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Astronomy in Indonesia
Prof. Wahyu Srigutomo, Ph.D.
Dean of Faculty of Mathematics and Natural Sciences
Institut Teknologi Bandung (ITB), Bandung - Indonesia
Astronomy Related Institutions in Indonesia
 Department of Astronomy, ITB
 Bosscha Observatory, ITB
 Planetariums and Space parks (Jakarta, Yogyakarta,
Tenggarong)
 BRIN (National Research and Inovation Agency),
with three observing stations, the biggest facility is
3.8 m reflector telescope at Mount Timau (under
construction).
 Department of Atmospheric and Planetary Sciences,
ITERA (Sumatera Institute of Technology)
 BMKG (Meteorology, Climatology and Geophysics
Agency)
Astronomy Education and Research in ITB
 Programs : Bachelor, Masters & Doctorate
 Established in 1959
 Field of Research :
o Cosmology,
o Galaxies,
o Stars,
o Solar System .
 Connected to
o Bosscha Observatory (1923):
o Telescopes : 60 cm refractor,
o 71 cm reflector, radio telescope
Zeiss 60 cm
Refractor
Hydrogen 6 m
Radio Telescope
Astronomy Education and Research in ITB
Institute of Technology Sumatera (ITERA)
Department of Atmospheric and Planetary Sciences
ITERA
ITB Bosscha
Astronomy Education and Research in ITB
International Moon Sighting Station (IMSS) at ITERA campus
 3.8 m optical and infrared reflector telescope at Mount
Timau,Timor island, Kupang regency, East Nusa Tenggara
 Radio Telescope at Jatiluhur
 VGOS Station in ITB
 Public observatory for Astrotourism in Sabu Island
 Spacecraft launching Facility in Biak island, Papua or Morotai
in Maluku
Astronomy Education and Research in ITB
Future Facilities
 Will be the biggest optical telecope
in South East Asia and in near
Equator
 Altitude : 1300 m ASL
 Coordinates : 09o35’ South and 123o
56’ East
 Working wavelength : optical and
infrared
 Planned First Light : 2023
 Similar to Seimei telescope in
Okayama Observatory, Japan
Astronomy Education and Research in ITB
3.8 m Reflector at Timau Mountain
Timau National Observatory Mount Timau, Kupang Regency, Timor Island
MASTER PLAN: Programs on optical, radio, and … near infrared
3.8m Optical Telescope
0.5m optical survey telescopes
20m-class radio telescope
Low Frequency Dipole Field Array
Construction under LAPAN (National Space and Aeronautics Institute)  BRIN
Mount Timau Observatory under construction
 Will be the biggest optical telecope
in South East Asia and in near
Equator
 Altitude : 1300 m ASL
 Coordinates : 09o35’ South and 123o
56’ East
 Working wavelength : optical and
infrared
 Planned First Light : 2023
 Similar to Seimei telescope in
Okayama Observatory, Japan
Astronomy Education and Research in ITB
3.8 m Reflector at Timau Mountain
It is important to build our own
radio telescopes:
 Capacity Building
 Doing Science
o Astronomy
o Astrophysics
o Geodesy
o Atmospheric
o Geodynamics
Astronomy Education and Research in ITB
Motivation with radio astronomy; interdisciplinary fields
 Skill enhancement/ Technology /
Experiences, and so on
o Construct Radio Telescope
o Design/Produce receivers
o RFI Technology
o Cryogenics
o Time & Freq. stability
o ADC processing
 Global cooperation (Not only with Asia,
but also with Europe, Australia, North
America, Africa, and Latin America) to
make VLBI network
VLBI (Very Long Baseline Interferometry)
is a network of many radio telescope all
over the world to create a comparable
resolution with Earth size radio telescope.
