Mars Colour Camera (MCC) 
( usead for optical imaging ) 
Has three color imaging sensor to obtain images of 
surface features and weather of Mars and its two 
Moons Phobos & Deimos 
Lyman Alpha Photometer (LAP) 
( Study of Escape processes of Martian upper 
atmosphere through Deuterium/Hydrogen ) 
This is an absorption cell photometer which 
measures D/H (Deuterium to Hydrogen Ratio) in 
the Martian upper atmosphere. 
To Study the loss of water from the planet.
The Two spectrometers aboard 
- Mars Enospheric Neutral Composition Analyser 
(MENCA) 
( To Study of the composition of Martian upper 
atmosphere ) 
This is a quadruple mass spectrometer based on 
proven CHACE (Chandra’s Altitudinal Composition 
Explorer) design used in Chandrayaan mission. 
- Thermal Infrared Imaging Spectrometer(TIS) 
( To study surface composition and mineralogy ) 
Measures the thermal emission during day and 
night. With this Temperature and emissivity are 
estimated.
Methane Sensor for Mars (MSM) 
( Detection of Methane ( CH4 ) presence ) 
MSM measures solar radiation reflected by 
Martian atmosphere. Works over illuminated 
scene only 
Derives spatial and temporal variations of 
Methane concentration in the Martian 
atmosphere
1st image obtained 
within minutes after MOI 
1st image fitted on 
Google Mars Atlas
1st image of Martian Atmosphere 
obtained shortly after MOI
1st image of Full disk of Mars 
obtained shortly after MOI 
Same image enhanced by a non-ISRO 
enthusiast identifies locations
http://indiaspaceactivity.blogspot.com/ 
http://salviblogs.blogspot.com/

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Mangalyaan mom maven essentials

  • 1. Essentials of Mangalyaan OR Mars Orbiter Mission ( MOM ) An Overview presented by: Shashikant Salvi
  • 2. MANGALYAAN ( मंगलयान ) मंगल + यान Mangal + Yaan Mars + Vehicle Indian Satellite for the exploration of Mars MARS ORBITER MISSION ( MOM )
  • 3. Mars is the 4th planet in Solar System.
  • 4. Physical characteristics of Mars and Earth Parameter Mars Earth Radius 3390 kms 6371 Kms Mass 0.64E24 kg 5.98E24 Gravitational Acceleration 3.7 m/s2 9.8 m/s2 Orbital period around Sun 687 days 365 days Length of a Day 24Hrs 39 Min 24Hrs Tilt of rotation axis 25 deg 23.5deg Weight on Mars and Earth 37.7 Kg 100 Kg
  • 5. Why Mars? – Neighbour planet with Earth like features – Mars has an atmosphere ( although thin ) – Surface features like impact craters, volcanoes, valleys, deserts, and polar ice caps – Tilt in rotational axis that produces the seasons – Mountains and canyons. – Two moons, Phobos and Deimos Therefore it was explored by spacecrafts and probes from 60s. So India’s choice of 1st interplanetary spacecraft was for Mars ( after Moon mission, Chandrayaan in 2008 )
  • 6. TIMING of MOM mission In November 2013, two missions started their journey from Earth to Mars MAVEN of USA on 18th Nov MOM of India on 8th Nov ( 1st Dec ) They Reached Mars on 22nd and 24th Sept 2014 Both started from Earth in Nov 2013 time and reached Mars in Sept 2014. Was it just a coincidence?
