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
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
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
In Timau, there will be other telescopes, not only 3.8 m optical telescope. There will be smaller telescopes and radio telescopes
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.
In Timau, there will be other telescopes, not only 3.8 m optical telescope. There will be smaller telescopes and radio telescopes
A radio telescope in Indonesia, capable to become one node of VLBI will fill a gap of VLBI
A radio telescope in Indonesia, capable to become one node of VLBI will fill a gap of VLBI
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.
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.
A VLBI radio telescope is planned to be installed near the Bosscha Observatory, in cooperation with China
A VLBI radio telescope is planned to be installed near the Bosscha Observatory, in cooperation with China
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
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