Amer v2

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DEVELOPMENT OF UNCERTAINTY FACTORS FROM HISTORICAL NASA PROJECTS Dr. Tahani Amer, OE/IPAO NASA-HQ Dr. Will Jarvis, OE/IPAO NASA-HQ Dr. Ariel Pinto, Old Dominion University NASA Program Management Challenge 2012 This briefing is for status only and does not represent complete release of usage.

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Transcript of Amer v2

 DEVELOPMENT OF UNCERTAINTY FACTORS FROM 

HISTORICAL NASA PROJECTS 

Dr. Tahani Amer, OE/IPAO NASA-HQDr. Will Jarvis, OE/IPAO NASA-HQ

Dr. Ariel Pinto, Old Dominion University

NASA Program Management Challenge 2012 This briefing is for status only and does not represent complete release of usage.

Project Background

• Uncertainty analysis should be performed to capture the program risks.

• NASA has been using available uncertainty factors from Aerospace, Air Force, and Booz Allen Hamilton.

• NASA has no insight into the development of these factors, which can lead to unrealistic risks in most NASA projects.

• SRB analysis requires cost growth factors that are transparent and based on recent NASA experience.

• Better estimation and prediction of missions cost is needed early on.

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Data Collection Methodology 

• NASA Fiscal Year Budget Estimates

• Cost Analysis Data Requirement (CADRe)

• Government Accountability Office Reports

• NASA Personal- IPAO/CAD/SMD

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Data Collection Model

GAO Report

Budget Report

Analysis- Recheck

Analysis- Recheck

Assess Assess Assess

CA

DR

e R

epo

rt Data S

et

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5

FY 2009 BudgetFebruary 4, 2008

Amer DENG

Source of Data

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Data Sampling Criteria

• Difficulty in collecting accurate data – limited dataset

• Criteria– Science Mission Projects– Developmental Phase– Only cost data– Use CARDe data as final for completed Missions– For active missions: used in search of credible earliest available

and latest available estimates. Errors probably exist because some projects are still in development and continue to evolve

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Summary of NASA Missions Investigated

Completed Missions Active Missions

NEARLUNAR PROSPECTOR GENESISMESSENGERMARS PATHFINDER STARDUST CONTOURDEEP IMPACT MGSMCO/MPL

MERMRO FAST SWAS TRACE WIRE ACE FUSE IMAGEMAP

HESSI GALEX SWIFT GRACE CLOUDSAT CALIPSODS-1EO-1SIRTFSTEREO

EOS-Aqua EOS-Aura LANDSAT-7TRMM TIMEDGRAVITY PROBE B THEMISHETE-II SORCEICESAT

AIM DAWN PHOENIX GLAST KEPLER SDOWISENEW HORIZONS LROOCO

JUNO AQUARIUS LDCMNPP GPM MMS JWSTMSL GLORYGRAIL

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Initial & Final Cost for 50 Completed Projects and Cost Growth Percentage 

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60 NASA Missions - Historical Data

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Mission Cost Growth Histogram

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NASA & DOD Distribution

0

2

4

6

8

10

12

14

Num

ber o

f Pro

ject

-21-0% 0 -10% 10-20% 20-30% 30-40% 40-50% 50-60% 60-70% >70%

Permission from McCrillis, DOD

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60 NASA Missions

0

2

4

6

8

10

12

14

Num

ber o

f Pro

ject

- 21-0% 0 -10% 10-20% 20-30% 30-40% 40-50% 50-60% 60-70% >70%

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Reasons for Cost Growth

• The major categories for cost growth:

– Overly optimistic and unrealistic initial cost estimates– Project instability and funding issues– Problems with development of instruments and other spacecraft

technology– Launch service issues– “Stuff” Happens

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Level Optimistic Most Likely Pessimistic

Low 0.95 1 1.1

Low Plus 0.96 1 1.23

Moderate 0.97 1 1.36

Moderate Plus 0.98 1 1.49

High 0.98 1 1.61

High Plus 0.99 1 1.74

Very High 1 1 1.87

Very High Plus 1 1 2

Aerospace Air Force

Booz Allen Hamilton

Uncertainly Factors from non-NASA Missions

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NASA  Data & Air Force UF

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NASA  Data & Aerospace UF

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NASA  Data & BAH UF

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Development of Distribution-54

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Development of Distribution-44

Lognormal

Cost Growth (%)1501401301201101009080706050403020100

PD

F

0.12

0.11

0.1

0.09

0.08

0.07

0.06

0.05

0.04

0.03

0.02

0.01

0

F(X) =

µ= 3.03σ= 1.08

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More Test Runs

• All data including Project A & B (A- Data), 54 missions.• All data excluding Project A & B (B- Data), 52 missions.• All completed missions (C-Data), 44 missions.• All data less than 100% cost growth (D- Data).

