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Research Spending & Results

Award Detail

Awardee:UNIVERSITY OF HAWAII SYSTEMS
Doing Business As Name:University of Hawaii
PD/PI:
  • Mark Chun
  • (808) 956-7800
  • mchun@ifa.hawaii.edu
Co-PD(s)/co-PI(s):
  • Christoph Baranec
Award Date:06/10/2019
Estimated Total Award Amount: $ 1,154,117
Funds Obligated to Date: $ 1,154,117
  • FY 2019=$1,154,117
Start Date:09/01/2019
End Date:08/31/2022
Transaction Type:Grant
Agency:NSF
Awarding Agency Code:4900
Funding Agency Code:4900
CFDA Number:47.049
Primary Program Source:040100 NSF RESEARCH & RELATED ACTIVIT
Award Title or Description:A new adaptive secondary mirror for astronomy
Federal Award ID Number:1910552
DUNS ID:965088057
Parent DUNS ID:009438664
Program:ADVANCED TECHNOLOGIES & INSTRM
Program Officer:
  • Peter Kurczynski
  • (703) 292-7248
  • pkurczyn@nsf.gov

Awardee Location

Street:2440 Campus Road, Box 368
City:HONOLULU
State:HI
ZIP:96822-2234
County:Honolulu
Country:US
Awardee Cong. District:01

Primary Place of Performance

Organization Name:University of Hawaii
Street:640 N. Aohoku Place
City:Hilo
State:HI
ZIP:96720-2700
County:Hilo
Country:US
Cong. District:02

Abstract at Time of Award

Adaptive optics (AO) removes aberrations in starlight caused by the turbulent atmosphere. It greatly enhances astronomical observations from ground-based telescopes. This project will develop a more capable and reliable AO system than currently exists. The main technical advance will be an innovative adaptive secondary mirror. This optical element combines a part of the telescope with a part of the AO system. It simplifies the optics and improves performance. This project will have a broad impact on major ground-based observatories. It will reduce the complexity and improve the reliability of AO, which is essential for these observatories. The project will also support both undergraduate and graduate students, and it will engage high school students as summer interns. An AO system with its correcting element integrated into the telescope optics is an ideal implementation since it simplifies the optics, maximizes the system sensitivity, and provides both narrow-field high-resolution and wide-field modest resolution observations free of the optical blurring from the atmosphere. This enables unique science at very high angular resolution at infrared wavelengths and roughly doubles the survey efficiency of wide-field observations. However, current adaptive secondary mirrors are expensive, complex, and suffer from a range of failure modes. These limitations arise from the choice of the type of actuator and are not fundamental. This project will deploy an adaptive secondary mirror on the University of Hawaii 2.2-meter telescope based on a new actuator technology developed by collaborators at The Netherlands Organization for Applied Research (TNO). The new actuator has a linear displacement with input command, produces a higher force actuation, and is more efficient than the voice-coil actuators used in current systems. This will result in a simpler, more capable, and more reliable adaptive secondary mirror. This work is critical for the next generation extremely large telescopes where an adaptive secondary mirror will need to be very reliable. In addition, by reducing cost, this project can bring adaptive secondaries within the reach of smaller aperture telescopes. This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

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