Most spectacular result of VLBI is the
historical first picture of Black Hole
Astronomy Education and Research in ITB
Motivation with radio astronomy; interdisciplinary fields
 Considering conversion of
telecommunication antenna
 Multidisciplinary research with
astronomy (with FITB, STEI and FTMD)
 Radio Instrumentation
 Accurate time keeping
 Geodynamics, EOP
 Astrometry/astronomy (imaging)
 Software engineering
 etc
Astronomy Education and Research in ITB
Development of VLBI Radio Telescope with Indosat Ooredoo, Jatiluhur
There are many radio
telescopes in East Asia
mostly in nothern
hemisphere and some in
Australia and New
Zealand
There are no VLBI
telescope near the
Equator
In cooperation with Shanghai Astronomical Observatory
(Chinese Academy of Sciences), ITB will join the IVS
(International VLBI Service for Astrometry and Geodesy)
15
https://ivscc.gsfc.nasa.gov/about/vlbi/whatis.html
Organizations and Countries
Consejo Nacional de Investigaciones Cientificas y Scinicas Argentina
Geoscience Australia Australia
University of Tasmania Australia
CSIRO Australia
Vienna University of Technology Austria
Centro de Radio Astronomia e Aplicacoes Espaciais Brazil
Dominion Radio Astrophysical Observatory Canada
Chinese Academy of Sciences China
Observatoire de Paris France
Observatoire de Bordeaux France
Deutsches Geodeisches Forschungsinstitut, TU Munchen Germany
Bundesamt fur Kartographie und Geodesie Germany
Forschungseinrichtung Satellitengeodesie TU Munchen Germany
GeoForschungsZentrum Potsdam Germany
Max-Planck-Institut fűr Radioastronomie Germany
Istituto di Radioastronomia INAF Italy
Agenzia Spaziale Italiana Italy
Politecnico di Milano DICA Italy
Geospatial Information Authority of Japan Japan
National Institute of Information and Communications Technology Japan
National Astronomical Observatory of Japan Japan
National Institute of Polar Research Japan
Auckland University of Technology New Zealand
Norwegian Mapping Authority Norway
Astronomical Institute of St.-Petersburg University Russia
Central (Pulkovo) Astronomical Observatory Russia
Institute of Applied Astronomy Russia
Sternberg Astronomical Institute Russia
Hartebeesthoek Radio Astronomy Observatory South Africa
Korea Astronomy and Space Science Institute South Korea
National Geographic Information Institute South Korea
Instituto Geografico Nacional Spain
Chalmers University of Technology Sweden
Eidgenossische Technische Hochschule Zurich Switzerland
Karadeniz Technical University Turkey
Main Astronomical Observatory, National Academy of Sciences Kiev Ukraine
Laboratory of Radioastronomy of Crimean Astrophysical Observatory Ukraine
NASA Goddard Space Flight Center USA
U. S. Naval Observatory USA
Jet Propulsion Laboratory USA
16
https://www.mt-mechatronics.com/vlbi-2010.html
https://earth.gsfc.nasa.gov/geo/instruments/vlbi-global-observing-system-vgos
 New generation VLBI infrastructure
o Dense sampling of atmosphere
o Fast slewing telescopes
• Small diameter: 12 – 13 m
• Slew rate: 12 deg/sec
o Up to 2 observations per minute (2880/day)
 Broad bandwidth
o 2-14 (or 3-18)GHz
Wettzell, Germany Yebes, Spain
Hawaii, USA
Astronomy Education and Research in ITB
We will construct one of VLBI Global Observing System (VGOS)
Stations in ITB
Astronomy Education and Research in ITB
We will construct one of VLBI Global Observing System (VGOS)
Stations in ITB
The Space Very Long Baseline
Interferometry is a network of
space- and Earth-based radio
antennas that combine to create
the equivalent of a telescope with a
diameter more than two-and-a-half
times the diameter of Earth.
