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EXPANDING THE FRONTIERS OF SPACE ASTRONOMY Advancing Technologies for future Segmented Telescopes Russell B. Makidon Optics Laboratory Laurent Pueyo for STScI HiCAT team

Advancing Technologies for future Segmented Telescopes · 2021. 1. 13. · Juanola-Parramon et al. (2019) First result with fully segmented aperture Contrast with monolithic aperture

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Page 1: Advancing Technologies for future Segmented Telescopes · 2021. 1. 13. · Juanola-Parramon et al. (2019) First result with fully segmented aperture Contrast with monolithic aperture

EXPANDING THE FRONTIERS OF S PACE AS TRONOMY

Advancing Technologies for future Segmented Telescopes

Russell B. Makidon Optics Laboratory

Laurent Pueyo for STScI HiCAT team

Page 2: Advancing Technologies for future Segmented Telescopes · 2021. 1. 13. · Juanola-Parramon et al. (2019) First result with fully segmented aperture Contrast with monolithic aperture

High contrast imaging with segmented apertures

FACT SHEET

MONITOR THE SOLAR SYSTEM IN HIGH DEFINITION

2.4-m space telescope 8-m LUVOIR-B 15-m LUVOIR-A

REVEAL THE FORMATION OF COSMIC STRUCTURE AND THE EVOLUTION OF GALAXIES

LARGE UV / OPTICAL / INFRARED SURVEYOR

TELLING THE STORY OF LIFE IN THE UNIVERSE

CHARACTERIZE LARGE NUMBERS OFDIVERSE EXOPLANETS

FIND EARTH-LIKE WORLDS ANDSEARCH FOR SIGNS OF LIFE

Pluto

https://asd.gsfc.nasa.gov/luvoir/

What we want. What we are working on.

Juanola-Parramon et al. (2019)

Page 3: Advancing Technologies for future Segmented Telescopes · 2021. 1. 13. · Juanola-Parramon et al. (2019) First result with fully segmented aperture Contrast with monolithic aperture

First result with fully segmented aperture

Contrast with monolithic aperture 6e-8

Contrast with segmented aperture 2e-7 (partial calibration, circa December 2020)

Co

ron

agra

ph

WF

sen

sin

g &

co

ntr

ol

Segmented DM

Page 4: Advancing Technologies for future Segmented Telescopes · 2021. 1. 13. · Juanola-Parramon et al. (2019) First result with fully segmented aperture Contrast with monolithic aperture

Wavefront Maintenance under in the presence of artificial drifts

• Unobstructed monolithic aperture

• 0.01 nm random drift per iteration (4000 iterations)

• 8e-8 stable contrast over 6 hours compared to 4e-7 open loop measured contrast

• Susan Redmond (PhD student Princeton), SPIE astronomical instrumentation 2020