TINJAUAN PROGRAM SETI (SEARCH FOR EXTRATERRESTRIAL INTELLIGENCE) DI OBSERVATORIUM BOSSCHA
“Are we alone?” has been a big question for scientists until now. Drake’s Equation gives an estimation about how many intelligent civilization capable to communicate that can be found in the Galaxy. In order to answer questions about their existence, a scientific program called SETI (Search for E...
Saved in:
Main Author: | |
---|---|
Format: | Final Project |
Language: | Indonesia |
Online Access: | https://digilib.itb.ac.id/gdl/view/45476 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Institution: | Institut Teknologi Bandung |
Language: | Indonesia |
id |
id-itb.:45476 |
---|---|
spelling |
id-itb.:454762019-12-26T11:41:10ZTINJAUAN PROGRAM SETI (SEARCH FOR EXTRATERRESTRIAL INTELLIGENCE) DI OBSERVATORIUM BOSSCHA Ramadhan, Sahlan Indonesia Final Project astrobiology, extraterrestrial intelligence, radio lines: general. INSTITUT TEKNOLOGI BANDUNG https://digilib.itb.ac.id/gdl/view/45476 “Are we alone?” has been a big question for scientists until now. Drake’s Equation gives an estimation about how many intelligent civilization capable to communicate that can be found in the Galaxy. In order to answer questions about their existence, a scientific program called SETI (Search for Extraterrestrial Intelligence) has been performing. The program is conducted by searching artificial electromagnetic signal from space in the radio spectrum. The spectrum is chosen based on observing window which is known as ‘Water Hole’ in the frequncy range of 1,42 – 1,68 GHz that has minimum noise. Many SETI programs were done with various instruments and methods since 1960 until now, but no ETI signal was detected. By examining the development on previous SETI programs, a study in SETI research in Bosscha Observatory was conducted. The study was done by observing radio signal in the frequency range of 1,4 – 1,7 GHz. There were two types of observation, RFI (Radio Frequency Interference) observation and Drift Scan observation. RFI observation was counducted by using omnidirecitional antenna to detect spurious signal from terrestrial sources,. Drift Scan observation was conducted by using Bosscha Hydrogen Radio Telescope with 5,72 meter in diameter pointed to zenith direction. Spectrum Analyzer GWSInstek-GSP380 was used as the receiver and Cricket 2.1 software utilized for data acquisition. Most of the observed signals were RFIs, and there were transient signals that appeared only in a short time. No SETI signals have been detected. In general, the system functions properly and the corresponding sensitivity must be increased to continue thus program. text |
institution |
Institut Teknologi Bandung |
building |
Institut Teknologi Bandung Library |
continent |
Asia |
country |
Indonesia Indonesia |
content_provider |
Institut Teknologi Bandung |
collection |
Digital ITB |
language |
Indonesia |
description |
“Are we alone?” has been a big question for scientists until now. Drake’s Equation
gives an estimation about how many intelligent civilization capable to communicate
that can be found in the Galaxy. In order to answer questions about their existence,
a scientific program called SETI (Search for Extraterrestrial Intelligence) has been
performing. The program is conducted by searching artificial electromagnetic
signal from space in the radio spectrum. The spectrum is chosen based on observing
window which is known as ‘Water Hole’ in the frequncy range of 1,42 – 1,68 GHz
that has minimum noise. Many SETI programs were done with various instruments
and methods since 1960 until now, but no ETI signal was detected.
By examining the development on previous SETI programs, a study in SETI
research in Bosscha Observatory was conducted. The study was done by observing
radio signal in the frequency range of 1,4 – 1,7 GHz. There were two types of
observation, RFI (Radio Frequency Interference) observation and Drift Scan
observation. RFI observation was counducted by using omnidirecitional antenna to
detect spurious signal from terrestrial sources,. Drift Scan observation was
conducted by using Bosscha Hydrogen Radio Telescope with 5,72 meter in
diameter pointed to zenith direction. Spectrum Analyzer GWSInstek-GSP380 was
used as the receiver and Cricket 2.1 software utilized for data acquisition. Most of
the observed signals were RFIs, and there were transient signals that appeared only
in a short time. No SETI signals have been detected. In general, the system
functions properly and the corresponding sensitivity must be increased to continue
thus program. |
format |
Final Project |
author |
Ramadhan, Sahlan |
spellingShingle |
Ramadhan, Sahlan TINJAUAN PROGRAM SETI (SEARCH FOR EXTRATERRESTRIAL INTELLIGENCE) DI OBSERVATORIUM BOSSCHA |
author_facet |
Ramadhan, Sahlan |
author_sort |
Ramadhan, Sahlan |
title |
TINJAUAN PROGRAM SETI (SEARCH FOR EXTRATERRESTRIAL INTELLIGENCE) DI OBSERVATORIUM BOSSCHA |
title_short |
TINJAUAN PROGRAM SETI (SEARCH FOR EXTRATERRESTRIAL INTELLIGENCE) DI OBSERVATORIUM BOSSCHA |
title_full |
TINJAUAN PROGRAM SETI (SEARCH FOR EXTRATERRESTRIAL INTELLIGENCE) DI OBSERVATORIUM BOSSCHA |
title_fullStr |
TINJAUAN PROGRAM SETI (SEARCH FOR EXTRATERRESTRIAL INTELLIGENCE) DI OBSERVATORIUM BOSSCHA |
title_full_unstemmed |
TINJAUAN PROGRAM SETI (SEARCH FOR EXTRATERRESTRIAL INTELLIGENCE) DI OBSERVATORIUM BOSSCHA |
title_sort |
tinjauan program seti (search for extraterrestrial intelligence) di observatorium bosscha |
url |
https://digilib.itb.ac.id/gdl/view/45476 |
_version_ |
1821999371965693952 |