https://ggos.org/item/vlbi/
Sabu
Island
Sabu Island has more
clear nights than any
other places in Indonesia
Astronomy Education and Research in ITB
Another potential place for observatory and astrotourism : Sabu island
Biak Island
Astronomy Education and Research in ITB
Planned Satellite Launching Facility : Biak island
THANK YOU
TERIMA KASIH

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AAO2_ITB SlidesAstronomy In Indonesia.pptx

  • 1. Astronomy in Indonesia Prof. Wahyu Srigutomo, Ph.D. Dean of Faculty of Mathematics and Natural Sciences Institut Teknologi Bandung (ITB), Bandung - Indonesia
  • 2. Astronomy Related Institutions in Indonesia  Department of Astronomy, ITB  Bosscha Observatory, ITB  Planetariums and Space parks (Jakarta, Yogyakarta, Tenggarong)  BRIN (National Research and Inovation Agency), with three observing stations, the biggest facility is 3.8 m reflector telescope at Mount Timau (under construction).  Department of Atmospheric and Planetary Sciences, ITERA (Sumatera Institute of Technology)  BMKG (Meteorology, Climatology and Geophysics Agency)
  • 3. Astronomy Education and Research in ITB  Programs : Bachelor, Masters & Doctorate  Established in 1959  Field of Research : o Cosmology, o Galaxies, o Stars, o Solar System .  Connected to o Bosscha Observatory (1923): o Telescopes : 60 cm refractor, o 71 cm reflector, radio telescope Zeiss 60 cm Refractor Hydrogen 6 m Radio Telescope Astronomy Education and Research in ITB
  • 4. Institute of Technology Sumatera (ITERA) Department of Atmospheric and Planetary Sciences ITERA ITB Bosscha
  • 5. Astronomy Education and Research in ITB International Moon Sighting Station (IMSS) at ITERA campus
  • 6.  3.8 m optical and infrared reflector telescope at Mount Timau,Timor island, Kupang regency, East Nusa Tenggara  Radio Telescope at Jatiluhur  VGOS Station in ITB  Public observatory for Astrotourism in Sabu Island  Spacecraft launching Facility in Biak island, Papua or Morotai in Maluku Astronomy Education and Research in ITB Future Facilities
  • 7.  Will be the biggest optical telecope in South East Asia and in near Equator  Altitude : 1300 m ASL  Coordinates : 09o35’ South and 123o 56’ East  Working wavelength : optical and infrared  Planned First Light : 2023  Similar to Seimei telescope in Okayama Observatory, Japan Astronomy Education and Research in ITB 3.8 m Reflector at Timau Mountain
  • 8. Timau National Observatory Mount Timau, Kupang Regency, Timor Island MASTER PLAN: Programs on optical, radio, and … near infrared 3.8m Optical Telescope 0.5m optical survey telescopes 20m-class radio telescope Low Frequency Dipole Field Array Construction under LAPAN (National Space and Aeronautics Institute)  BRIN
  • 9. Mount Timau Observatory under construction
  • 10.  Will be the biggest optical telecope in South East Asia and in near Equator  Altitude : 1300 m ASL  Coordinates : 09o35’ South and 123o 56’ East  Working wavelength : optical and infrared  Planned First Light : 2023  Similar to Seimei telescope in Okayama Observatory, Japan Astronomy Education and Research in ITB 3.8 m Reflector at Timau Mountain
  • 11. It is important to build our own radio telescopes:  Capacity Building  Doing Science o Astronomy o Astrophysics o Geodesy o Atmospheric o Geodynamics Astronomy Education and Research in ITB Motivation with radio astronomy; interdisciplinary fields  Skill enhancement/ Technology / Experiences, and so on o Construct Radio Telescope o Design/Produce receivers o RFI Technology o Cryogenics o Time & Freq. stability o ADC processing
  • 12.  Global cooperation (Not only with Asia, but also with Europe, Australia, North America, Africa, and Latin America) to make VLBI network VLBI (Very Long Baseline Interferometry) is a network of many radio telescope all over the world to create a comparable resolution with Earth size radio telescope. Most spectacular result of VLBI is the historical first picture of Black Hole Astronomy Education and Research in ITB Motivation with radio astronomy; interdisciplinary fields
  • 13.  Considering conversion of telecommunication antenna  Multidisciplinary research with astronomy (with FITB, STEI and FTMD)  Radio Instrumentation  Accurate time keeping  Geodynamics, EOP  Astrometry/astronomy (imaging)  Software engineering  etc Astronomy Education and Research in ITB Development of VLBI Radio Telescope with Indosat Ooredoo, Jatiluhur
  • 14. There are many radio telescopes in East Asia mostly in nothern hemisphere and some in Australia and New Zealand There are no VLBI telescope near the Equator
