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Progress on the Development of Astronomy,
Polar Science and Space Science in Thailand
1
Boonrucksar Soonthornthum, NARIT
2 March 2018
SE Asia Galaxy Forum 2018
National Astronomical Research Institute
of Thailand
Established since 1 January 2009
under the Ministry of Science and Technology
2
NARIT’s Headquarter “Princess Sirindhorn AstroPark”
@ 260 Moo 4, Donkaew, Mae Rim District, Chiang Mai (22 acres)
Functions
• Main Administration Office of NARIT
• Advanced Research Laboratories: High Performance Computing,
Optics, Radio Frequencies
• Workshops: High Precision Machining, Mechatronics, Mirror
Coating
• Observatory and Planetarium for Public
NARIT’s Key Sciences
1. Impact from Space: The first key science deals with investigating how
space weather affects the upper atmosphere, as well as how the upper
atmosphere affects the lower atmosphere and vice versa. It also aims to
study the effect of man on earth’s climate.
2. Understanding Physics of the Universe: The key science comprises
several fields in stellar physics, including the study of the extremes of the
Universe (i.e. gamma ray burst, compact objects) and the study of stellar
evolutionary process. A few highlighted research topics in this key
science are: variable stars and binary systems, star formation, and stellar
population study.
3. Exoplanets and Astrobiology: The key science focuses on the search for
new exoplanets using various observational techniques, the study of the
physical properties of exoplanets and the understanding of planetary
formation, the exploration of the earth-like exoplanets with habitable
zone and clues of lives outside the Solar system.
4. Understanding the Origin of the Cosmos: The key science focuses on
the key questions of modern cosmology and physics: What causes the
late-time accelerated expansion of the Universe? What is the Dark
Matter? And how do the large-scale structures (e.g. galaxies, groups and
clusters of galaxies) form and evolve?
NARIT’s Major Infrastructures
NARIT’s
Astronomy
Infrastructure
Thai National Observatory,
2.4-m Thai National Telescope, TNT
Major Instruments
• ULTRASPEC
• 4k x 4k CCD Camera
• Medium Resolution
Spectrograph (MRES)
Thai Remote Telescope Network (TRTN)
Cerro Tololo
Inter-American
Observatory
(CTIO)
Republic of
Chile
Gao Mei Gu Observatory,
Lijiang, P.R. of China
Sierra Remote Observatory,
California, U.S.A.
Springbrook Observatory,
Queensland, Australia
GOTO Project at La Palma
Canary Island, Spain
High Performance Computer cluster
Hardware (”Chalawan” Cluster)
 1 Management node (12 cores, 2.4 GHz Intel Xeon E5-26xx v3)
 19 compute nodes (rack + Blade servers)
• CPU 496 cores (@ 2.6GHz clock speed)
• Memory 2.2TB
• Infiniband FDR 56Gbps interconnect
• 2 Intel Xeon Phi Coprocessors (112 cores @ 1.2GHz)
 Storage: Lustre 90TB over IB FDR
 Rpeak= 22 TeraFLOPS
National Network on Radio Astronomy and Geodesy
NARIT’s 40-meter Radio Telescope
- `Updated’ version of IGN’s
40m Yebes Radio Telescope
- 40m Diameter with Parabolic
Surface, Cassegrain-Nasmyth
optics
- total surface accuracy<200 um
(rms)
- Slew: 3 m/s in Azimuth , 1 m/s
in Vertical
- Pointing: 2” (no wind),
6” (5 m/s wind)
- Prime-focus receiver
mechanism
Yebes, 23 March 2017
Thailand-China Collaboration on
VLBI Geodesy under “One Belt’ One
Road” policy of Chinese’s government
NARIT’s 13m VGOS (VLBI
Global Observing System) antenna for
a very precise plate tectonic
measurement
13m VGOS Zelenchukskaya (RU) 13m VGOS GGAO (US)
NARIT-NAOC MoU April 5 2017
14
FAST Radio Telescope
Astronomyand Atmospheric
Science inthe PolarRegion
Astronomy at Polar Region
Polar region (Arctic/Antarctic Plateau) is
a perfect place for astronomical observations
due to its
- Long and continuous 6 months dark clear
winter sky
- Stable atmospheric condition with
excellent sky seeing
We can do the long-term, unbroken and
continuous monitoring of various types of
celestial objects eg: binary stars, variable
stars, exoplanets, transient phenomena,
exploding stars ect. Also the investigations of
the aurora phenomena on earth.