Type of Data µ =Mean σ= Std Dev.

A - Data 3.01

20.3 %

1.18

B - Data 2.92=

18.5 %

1.11

C - Data 3.03

Mean=37.08

Median= 20.7

Std. Dev.= 55.14

1.08

D-Data 2.85

17.3%

1.07

October 7, 2011 Lognormal

Cost Growth (%)1501401301201101009080706050403020100

PD

F

0.12

0.11

0.1

0.09

0.08

0.07

0.06

0.05

0.04

0.03

0.02

0.01

0

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Selected Distribution 

• The lognormal distribution is the most suitable distribution that the cost estimator can use to perform an uncertainty analysis for the NASA data.

• The quality of the fit of two tests: – The Kolmogorov-test – The Anderson-Darling test

Lognormal (1.08; 3.03)

Cost Growth (%)100500

PD

F

0.032

0.028

0.024

0.02

0.016

0.012

0.008

0.004

0

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Recommended UFs

Level of RiskUncertainty Factors  

 No- Risk Adjusted Conservative Aggressive

Moderate (10-30%) 1 1.1 1.3

High (30-75%) 1 1.3 1.75

Very High (>75%) 1 1.75 2.5

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UFs w/Conservative High Risk Level

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UFs w/Aggressive Moderate Risk Level

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Guideline to UFs

• Cost Analyst Judgment

• Mission Complexity: Number of Instruments, Technical Development

• Heritage Level

• Partners Performance

• Mission Visibility: International & Commercial

• Similarity of Missions

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Comparison of UFs

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UFs ------Test Case

– Project A---• Development Cost as of 2006 ~ $969 M• Development Cost as of 2011 ~ $1.8 B• Apply NUFs:

– Make the following assumptions:» High Risk Mission (10 instruments, new Technology, Planetary)» Aggressive Risk » Select a range from NUFs, Table 20, 1.75-2.5

• Expected development estimate range: 1.69- $2.42 B• Other factors estimates:

– AF (1.61- 1.74) $1.56B- $1.69 B, which is lower than the current actual development cost.

– Aerospace (2.05-2.5) $1.99- $2.52 B, which is much higher then expected estimate from the low range. Note: LCC is @$2.5B.

– BAH (1.9-2.10) $1.84- $2.03 B, which is might be closer to the expected development cost . Note: see section 3.3 for these factors interpolation from BAH table.

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UFs Test Case

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.

Current EST.

970 1.2 1.4 1.8 2.2 2.6 2.8

UF

AF

AS

BAH

$1.69- $2.42B

$1.56B- $1.69B

$1.99- $2.52B

$1.84- $2.03B

Conclusions

• This research provides an important contribution to the discipline of cost estimating.

• It has developed a solid database of actual cost growth history and adds some statistical rigor to the derivation of cost growth factors based on the data.

• Thoughtful execution and effective monitoring of the NUFs will improve the cost estimating.

• Additionally, it is expected that this work will be referenced often for independent cost estimates, correction of advocacy-bias in project-generated estimates, and other programmatic work.

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Point Taken

• The greatest benefit of this research is providing a proactive approach to make a quick cost estimating as in back of envelope by:

– Program Managers– Decision Makers– Congressional Staffer– Cost analysts– Awareness and reference to Standard Review Board

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Future Work

• Increase the number of historical missions captured in the database.

• Validate UFs with more available actual cost data.

• Test the UFs for missions in various life-cycle phases.

• Develop a more adaptable tool for NUFs.

• Accept the UFs by the cost analysis’ community for implementation.

• Develop Agency standard.

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Backup

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