  • 15. In cooperation with Shanghai Astronomical Observatory (Chinese Academy of Sciences), ITB will join the IVS (International VLBI Service for Astrometry and Geodesy) 15 https://ivscc.gsfc.nasa.gov/about/vlbi/whatis.html Organizations and Countries Consejo Nacional de Investigaciones Cientificas y Scinicas Argentina Geoscience Australia Australia University of Tasmania Australia CSIRO Australia Vienna University of Technology Austria Centro de Radio Astronomia e Aplicacoes Espaciais Brazil Dominion Radio Astrophysical Observatory Canada Chinese Academy of Sciences China Observatoire de Paris France Observatoire de Bordeaux France Deutsches Geodeisches Forschungsinstitut, TU Munchen Germany Bundesamt fur Kartographie und Geodesie Germany Forschungseinrichtung Satellitengeodesie TU Munchen Germany GeoForschungsZentrum Potsdam Germany Max-Planck-Institut fűr Radioastronomie Germany Istituto di Radioastronomia INAF Italy Agenzia Spaziale Italiana Italy Politecnico di Milano DICA Italy Geospatial Information Authority of Japan Japan National Institute of Information and Communications Technology Japan National Astronomical Observatory of Japan Japan National Institute of Polar Research Japan Auckland University of Technology New Zealand Norwegian Mapping Authority Norway Astronomical Institute of St.-Petersburg University Russia Central (Pulkovo) Astronomical Observatory Russia Institute of Applied Astronomy Russia Sternberg Astronomical Institute Russia Hartebeesthoek Radio Astronomy Observatory South Africa Korea Astronomy and Space Science Institute South Korea National Geographic Information Institute South Korea Instituto Geografico Nacional Spain Chalmers University of Technology Sweden Eidgenossische Technische Hochschule Zurich Switzerland Karadeniz Technical University Turkey Main Astronomical Observatory, National Academy of Sciences Kiev Ukraine Laboratory of Radioastronomy of Crimean Astrophysical Observatory Ukraine NASA Goddard Space Flight Center USA U. S. Naval Observatory USA Jet Propulsion Laboratory USA
  • 16. 16 https://www.mt-mechatronics.com/vlbi-2010.html https://earth.gsfc.nasa.gov/geo/instruments/vlbi-global-observing-system-vgos  New generation VLBI infrastructure o Dense sampling of atmosphere o Fast slewing telescopes • Small diameter: 12 – 13 m • Slew rate: 12 deg/sec o Up to 2 observations per minute (2880/day)  Broad bandwidth o 2-14 (or 3-18)GHz Wettzell, Germany Yebes, Spain Hawaii, USA Astronomy Education and Research in ITB We will construct one of VLBI Global Observing System (VGOS) Stations in ITB
  • 17. Astronomy Education and Research in ITB We will construct one of VLBI Global Observing System (VGOS) Stations in ITB The Space Very Long Baseline Interferometry is a network of space- and Earth-based radio antennas that combine to create the equivalent of a telescope with a diameter more than two-and-a-half times the diameter of Earth. https://ggos.org/item/vlbi/
  • 18. Sabu Island Sabu Island has more clear nights than any other places in Indonesia Astronomy Education and Research in ITB Another potential place for observatory and astrotourism : Sabu island
  • 19. Biak Island Astronomy Education and Research in ITB Planned Satellite Launching Facility : Biak island

Editor's Notes

  1. In Timau, there will be other telescopes, not only 3.8 m optical telescope. There will be smaller telescopes and radio telescopes
  2. This is the building for housing the 3.8 m telescope, contruction is planned to finish in the end of this year. Observation for research is expected to be start in the mid of 2023.
  3. In Timau, there will be other telescopes, not only 3.8 m optical telescope. There will be smaller telescopes and radio telescopes
  4. A radio telescope in Indonesia, capable to become one node of VLBI will fill a gap of VLBI
  5. A radio telescope in Indonesia, capable to become one node of VLBI will fill a gap of VLBI
  6. There are many radio telescopes in East Asia, mostly in nothern hemisphere and some in Australia and New Zealand. There are no VLBI telescope near the Equator. It is a big gap.
  7. There is only one VLBI radio telescope in the world, that is in Brazil, while so many in Northern Hemisphere. A VLBI telescope in Indonesia will provide great contribution in filling the gap.
  8. A VLBI radio telescope is planned to be installed near the Bosscha Observatory, in cooperation with China
  9. A VLBI radio telescope is planned to be installed near the Bosscha Observatory, in cooperation with China
  10. Sabu island is one of the places in Indonesia which has greatest fraction of clear sky (Hidayat et al, 2012), very good for constructing an observing station for research and astrotourism
  11. Biak island in Papua province very close to the equator and face an ocean in the East. Launching geo stationary and equatorial telescope from equator will be cheaper, because of higher initial velocity and simpler maneuver, when compared to higher latitude