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Cassini-Huygens -
   Organizing and Running a
     Multifaceted Mission
                Greg Fletcher
      (210) 522-6269, gfletcher@swri.org
Program Manager, Southwest Research Institute




                                                Used with Permission
Outline
• Deep Space Missions
• Cassini-Huygens Mission Background
• Spacecraft Overview
• Project Organization
• Science Payload
• INMS (Ion and Neutral Mass Spectrometer)
• Staffing Plan Management
• Distributed Operations Concept
• Process Driven
• Schedule Driven
• Decision Making
• Secrets to Cassini’s Success

   Southwest Research Institute – Chemistry & Chemical Engineering Division
What are Deep Space Missions
                      All About?

If you’re a scientist:


          It’s all about
          the science!
 Southwest Research Institute – Chemistry & Chemical Engineering Division
What are Deep Space Mission
               About for Program Managers?

It’s all about managing the scientists
and Engineers
and Software Designers
and Budget
and Schedule

If you don’t do it well, it will get
away from you…
  Southwest Research Institute – Chemistry & Chemical Engineering Division
Cassini-Huygens Mission
      Background
Cassini-Huygens Mission
                          Background
• Cassini-Huygens is a joint
NASA/ESA/ASI robotic spacecraft
currently in orbit around Saturn
• Goal is to explore the Saturn
system, with its many moons, and
rings
• Launched on October 15, 1997
• Reached Saturn orbit July 1, 2004
• Huygens Probe landed on the
surface of Titan January 14, 2005
• Cassini Orbiter continues to
collect data studying Saturn, the
Rings, Titan, Saturn’s many other
moons, and Saturn’s
magnetosphere
• Hundreds of scientists and
engineers from the United States
and 16 European countriesChemical Engineering Division
     Southwest Research Institute – Chemistry &
Cassini-Huygens Spacecraft
         Overview
Cassini-Huygens Spacecraft
                        Overview
• Cassini spacecraft, including the
Huygens Probe, is the largest, most
complex interplanetary spacecraft NASA
has flown to date
• Approximately the length of a school bus
from the tip of the main antenna to the
main engines
• Launch mass of approximately 5,600 kg
(12,000 lb), including 3,132 kg (6,900 lb)
of propellants
• Height of 6.8 m (22 ft)
• Main antenna width of 4 meters (13 ft),
though RPWS and MAG stick out the
sides by as much as 9 meters (29 ft
• Over 1,630 interconnected electrical
components
• 22,000 wire connections
• Over 14 km (8.7 mi) of cablesEngineering Division
    Southwest Research Institute – Chemistry & Chemical
Southwest Research Institute – Chemistry & Chemical Engineering Division
Project Organization
Indicates where
the 12 instrument
 PIs/TLs report to
    the project




                                                                                 Indicates where
                                                                               the 12 instrument
                                                                                teams fit into the
                                                                              science and uplink
                                                                                   organization




   Southwest Research Institute – Chemistry & Chemical Engineering Division
Cassini Instrumentation

• 12 instrument teams each based in a different location

CAPS – Southwest Research Institute (SwRI), San Antonio, Tx
CDA – Max Planck Institute for Nuclear Physics, Heidelberg, Germany
CIRS – GSFC, Greenbelt, Md
INMS – Southwest Research Institute (SwRI), San Antonio, Tx
ISS – Space Science Institute, Boulder, Co
MAG – Imperial College, London, UK
MIMI – Applied Physics Labs, Columbia, Md
RADAR – Jet Propulsion Laboratory, Pasadena, Ca
RPWS – University of Iowa, Iowa City, Io
RSS - Jet Propulsion Laboratory, Pasadena, Ca
UVIS – University of Colorado, Boulder, Co
VIMS - Lunar and Planetary Labs, U of Arizona




   Southwest Research Institute – Chemistry & Chemical Engineering Division
INMS (Ion and Neutral Mass
      Spectrometer)
INMS (Ion and Neutral Mass
                     Spectrometer)
• Measures neutral and ion species from 1 to 100 AMU (m/q)
• Designed to measure Titan’s atmosphere, but can measure
any particles that are present in high enough concentrations




  Example of INMS data (spectra)                        Example of INMS data (spectra)
  with basic processing applied Engineering Division
  Southwest Research Institute – Chemistry & Chemical
                                                        with labels showing what is
                                                        represented in each signal group.
INMS Organization By Task




• INMS team is broken into smaller teams by area of
responsibility
• Some members of the team are in more than one group
• Only one person on the team is dedicated full time to Cassini
   Southwest Research Institute – Chemistry & Chemical Engineering Division
INMS Organization By Task




