We therefore propose to test the expectations concerning the physico-chemical evolution of protoplanetary disks via high resolution IR through MM-/cmwave spectroscopy of disks and comets. Through…

Ended Cooperative Agreement Awarded Last action

Contract number
NNX15AT33A
Awardee
Awarding agency
Obligated
$424,733

Award facts

Contract value 100% obligated
$424,732.99 Current and potential, with all options
Completion date 100% complete
Current and potential, with all options
NAICS code
Not on record
Set-aside
No set-aside
Competition
Not Competed · 0 offers Basic Research
Pricing
Other
Place of performance
Pasadena, CA 91125, USA

Award details come from SAM.gov/FPDS.

Transactions

Action Obligated Date
Other Administrative Action 9 $0
Funding Only Action 10 -$0
Other Administrative Action 8 $0
Other Administrative Action 7 $0
Funding Only Action 6 $57,174
Funding Only Action 5 $32,868
Funding Only Action 4 $76,847
Funding Only Action 3 $10,572
Funding Only Action 2 $84,872
Funding Only Action 1 $82,400
Original award $80,000
Show all 11

About this award

This is a $424,732.99 Cooperative Agreement awarded by the National Aeronautics and Space Administration (NASA) to the California Institute of Technology (Caltech) to conduct research on the physico-chemical evolution of protoplanetary disks. The research will use high-resolution infrared through millimeter-/centimeter-wave spectroscopy of disks and comets to test expectations. The key objectives are to conduct detailed studies involving statistically significant samples. This award is not set aside and is part of NASA's "Origin and Evolution of Organics and Water in Planetary System" major program. Caltech is a private research university that has received over $500 million in prime federal contract awards over the past 5 years, primarily from NASA and the Department of Defense, in areas such as space technology, quantum computing, and scientific research.

Description

We therefore propose to test the expectations concerning the physico-chemical evolution of protoplanetary disks via high resolution IR through MM-/cmwave spectroscopy of disks and comets. Through extensive nirspec m-band spectroscopy we have confirmed that CO is indeed a widespread t racer in classical and transitional disks. Spectro-astrometric observations of the CO v= l --to band have confirmed the expected keplerian velocity fields and "imaged" the disk gas down to scales of 0.1 AU. The key to future progress are detailed studies involving statistically significant samples, which forms the basis of this proposal.

Quick answers

Who was awarded contract NNX15AT33A?

NNX15AT33A was awarded to California Institute Of Technology by Shared Services Center (National Aeronautics and Space Administration) on October 1, 2015.

How much is contract NNX15AT33A worth?

The government has obligated $424,733 on NNX15AT33A.

Was contract NNX15AT33A competed?

The extent of competition for NNX15AT33A was not competed. The government received 0 offers.

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