HRH Princess Maha Chakri Sirindhorn’s visits to China
18
MoU Signing with Polar Research Institute of China (PRIC)
6 April 2016
NARIT’s Antarctic Research Topics (Under
PRIC-NARIT Collaboration
1. Exo-planets/ Exo-earths Detection
2. Variable Stars, Transient Phenomena
3. Stellar Seismology: Vibrations of
stars/Starquakes
4. Growth of Supermassive Black Holes and Co-
evolution of Host Galaxies
5. Pipeline development for wide-field photometry
6. A cooperation on the construction of a 1-meter
telescope for spectroscopy in Antarctic
7. Astronomical and upper atmosphere physical
instruments operated at Chinese Stations
Join Bright Stars Survey Telescope (BSST)
Project at Zhongshan Station, Antarctica, 2016
(30 cm aperture, 3.4ºx 3.4º Field of View)
TEST in April-May 2015)
Collaboration with East Asian Observatory
(EAO)
21
NARIT, as the IAU Southeast Asia Regional
Office of Astronomy for Development, has
been invited as one of the member institutes
of the EAO. NARIT is now working in
collaboration with EAO under an the
Memorandum of Agreement between the 2
institutes (September 2017). The EAO
currently operates the James Clerk Maxwell
Telescope (JCMT), which is the largest
single dish telescope to operate at
submillimeter wavelengths. The 15-meter
telescope is located on the summit of Mauna
Kea in Hawaii. The EAO operates the JCMT
on behalf of the University of Hawaii since
1st March 2015.
Terahertz Astronomy
22
We are interested in using the Terahertz (THz)
observations of interstellar atoms, molecules,
and dust serve as powerful probes of the
conditions within the interstellar medium that
permeates newly formed distant galaxies in
the early universe which can be well detected
in terahertz frequencies.
The Study on Close Binary Systems
Evolutionary stages of close binary
systems can be study through different
classes:
• Detached binaries
• Semi-detached binaries
• Contact binaries
• Low mass ratio deep contact
binaries
• Binary mergers: Such binary
mergers are likely to be
responsible for many eruptive
events in the Galaxy (e.g., V838
Mon; Tylenda & Soker 2006)
• Luminous Red Novae (LRN)
Search for the progenitor of LRNs by AST3-1
 Yunnan Observatories and NARIT has
long been cooperated on the research of
eclipsing binary stars
 AST3-1 is the second-generation wide
field optical photometric telescope at
Dome A
 285 eclipsing binaries (including EW,
EB, and EA-types) were observed in the
Galactic Disk (e.g., Wang et al. 2017)
 Search for the progenitors of LRNe
(deep and low-mass ratio contact
systems).
It is discovered that AST7302 is a contact
binary with the lowest mass ratio 0.067
• i=15.38 mag.
• P=0.37218 days
• T1=5400 K
• i = 75.5
• f = 13.0 %
• q=0.067
They are the progenitor candidates of Luminous red
novae
The “Thai Robotic Network” in Chile and Australia
Participation of Thai Robotic Telescopes
on Antarctic Astronomy
Cerro Tololo
60-cm
Lijiang
70-cm
AAT
70-cm
Thai Atmospheric Science Research
The study of “Impact from
space” deals with investigating
how space weather affects the
upper atmosphere, as well as
how the upper atmosphere
affects the lower atmosphere
and vice versa.
Thai Space Consortium
To build Thai capability (human, facilities &
Infrastructure) for development of Thai research
Satellites
CONSORTIUM’s GOAL
NARIT’s
GOAL
To build NARIT capability (human, facilities &
Infrastructure) for design and construction of mission
payloads (instruments) which are in line with NARIT’s
instrumentation direction
Payload
Satellite
platform
Test
facilities
The Development of
Satellites' Payloads for
Earth/Space Observation
Test Facility for Earth and
Space Observation Satellite
Satellite
Development for
Space Research
Phase 1 (2018): Prep
& feasibility study
Phase 2 (2019):
Payload development
Phase 3 (2020):
Platform
development & test
Phase 4 (2021):
AIT & test
Phase 5 (2022):
Launch &
commissioning
Roles
Research Satellite
 upgrade research by utilizing Satellite
 unlock the unsolved research problems and support data mining inside
and outside of the country.
 research integration and sharing the resources among organization
 built confidence and awareness in using and developing satellite and
space technology in Thailand
Long term target
 develop small and medium size satellite (100-300kg) with cheap and quick to specify
research (Custom made satellite for research)
 open opportunity for competition, develop research capability to develop satellite for
new missions
 realize and sustain the growth of satellite and space technology
 support new immerging industries and business for expansion of economic and
society.