• ScienceTeam
   − Responsible for deciding what types of observations
   INMS should make for each target, like Titan, Enceladus,
   the Rings, and Saturn’s magnetosphere
   − Analyzing data and publishing results
   Southwest Research Institute – Chemistry & Chemical Engineering Division
INMS Organization By Task




• OperationsTeam
   − Creating command files based on the science plan
   − Monitoring health and safety, including long term trends
   − Data production
   − Data archival
   Southwest Research Institute – Chemistry & Chemical Engineering Division
INMS Organization By Task




• Development  Team
     − Design and develop INMS ground system (ION)
     − Design and develop Flight Software
     − Develop analysis toolkit for data processing and analysis
   Southwest Research Institute – Chemistry & Chemical Engineering Division
Tethys   Epimetheus   Enceladus




Hyperion
Staffing Plan Management (1 of
                             2)
• Long duration deep space missions like Cassini present
unique staffing challenges
• New people working on Cassini today were newborns when
the Cassini program office was formed at JPL in 1988
    − Key people retire or are promoted into management roles
• On missions like Cassini, key staff members such as
operations team members can take up to two years to fully train
• Post Doctoral staff members with the right experience can
take years to find
    − In some cases, we take on students as undergraduates,
    and keep them on through their Post-Doc and beyond


   Southwest Research Institute – Chemistry & Chemical Engineering Division
Staffing Plan Management (2 of
                             2)
Good News:
• Having only one full time staff member on INMS allows
flexibility
    − Allows for more people to be cross trained to avoid single
    point failures
    − Scheduling vacations and travel for key people is easier
Bad News:
• Having very few full time employees means that nearly
everyone works on other programs
    − Risk of not having resources available exactly when they
    are needed due to high priority events on other programs
• As a manager you have to decide how to best
staff your program
   Southwest Research Institute – Chemistry & Chemical Engineering Division
Distributed Operations
Distributed Operations
• Distributed operations means the 12 instrument teams are
based in different locations around the world (CDA is in
Heidelberg, Germany, MAG is in London, UK)
• Science and operations for each instrument are run from the
remote sites
• JPL plays the following roles:
      − Program Office (Cassini PM and Project Scientist)
      − Spacecraft Operations (SCO) team
      − Coordination function for science planning
      − Merging, processing and loading instrument and
      spacecraft commanding


   Southwest Research Institute – Chemistry & Chemical Engineering Division
Distributed Operations (cont)

How do scientists, engineers and managers from so many
institutions communicate?




 Telecons
 Telecons
 and more Telecons…

   Southwest Research Institute – Chemistry & Chemical Engineering Division
Distributed Operations (cont)

• Instrument teams’ co-investigators are also distributed at
different sites
• INMS has science team members at:
        - University of California Berkeley
        - University of Kansas
        - Johns Hopkins Applied Physics Labs
        - Goddard Space Flight Center
        - University of Maryland
        - University of Arizona Lunar and Planetary Labs
        - Imperial College, London, UK (Affiliate)
        - Central University, Taiwan


    Southwest Research Institute – Chemistry & Chemical Engineering Division
Distributed Operations (cont)

• Additional communication needs to be facilitated to coordinate
the INMS team internally
    − Weekly Telecons
    − Team meetings two to three times per year
    − Phone calls to team members as necessary




   Southwest Research Institute – Chemistry & Chemical Engineering Division
Disadvantages of Distributed
                            Teams
• Makes communication across the program complicated
   − Scheduling meetings across 18 times zones means that
        some of the teams have to participate at off hours
• During the initial planning of the science timelines there were
as many as 28 hours of telecons per week
   − Smaller teams often only had one or two people covering
   all the these meetings, which doesn’t leave much time for
   getting other work done
   − Leads to consistently working long days for an extended
   period




   Southwest Research Institute – Chemistry & Chemical Engineering Division
Disadvantages of Distributed
                        Teams (cont.)
• High volume of email to keep up with negotiations regarding
details of the plan
• Negotiations between 12 teams is difficult enough in person,
let alone by phone and email




  Southwest Research Institute – Chemistry & Chemical Engineering Division
Advantages of Distributed
                               Teams
• Allows experts from around the world to participate in the
program as instrument PIs
    − PIs are then in turn supported by a science team who are
    experts in relevant fields
• Encourages young people to get involved in space science
by providing funding to Universities and Institutes for graduate
students




