SERENDIP
SERENDIP (Search for Extraterrestrial Radio Emissions from Nearby Developed Intelligent Populations) is a Search for Extra-Terrestrial Intelligence (SETI) program originated by the Berkeley SETI Research Center at the University of California, Berkeley.[1]
SERENDIP takes advantage of ongoing "mainstream" radio telescope observations as a "piggy-back" or "commensal" program. Rather than having its own observation program, SERENDIP analyzes deep space radio telescope data that it obtains while other astronomers are using the telescope.
Background
The initial SERENDIP instrument was a 100-channel analog radio spectrometer covering 100 kHz of bandwidth. Subsequent instruments have been significantly more capable, with the number of channels doubling roughly every year. These instruments have been deployed at a large number of telescopes including the NRAO 90m telescope at the Green Bank Observatory and the Arecibo 305m telescope.
SERENDIP observations have been conducted at frequencies between 400 MHz and 5 GHz, with most observations near the so-called Cosmic Water Hole (1.42 GHz (21 cm) neutral hydrogen and 1.66 GHz hydroxyl transitions).
Projects
SERENDIP V was installed at the Arecibo Observatory in June 2009. The digital back-end instrument was an FPGA-based 128 million-channel digital spectrometer covering 200 MHz of bandwidth. It took data commensally with the seven-beam Arecibo L-band Feed Array (ALFA).[2]
The next generation of SERENDIP experiments, SERENDIP VI was deployed in 2014 at both Arecibo and the Green Bank Telescope.[3] SERENDIP VI will also look for fast radio bursts, in collaboration with scientists from University of Oxford and West Virginia University.[4]
Findings
The program has found around 400 suspicious signals, but there is not enough data to prove that they belong to extraterrestrial intelligence.[5] In September–October 2004 the media wrote about Radio source SHGb02+14a and its artificial origin, but scrutiny has not been able to confirm its connection with an extraterrestrial civilization.[6] Currently no confirmed extraterrestrial signals have been found.[7]
See also
- Berkeley Open Infrastructure for Network Computing (BOINC)
- List of volunteer computing projects
- Radio source SHGb02+14a
- SETI
- SETI@home
- BLC1
- Wow! signal
References and notes
- ^ "SERENDIP". UC Berkeley. Archived from the original on 2013-03-11. Retrieved 2006-08-20.
- ^ "ALFA: Arecibo L-Band Feed Array". 26 November 2012. Archived from the original on 3 September 2009. Retrieved 24 August 2009.
- ^ Lebofsky, Matt (June 23, 2015). "SETI@Home Mid June Update". Retrieved 23 June 2015.
- ^ Cobb, Jeff (November 2013). "Winter 2013 SETI@home Letter". Archived from the original on 2013-11-18. Retrieved 15 November 2013.
- ^ Л.М.Гиндилис. Радиопоиск: век двадцатый
- ^ Г.М.Рудницкий. Что обнаружили в Аресибо?
- ^ Поиск внеземных цивилизаций
Content Disclaimer
Informasi ini disarikan dari Wikipedia dan disajikan kembali untuk tujuan edukasi. Konten tersedia di bawah lisensi CC BY-SA 3.0. Kami tidak bertanggung jawab atas ketidakakuratan data yang bersumber dari kontribusi publik tersebut.
- The information displayed on this website is sourced in part or in whole from Wikipedia and has been adapted for the purpose of restating it. We strive to provide accurate and relevant information, however:
- There is no guarantee of absolute accuracy. Wikipedia is an open, collaborative project that can be edited by anyone, so information is subject to change.
- It is not intended to constitute professional advice. The content displayed is for informational and educational purposes only. For important decisions (e.g., medical, legal, or financial), please consult a professional.
- Content copyright. Wikipedia is licensed under the Creative Commons Attribution-ShareAlike License (CC BY-SA). This means that content may be reused with appropriate attribution and shared under a similar license.
- Responsible use. Any risk arising from the use of information from this website is entirely the responsibility of the user.