To solve problems addressed in
 20 years National Research and Innovation
Strategy plan
 2017-2026 Space Strategy plan
 5 years S&T Strategy plan (2018-2022)
Space Technology Development
Communications
Planetary exploration
Navigation
Meteorology
Earth
observation
 Atmospheric Science
 Climate Change
 Space Environment/Weather
 Methane Detection
Potential Mission:
Research

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Presentation se asia galaxy forum 2018 narit

  • 1. Progress on the Development of Astronomy, Polar Science and Space Science in Thailand 1 Boonrucksar Soonthornthum, NARIT 2 March 2018 SE Asia Galaxy Forum 2018
  • 2. National Astronomical Research Institute of Thailand Established since 1 January 2009 under the Ministry of Science and Technology 2
  • 3. NARIT’s Headquarter “Princess Sirindhorn AstroPark” @ 260 Moo 4, Donkaew, Mae Rim District, Chiang Mai (22 acres) Functions • Main Administration Office of NARIT • Advanced Research Laboratories: High Performance Computing, Optics, Radio Frequencies • Workshops: High Precision Machining, Mechatronics, Mirror Coating • Observatory and Planetarium for Public
  • 4. NARIT’s Key Sciences 1. Impact from Space: The first key science deals with investigating how space weather affects the upper atmosphere, as well as how the upper atmosphere affects the lower atmosphere and vice versa. It also aims to study the effect of man on earth’s climate. 2. Understanding Physics of the Universe: The key science comprises several fields in stellar physics, including the study of the extremes of the Universe (i.e. gamma ray burst, compact objects) and the study of stellar evolutionary process. A few highlighted research topics in this key science are: variable stars and binary systems, star formation, and stellar population study. 3. Exoplanets and Astrobiology: The key science focuses on the search for new exoplanets using various observational techniques, the study of the physical properties of exoplanets and the understanding of planetary formation, the exploration of the earth-like exoplanets with habitable zone and clues of lives outside the Solar system. 4. Understanding the Origin of the Cosmos: The key science focuses on the key questions of modern cosmology and physics: What causes the late-time accelerated expansion of the Universe? What is the Dark Matter? And how do the large-scale structures (e.g. galaxies, groups and clusters of galaxies) form and evolve?
  • 7. Thai National Observatory, 2.4-m Thai National Telescope, TNT
  • 8. Major Instruments • ULTRASPEC • 4k x 4k CCD Camera • Medium Resolution Spectrograph (MRES)
  • 9. Thai Remote Telescope Network (TRTN) Cerro Tololo Inter-American Observatory (CTIO) Republic of Chile Gao Mei Gu Observatory, Lijiang, P.R. of China Sierra Remote Observatory, California, U.S.A. Springbrook Observatory, Queensland, Australia GOTO Project at La Palma Canary Island, Spain
  • 10. High Performance Computer cluster Hardware (”Chalawan” Cluster)  1 Management node (12 cores, 2.4 GHz Intel Xeon E5-26xx v3)  19 compute nodes (rack + Blade servers) • CPU 496 cores (@ 2.6GHz clock speed) • Memory 2.2TB • Infiniband FDR 56Gbps interconnect • 2 Intel Xeon Phi Coprocessors (112 cores @ 1.2GHz)  Storage: Lustre 90TB over IB FDR  Rpeak= 22 TeraFLOPS
  • 11. National Network on Radio Astronomy and Geodesy
  • 12. NARIT’s 40-meter Radio Telescope - `Updated’ version of IGN’s 40m Yebes Radio Telescope - 40m Diameter with Parabolic Surface, Cassegrain-Nasmyth optics - total surface accuracy<200 um (rms) - Slew: 3 m/s in Azimuth , 1 m/s in Vertical - Pointing: 2” (no wind), 6” (5 m/s wind) - Prime-focus receiver mechanism
  • 13. Yebes, 23 March 2017 Thailand-China Collaboration on VLBI Geodesy under “One Belt’ One Road” policy of Chinese’s government NARIT’s 13m VGOS (VLBI Global Observing System) antenna for a very precise plate tectonic measurement 13m VGOS Zelenchukskaya (RU) 13m VGOS GGAO (US)
  • 14. NARIT-NAOC MoU April 5 2017 14 FAST Radio Telescope
  • 16. Astronomy at Polar Region Polar region (Arctic/Antarctic Plateau) is a perfect place for astronomical observations due to its - Long and continuous 6 months dark clear winter sky - Stable atmospheric condition with excellent sky seeing We can do the long-term, unbroken and continuous monitoring of various types of celestial objects eg: binary stars, variable stars, exoplanets, transient phenomena, exploding stars ect. Also the investigations of the aurora phenomena on earth.
  • 17.