   Southwest Research Institute – Chemistry & Chemical Engineering Division
Process and Schedule
Process Driven
• Well documented processes reduce risk by preventing
mistakes
    − No margin for error in spaceflight
    − Mistakes in flight can be catastrophic
• Cassini program has a formal process for delivery and merge
of all instrument and spacecraft subsystem commanding
• INMS Operations team has a checklist for every task we
perform
• Formal review process for INMS instrument commanding prior
to each delivery port
• Process for review of housekeeping data
• Process for responding to flight anomalies
• Process for upload of ‘realtime’ commands
   Southwest Research Institute – Chemistry & Chemical Engineering Division
Schedule Driven
• Most spaceflight missions are schedule driven by hard
deadlines
     − Launch date has a hard window due to trajectory based
     on planetary alignments
     − Command deliveries have hard deadlines based on
     observation events
• If an instrument misses a delivery deadline, they are pulled
from that sequence (and lose about 40 days of observations)
     − On Cassini, no instrument or subsystem has ever
     missed a delivery deadline



   Southwest Research Institute – Chemistry & Chemical Engineering Division
Decision Making
Decision Making
• After the Cassini Spacecraft was designed and the instrument
teams were selected, Congress decided the mission was going
to cost to much
• Decision was made to remove instrument scan platforms and
re-design the spacecraft to hard mount science payloads
• Saved money up front in spacecraft construction
• More than made up for savings in added operational
complexity
    − Drives instrument negotiations for science observations
    − Flight rule constraints are far more complicated
    − Observation designs are more complicated (instrument
    teams actually have to design the spacecraft pointing for
    their observations)
   Southwest Research Institute – Chemistry & Chemical Engineering Division
Decision Making
What is the lesson to be learned from this?

Every decision managers make, effects
everything that happens on the program
from that point on, so…

Good decision making skills are essential
to be a successful program manager

   Southwest Research Institute – Chemistry & Chemical Engineering Division
Tough PM Decisions
• First efforts to create an integrated science plan started
slowly because the scientists assigned to the planning were
creating a timeline that was so complicated it could not be
implemented
    − Program management recognized this within the first
    two weeks and created guidelines to allow the science
    plan to match the workforce available to implement the
    timeline




   Southwest Research Institute – Chemistry & Chemical Engineering Division
Tough PM Decisions
• Huygens team realized they had a problem with Doppler
shift in the transmitter that would cause loss of critical data
    − Solution to this problem was complicated and there
    were a number of decisions and actions taken to remedy
    the problem
    − Single largest action was the Cassini navigation team
    modified the first two orbits around Saturn, changing the
    trajectory for the probe mission without effecting the orbits
    after Rev 3




   Southwest Research Institute – Chemistry & Chemical Engineering Division
Management Challenges
• Facilitating communication among your team, and to other
teams as appropriate
• Spaceflight programs can be very demanding, and teams
are often working against hard deadlines like launch dates or
events in orbit
    − Working long hours is fairly routine, so managers need
    to be careful not to burn out team members
    − Plan the work to be complete well in advance, so there
    is ample time to review and make corrections
• Scientists, engineers and software developers are all very
bright, creative, independent people and are typically
challenging to manage
• Delegate appropriately
    − Spread the work load as evenly as possible
    − Delegate authority with the responsibility
    Southwest Research Institute – Chemistry & Chemical Engineering Division
Secrets to Cassini’s Success


• Effective communication!
• Tremendously talented and dedicated
scientists and engineers who are all vested
in the program’s success
• Cooperation and trust between teams
• Managers who know how to organize,
plan and follow through



 Southwest Research Institute – Chemistry & Chemical Engineering Division
Backup Slides
Cassini Trajectory from Earth to
                       Saturn




Southwest Research Institute – Chemistry & Chemical Engineering Division
Fletcher.greg
Fletcher.greg
Fletcher.greg