  • 7. Mars is farther from Sun than Earth Kepler’s laws state that it has to take more time to make a revolution than Earth ( 687 days for Mars and 365 days for Earth ) They come near each other once in 780 days (2 yr 50 days ) This year’s situation is shown in next few slides. Notice how the Earth-Mars distance varies every month .. In right top corner of each slide Next possibility after 12th April 2014 is 30th May 2016
  • 8. 1st Feb 14 Watch this space .. Every month’s distance is plotted for comparison 1st Feb 2014
  • 9. 1st Feb 14 1st Mar ‘14 1st March 2014 Distance between Earth and Mars
  • 10. 1st Feb 14 1st Mar ‘14 1st Apr ‘14 1st April 2014 Distance between Earth and Mars
  • 11. 1st Feb 14 1st Mar ‘14 1st Apr ‘14 14th Apr ‘14 14th April 2014 Distance between Earth and Mars
  • 12. 1st Feb 14 1st Mar ‘14 1st Apr ‘14 14th Apr ‘14 1st May ‘14 1st May 2014 Distance between Earth and Mars
  • 13. - Mars and Earth are nearest on 14th April 2014. (≈ 0.5 AU , 92 million kms ) - They were in Opposition on 8th April 2014 - So MOM was launched such that its position on 8th April is exactly midway ( 343 million kms done and 343 million kms remaining ) 343 686 800 700 600 500 400 300 200 100 0 2013-Dec-02 2013-Dec-17 2014-Jan-01 2014-Jan-16 2014-Jan-31 2014-Feb-15 2014-Mar-02 2014-Mar-17 2014-Apr-01 2014-Apr-16 2014-May-01 2014-May-16 2014-May-31 2014-Jun-15 2014-Jun-30 2014-Jul-15 2014-Jul-30 2014-Aug-14 2014-Aug-29 2014-Sep-13
  • 14. Transportation of satellite from one planet to the other using Sun is known as Hohemann Transfer MOM and MAVEN travelled from Earth to Mars on two slightly different elliptical paths with Sun as one of the focus
  • 15. MOM aboard PSLV C25 Rocket MOM Heat shield 4th Stage Heat shield open Heat shield Closed Feed Line for MOM
  • 16. 1st Stage Mobile Service Tower ( MST ) Launch Pedestal Umbilical Tower Feed lines How Big is the PSLV? Compare with people on the MST Feed lines for liquid propellants , high-pressure gases, checkout cables, chilled air
  • 17. MOM is basically a Demonstration Mission • Scientific Objectives - Usage of indigenous scientific Instruments for Martian Study • Technological Objectives Demonstrate the ability to - Design a satellite to survive Martian conditions - Design Interplanetary orbit and later - Achieve and operate Mars orbit
  • 18. Scientific Objectives Demonstrate the usage of indigenous scientific instruments for Exploration of - Mars surface features - morphology - mineralogy and - Martian atmosphere
  • 19. Technological Objectives of MOM - Design an orbiter to survive Martian conditions - Design cruise phase of 300 days - Achieve and operate Mars orbit - Establish and evaluate navigation Deep space communication mission planning and management - Incorporate autonomous features to handle contingency situations.
  • 20. 80238 Kms 3807 Kms Orbit of MOM around Mars 418 Kms 76847 Kms Apoapsis Major Axis Periapsis
  • 21. Measuring Instruments on MOM Mars Orbiter Mission carries - camera ( MCC ) - two spectrometers ( MENCA and TIS ) - radiometer ( MSM ) - photometer ( LAP ) These instruments are used to study - Martian surface - atmosphere and - exosphere extending up to 80,000 kms to understand evolution of that planet and geologic and biogenic processes ( if possible )
  • 22. Location of various Components Propellant Tank High Gain Antenna Feed Horn High Gain Antenna Reflector Reaction Wheel TTC Antenna PITCH YAW ROLL
  • 23. Mars Colour Camera (MCC) ( usead for optical imaging ) Has three color imaging sensor to obtain images of surface features and weather of Mars and its two Moons Phobos & Deimos Lyman Alpha Photometer (LAP) ( Study of Escape processes of Martian upper atmosphere through Deuterium/Hydrogen ) This is an absorption cell photometer which measures D/H (Deuterium to Hydrogen Ratio) in the Martian upper atmosphere. To Study the loss of water from the planet.
  • 24. The Two spectrometers aboard - Mars Enospheric Neutral Composition Analyser (MENCA) ( To Study of the composition of Martian upper atmosphere ) This is a quadruple mass spectrometer based on proven CHACE (Chandra’s Altitudinal Composition Explorer) design used in Chandrayaan mission. - Thermal Infrared Imaging Spectrometer(TIS) ( To study surface composition and mineralogy ) Measures the thermal emission during day and night. With this Temperature and emissivity are estimated.
  • 25. Methane Sensor for Mars (MSM) ( Detection of Methane ( CH4 ) presence ) MSM measures solar radiation reflected by Martian atmosphere. Works over illuminated scene only Derives spatial and temporal variations of Methane concentration in the Martian atmosphere
  • 26. 1st image obtained within minutes after MOI 1st image fitted on Google Mars Atlas
  • 27. 1st image of Martian Atmosphere obtained shortly after MOI
  • 28. 1st image of Full disk of Mars obtained shortly after MOI Same image enhanced by a non-ISRO enthusiast identifies locations