NNX17AC26G
Project Grant
Overview
Grant Description
Rocket and laboratory experiments in astrophysics -- validation and verification of the next generation FORTIS. We submit herein a proposal describing plans for further development of a next generation far-UV off Rowland-circle telescope for imaging and spectroscopy (FORTIS).
The goal of the proposal is to demonstrate the scientific utility of multi-object spectroscopy over wide angular fields in the far-UV. Investigations include the blue straggler population in the globular cluster M10, low metallicity star formation in the Magellanic Bridge, shock structures in the Cygnus Loop supernova remnant, a search for unidentified emissions in star-forming galaxies, and potentially an as yet unnamed comet as a target of opportunity.
FORTIS is a pathfinder for developing the technologies necessary to enable far-UV spectroscopic surveys. Such surveys will allow us to probe problems relevant to the formation of large scale structures, the origin and evolution of galaxies, and the formation and evolution of stars from interstellar gas. In combination with existing and future spectroscopic surveys, they will provide a complete and compelling panchromatic picture of the observable universe.
Next generation FORTIS will fly as a sounding rocket-borne instrument and incorporate a number of unique technologies, including the next generation microshutter array (NGMSA), which provides for the simultaneous acquisition of spectra from multiple objects within a wide angular field. The NGMSA will be controlled by an autonomous targeting system capable of identifying multiple objects on-the-fly for further spectral analysis in the short time afforded to far-UV observations from a sounding rocket (~400 seconds).
We will also incorporate long-life microchannel plate (MCP) detectors that have high open area ratios, providing for increased quantum efficiency and improved resistance to gain sag, allowing operation at higher count rate. Recent flight experience with the first generation FORTIS has provided guidance to improving the science return of the next generation FORTIS.
Our plans for a rigorous validation and verification of the science and technology is detailed. This program will serve as the basis of doctoral theses for several graduate students, in addition to providing hands-on experience with space science missions to a number of undergraduates. It will enable new science thrusts enabled by new technologies while cultivating new skillsets in the next generation of space scientists.
The goal of the proposal is to demonstrate the scientific utility of multi-object spectroscopy over wide angular fields in the far-UV. Investigations include the blue straggler population in the globular cluster M10, low metallicity star formation in the Magellanic Bridge, shock structures in the Cygnus Loop supernova remnant, a search for unidentified emissions in star-forming galaxies, and potentially an as yet unnamed comet as a target of opportunity.
FORTIS is a pathfinder for developing the technologies necessary to enable far-UV spectroscopic surveys. Such surveys will allow us to probe problems relevant to the formation of large scale structures, the origin and evolution of galaxies, and the formation and evolution of stars from interstellar gas. In combination with existing and future spectroscopic surveys, they will provide a complete and compelling panchromatic picture of the observable universe.
Next generation FORTIS will fly as a sounding rocket-borne instrument and incorporate a number of unique technologies, including the next generation microshutter array (NGMSA), which provides for the simultaneous acquisition of spectra from multiple objects within a wide angular field. The NGMSA will be controlled by an autonomous targeting system capable of identifying multiple objects on-the-fly for further spectral analysis in the short time afforded to far-UV observations from a sounding rocket (~400 seconds).
We will also incorporate long-life microchannel plate (MCP) detectors that have high open area ratios, providing for increased quantum efficiency and improved resistance to gain sag, allowing operation at higher count rate. Recent flight experience with the first generation FORTIS has provided guidance to improving the science return of the next generation FORTIS.
Our plans for a rigorous validation and verification of the science and technology is detailed. This program will serve as the basis of doctoral theses for several graduate students, in addition to providing hands-on experience with space science missions to a number of undergraduates. It will enable new science thrusts enabled by new technologies while cultivating new skillsets in the next generation of space scientists.
Awardee
Grant Program (CFDA)
Awarding / Funding Agency
Place of Performance
Baltimore,
Maryland
21218-2608
United States
Geographic Scope
Single Zip Code
Related Opportunity
None
Analysis Notes
Amendment Since initial award the End Date has been extended from 12/31/21 to 12/31/23 and the total obligations have increased 397% from $662,059 to $3,287,810.
The Johns Hopkins University was awarded
Next Generation FORTIS: Advancing Far-UV Astrophysics through Rocket Experiments
Project Grant NNX17AC26G
worth $3,287,810
from Shared Services Center in January 2016 with work to be completed primarily in Baltimore Maryland United States.
The grant
has a duration of 7 years and
was awarded through assistance program 43.001 Science.
Status
(Complete)
Last Modified 9/20/23
Period of Performance
1/1/17
Start Date
12/31/23
End Date
Funding Split
$3.3M
Federal Obligation
$0.0
Non-Federal Obligation
$3.3M
Total Obligated
Activity Timeline
Transaction History
Modifications to NNX17AC26G
Additional Detail
Award ID FAIN
NNX17AC26G
SAI Number
None
Award ID URI
SAI EXEMPT
Awardee Classifications
Nonprofit With 501(c)(3) IRS Status (Other Than An Institution Of Higher Education)
Awarding Office
80NSSC NASA SHARED SERVICES CENTER
Funding Office
80NSSC NASA SHARED SERVICES CENTER
Awardee UEI
FTMTDMBR29C7
Awardee CAGE
5L406
Performance District
MD-07
Senators
Benjamin Cardin
Chris Van Hollen
Chris Van Hollen
Budget Funding
| Federal Account | Budget Subfunction | Object Class | Total | Percentage |
|---|---|---|---|---|
| Science, National Aeronautics and Space Administration (080-0120) | Space flight, research, and supporting activities | Grants, subsidies, and contributions (41.0) | $4,403,638 | 100% |
Modified: 9/20/23