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Fletcher.greg

  • 1. Cassini-Huygens - Organizing and Running a Multifaceted Mission Greg Fletcher (210) 522-6269, gfletcher@swri.org Program Manager, Southwest Research Institute Used with Permission
  • 2. Outline • Deep Space Missions • Cassini-Huygens Mission Background • Spacecraft Overview • Project Organization • Science Payload • INMS (Ion and Neutral Mass Spectrometer) • Staffing Plan Management • Distributed Operations Concept • Process Driven • Schedule Driven • Decision Making • Secrets to Cassini’s Success Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 3. What are Deep Space Missions All About? If you’re a scientist: It’s all about the science! Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 4. What are Deep Space Mission About for Program Managers? It’s all about managing the scientists and Engineers and Software Designers and Budget and Schedule If you don’t do it well, it will get away from you… Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 6. Cassini-Huygens Mission Background • Cassini-Huygens is a joint NASA/ESA/ASI robotic spacecraft currently in orbit around Saturn • Goal is to explore the Saturn system, with its many moons, and rings • Launched on October 15, 1997 • Reached Saturn orbit July 1, 2004 • Huygens Probe landed on the surface of Titan January 14, 2005 • Cassini Orbiter continues to collect data studying Saturn, the Rings, Titan, Saturn’s many other moons, and Saturn’s magnetosphere • Hundreds of scientists and engineers from the United States and 16 European countriesChemical Engineering Division Southwest Research Institute – Chemistry &
  • 8. Cassini-Huygens Spacecraft Overview • Cassini spacecraft, including the Huygens Probe, is the largest, most complex interplanetary spacecraft NASA has flown to date • Approximately the length of a school bus from the tip of the main antenna to the main engines • Launch mass of approximately 5,600 kg (12,000 lb), including 3,132 kg (6,900 lb) of propellants • Height of 6.8 m (22 ft) • Main antenna width of 4 meters (13 ft), though RPWS and MAG stick out the sides by as much as 9 meters (29 ft • Over 1,630 interconnected electrical components • 22,000 wire connections • Over 14 km (8.7 mi) of cablesEngineering Division Southwest Research Institute – Chemistry & Chemical
  • 9.
  • 10. Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 12. Indicates where the 12 instrument PIs/TLs report to the project Indicates where the 12 instrument teams fit into the science and uplink organization Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 13. Cassini Instrumentation • 12 instrument teams each based in a different location CAPS – Southwest Research Institute (SwRI), San Antonio, Tx CDA – Max Planck Institute for Nuclear Physics, Heidelberg, Germany CIRS – GSFC, Greenbelt, Md INMS – Southwest Research Institute (SwRI), San Antonio, Tx ISS – Space Science Institute, Boulder, Co MAG – Imperial College, London, UK MIMI – Applied Physics Labs, Columbia, Md RADAR – Jet Propulsion Laboratory, Pasadena, Ca RPWS – University of Iowa, Iowa City, Io RSS - Jet Propulsion Laboratory, Pasadena, Ca UVIS – University of Colorado, Boulder, Co VIMS - Lunar and Planetary Labs, U of Arizona Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 14. INMS (Ion and Neutral Mass Spectrometer)
  • 15. INMS (Ion and Neutral Mass Spectrometer) • Measures neutral and ion species from 1 to 100 AMU (m/q) • Designed to measure Titan’s atmosphere, but can measure any particles that are present in high enough concentrations Example of INMS data (spectra) Example of INMS data (spectra) with basic processing applied Engineering Division Southwest Research Institute – Chemistry & Chemical with labels showing what is represented in each signal group.
  • 16. INMS Organization By Task • INMS team is broken into smaller teams by area of responsibility • Some members of the team are in more than one group • Only one person on the team is dedicated full time to Cassini Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 17. INMS Organization By Task • ScienceTeam − Responsible for deciding what types of observations INMS should make for each target, like Titan, Enceladus, the Rings, and Saturn’s magnetosphere − Analyzing data and publishing results Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 18. INMS Organization By Task • OperationsTeam − Creating command files based on the science plan − Monitoring health and safety, including long term trends − Data production − Data archival Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 19. INMS Organization By Task • Development Team − Design and develop INMS ground system (ION) − Design and develop Flight Software − Develop analysis toolkit for data processing and analysis Southwest Research Institute – Chemistry & Chemical Engineering Division
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  • 21. Tethys Epimetheus Enceladus Hyperion
  • 22. Staffing Plan Management (1 of 2) • Long duration deep space missions like Cassini present unique staffing challenges • New people working on Cassini today were newborns when the Cassini program office was formed at JPL in 1988 − Key people retire or are promoted into management roles • On missions like Cassini, key staff members such as operations team members can take up to two years to fully train • Post Doctoral staff members with the right experience can take years to find − In some cases, we take on students as undergraduates, and keep them on through their Post-Doc and beyond Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 23. Staffing Plan Management (2 of 2) Good News: • Having only one full time staff member on INMS allows flexibility − Allows for more people to be cross trained to avoid single point failures − Scheduling vacations and travel for key people is easier Bad News: • Having very few full time employees means that nearly everyone works on other programs − Risk of not having resources available exactly when they are needed due to high priority events on other programs • As a manager you have to decide how to best staff your program Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 25. Distributed Operations • Distributed operations means the 12 instrument teams are based in different locations around the world (CDA is in Heidelberg, Germany, MAG is in London, UK) • Science and operations for each instrument are run from the remote sites • JPL plays the following roles: − Program Office (Cassini PM and Project Scientist) − Spacecraft Operations (SCO) team − Coordination function for