  • 18. HRH Princess Maha Chakri Sirindhorn’s visits to China 18 MoU Signing with Polar Research Institute of China (PRIC) 6 April 2016
  • 19. NARIT’s Antarctic Research Topics (Under PRIC-NARIT Collaboration 1. Exo-planets/ Exo-earths Detection 2. Variable Stars, Transient Phenomena 3. Stellar Seismology: Vibrations of stars/Starquakes 4. Growth of Supermassive Black Holes and Co- evolution of Host Galaxies 5. Pipeline development for wide-field photometry 6. A cooperation on the construction of a 1-meter telescope for spectroscopy in Antarctic 7. Astronomical and upper atmosphere physical instruments operated at Chinese Stations
  • 20. Join Bright Stars Survey Telescope (BSST) Project at Zhongshan Station, Antarctica, 2016 (30 cm aperture, 3.4ºx 3.4º Field of View) TEST in April-May 2015)
  • 21. Collaboration with East Asian Observatory (EAO) 21 NARIT, as the IAU Southeast Asia Regional Office of Astronomy for Development, has been invited as one of the member institutes of the EAO. NARIT is now working in collaboration with EAO under an the Memorandum of Agreement between the 2 institutes (September 2017). The EAO currently operates the James Clerk Maxwell Telescope (JCMT), which is the largest single dish telescope to operate at submillimeter wavelengths. The 15-meter telescope is located on the summit of Mauna Kea in Hawaii. The EAO operates the JCMT on behalf of the University of Hawaii since 1st March 2015.
  • 22. Terahertz Astronomy 22 We are interested in using the Terahertz (THz) observations of interstellar atoms, molecules, and dust serve as powerful probes of the conditions within the interstellar medium that permeates newly formed distant galaxies in the early universe which can be well detected in terahertz frequencies.
  • 23. The Study on Close Binary Systems Evolutionary stages of close binary systems can be study through different classes: • Detached binaries • Semi-detached binaries • Contact binaries • Low mass ratio deep contact binaries • Binary mergers: Such binary mergers are likely to be responsible for many eruptive events in the Galaxy (e.g., V838 Mon; Tylenda & Soker 2006) • Luminous Red Novae (LRN)
  • 24. Search for the progenitor of LRNs by AST3-1  Yunnan Observatories and NARIT has long been cooperated on the research of eclipsing binary stars  AST3-1 is the second-generation wide field optical photometric telescope at Dome A  285 eclipsing binaries (including EW, EB, and EA-types) were observed in the Galactic Disk (e.g., Wang et al. 2017)  Search for the progenitors of LRNe (deep and low-mass ratio contact systems).
  • 25. It is discovered that AST7302 is a contact binary with the lowest mass ratio 0.067 • i=15.38 mag. • P=0.37218 days • T1=5400 K • i = 75.5 • f = 13.0 % • q=0.067 They are the progenitor candidates of Luminous red novae
  • 26. The “Thai Robotic Network” in Chile and Australia Participation of Thai Robotic Telescopes on Antarctic Astronomy Cerro Tololo 60-cm Lijiang 70-cm AAT 70-cm
  • 27. Thai Atmospheric Science Research The study of “Impact from space” deals with investigating how space weather affects the upper atmosphere, as well as how the upper atmosphere affects the lower atmosphere and vice versa.
  • 28. Thai Space Consortium To build Thai capability (human, facilities & Infrastructure) for development of Thai research Satellites CONSORTIUM’s GOAL NARIT’s GOAL To build NARIT capability (human, facilities & Infrastructure) for design and construction of mission payloads (instruments) which are in line with NARIT’s instrumentation direction
  • 29. Payload Satellite platform Test facilities The Development of Satellites' Payloads for Earth/Space Observation Test Facility for Earth and Space Observation Satellite Satellite Development for Space Research Phase 1 (2018): Prep & feasibility study Phase 2 (2019): Payload development Phase 3 (2020): Platform development & test Phase 4 (2021): AIT & test Phase 5 (2022): Launch & commissioning Roles
  • 30. Research Satellite  upgrade research by utilizing Satellite  unlock the unsolved research problems and support data mining inside and outside of the country.  research integration and sharing the resources among organization  built confidence and awareness in using and developing satellite and space technology in Thailand Long term target  develop small and medium size satellite (100-300kg) with cheap and quick to specify research (Custom made satellite for research)  open opportunity for competition, develop research capability to develop satellite for new missions  realize and sustain the growth of satellite and space technology  support new immerging industries and business for expansion of economic and society. To solve problems addressed in  20 years National Research and Innovation Strategy plan  2017-2026 Space Strategy plan  5 years S&T Strategy plan (2018-2022)
  • 31. Space Technology Development Communications Planetary exploration Navigation Meteorology Earth observation  Atmospheric Science  Climate Change  Space Environment/Weather  Methane Detection Potential Mission: Research