science planning − Merging, processing and loading instrument and spacecraft commanding Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 26. Distributed Operations (cont) How do scientists, engineers and managers from so many institutions communicate? Telecons Telecons and more Telecons… Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 27. Distributed Operations (cont) • Instrument teams’ co-investigators are also distributed at different sites • INMS has science team members at: - University of California Berkeley - University of Kansas - Johns Hopkins Applied Physics Labs - Goddard Space Flight Center - University of Maryland - University of Arizona Lunar and Planetary Labs - Imperial College, London, UK (Affiliate) - Central University, Taiwan Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 28. Distributed Operations (cont) • Additional communication needs to be facilitated to coordinate the INMS team internally − Weekly Telecons − Team meetings two to three times per year − Phone calls to team members as necessary Southwest Research Institute – Chemistry & Chemical Engineering Division
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  • 31. Disadvantages of Distributed Teams • Makes communication across the program complicated − Scheduling meetings across 18 times zones means that some of the teams have to participate at off hours • During the initial planning of the science timelines there were as many as 28 hours of telecons per week − Smaller teams often only had one or two people covering all the these meetings, which doesn’t leave much time for getting other work done − Leads to consistently working long days for an extended period Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 32. Disadvantages of Distributed Teams (cont.) • High volume of email to keep up with negotiations regarding details of the plan • Negotiations between 12 teams is difficult enough in person, let alone by phone and email Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 33. Advantages of Distributed Teams • Allows experts from around the world to participate in the program as instrument PIs − PIs are then in turn supported by a science team who are experts in relevant fields • Encourages young people to get involved in space science by providing funding to Universities and Institutes for graduate students Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 35. Process Driven • Well documented processes reduce risk by preventing mistakes − No margin for error in spaceflight − Mistakes in flight can be catastrophic • Cassini program has a formal process for delivery and merge of all instrument and spacecraft subsystem commanding • INMS Operations team has a checklist for every task we perform • Formal review process for INMS instrument commanding prior to each delivery port • Process for review of housekeeping data • Process for responding to flight anomalies • Process for upload of ‘realtime’ commands Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 36. Schedule Driven • Most spaceflight missions are schedule driven by hard deadlines − Launch date has a hard window due to trajectory based on planetary alignments − Command deliveries have hard deadlines based on observation events • If an instrument misses a delivery deadline, they are pulled from that sequence (and lose about 40 days of observations) − On Cassini, no instrument or subsystem has ever missed a delivery deadline Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 38. Decision Making • After the Cassini Spacecraft was designed and the instrument teams were selected, Congress decided the mission was going to cost to much • Decision was made to remove instrument scan platforms and re-design the spacecraft to hard mount science payloads • Saved money up front in spacecraft construction • More than made up for savings in added operational complexity − Drives instrument negotiations for science observations − Flight rule constraints are far more complicated − Observation designs are more complicated (instrument teams actually have to design the spacecraft pointing for their observations) Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 39. Decision Making What is the lesson to be learned from this? Every decision managers make, effects everything that happens on the program from that point on, so… Good decision making skills are essential to be a successful program manager Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 40. Tough PM Decisions • First efforts to create an integrated science plan started slowly because the scientists assigned to the planning were creating a timeline that was so complicated it could not be implemented − Program management recognized this within the first two weeks and created guidelines to allow the science plan to match the workforce available to implement the timeline Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 41. Tough PM Decisions • Huygens team realized they had a problem with Doppler shift in the transmitter that would cause loss of critical data − Solution to this problem was complicated and there were a number of decisions and actions taken to remedy the problem − Single largest action was the Cassini navigation team modified the first two orbits around Saturn, changing the trajectory for the probe mission without effecting the orbits after Rev 3 Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 42. Management Challenges • Facilitating communication among your team, and to other teams as appropriate • Spaceflight programs can be very demanding, and teams are often working against hard deadlines like launch dates or events in orbit − Working long hours is fairly routine, so managers need to be careful not to burn out team members − Plan the work to be complete well in advance, so there is ample time to review and make corrections • Scientists, engineers and software developers are all very bright, creative, independent people and are typically challenging to manage • Delegate appropriately − Spread the work load as evenly as possible − Delegate authority with the responsibility Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 43. Secrets to Cassini’s Success • Effective communication! • Tremendously talented and dedicated scientists and engineers who are all vested in the program’s success • Cooperation and trust between teams • Managers who know how to organize, plan and follow through Southwest Research Institute – Chemistry & Chemical Engineering Division
  • 45. Cassini Trajectory from Earth to Saturn Southwest Research Institute – Chemistry & Chemical Engineering Division