中文
相关论文

相关论文: Lunar Opportunities for SETI

200 篇论文

Detecting primordial fluctuations from the cosmic dark ages requires extremely large low-frequency radio telescope arrays deployed on the far side of the Moon. The antenna of such an array must be lightweight, easily storable and…

Chang'E-4 (CE4), the first mission to soft-land on the lunar farside, provides a unique opportunity for astronomical observations from an environment shielded from terrestrial radio interference, and thus serves as pathfinder for lunar…

天体物理仪器与方法 · 物理学 2026-05-11 Jian-Kang Li , Zhen-Zhao Tao , Bo-Lun Huang , Kang-Jiao , Tong-Jie Zhang , Ming-Yuan Wang , Jin-Song Ping , Dan Werthimer , Vishal Gajjar

The discovery of ubiquitous habitable extrasolar planets, combined with revolutionary advances in instrumentation and observational capabilities, has ushered in a renaissance in the search for extra-terrestrial intelligence (SETI). Large…

A major aspect of the search for extraterrestrial intelligence (SETI) involves searching for electromagnetic transmissions from extraterrestrial sources, often using our own transmissions as a guide. Previous studies have suggested that…

天体物理仪器与方法 · 物理学 2025-08-22 Pinchen Fan , Jason T. Wright , T. Joseph W. Lazio

Observations at radio wavelengths address key problems in astrophysics, astrobiology, and lunar structure including the first light in the Universe (the Epoch of Reionization), the presence of magnetic fields around extrasolar planets,…

天体物理学 · 物理学 2007-05-23 J. Lazio , R. J. Macdowall , J. Burns , L. Demaio , D. L. Jones , K. W. Weiler

The far side of the Moon, shielded from terrestrial radio frequency interference and beyond the influence of Earth's ionosphere, should offer a uniquely quiet environment for radio astronomy and cosmological experiments. The radio sky below…

天体物理仪器与方法 · 物理学 2026-02-26 Kaja M. Rotermund , Aritoki Suzuki , Stuart D. Bale , Anže Slosar

The search for habitable conditions beyond Earth is a top priority in astrophysics. The discovery of habitable exoplanets beyond our solar system will require a suite of instruments providing long-term monitoring for detection (e.g. with…

We discuss low frequency radio astronomy from the moon, predominantly in the context of studying the neutral intergalactic medium during cosmic reionization using the HI 21cm line of neutral hydrogen. The epoch of reionization is the next…

天体物理学 · 物理学 2007-05-23 C. L. Carilli , J. N. Hewitt , A. Loeb

Radio astronomy provides a unique window on the universe, allowing us to study: non-thermal processes (galactic nuclei, quasars, pulsars) at the highest angular resolution using VLBI, with low opacity. It is the most interesting wave band…

天体物理学 · 物理学 2007-05-23 R D Ekers , J F Bell

Long baseline radio interferometers can provide some interesting opportunities for future SETI searches. Known advantages (compared to single dishes or beam-formed arrays), include the large reduction in false-positives due to the…

天体物理仪器与方法 · 物理学 2018-10-18 M. A. Garrett

The lunar geological record has much to tell us about the earliest history of the Solar System, the origin and evolution of the Earth-Moon system, the geological evolution of rocky planets, and the near-Earth cosmic environment throughout…

地球与行星天体物理 · 物理学 2015-06-05 I. A. Crawford , M. Anand , C. S. Cockell , H. Falcke , D. A. Green , R. Jaumann , M. A. Wieczorek

Radio telescopes observe extremely faint emission from astronomical objects, ranging from compact sources to large scale structures that can be seen across the whole sky. Satellites actively transmit at radio frequencies (particularly at…

天体物理仪器与方法 · 物理学 2025-04-17 M. Peel , S. Eggl , M. L. Rawls , H. Qiu , D. L. Clements

The Moon is our future. It may seem like a chimera with a projected cost in excess of 100 billion\$, and counting, dispensed on ARTEMIS with little to show to date. However it is the ideal site for the largest telescopes that we can dream…

宇宙学与河外天体物理 · 物理学 2025-09-11 Joseph Silk

We look at what astronomy from the Moon might be like in the visible over the next few decades. The Moon offers the possibility of installing large telescopes or interferometers with instruments larger than those on orbiting telescopes. We…

天体物理仪器与方法 · 物理学 2024-03-26 Jean Schneider , Pierre Kervella , Antoine Labeyrie

The Search for Extraterrestrial Intelligence (SETI) attempts to address the possibility of the presence of technological civilizations beyond the Earth. Benefiting from high sensitivity, large sky coverage, an innovative feed cabin for…

Due to ionosphere absorption and the interference by natural and artificial radio emissions, astronomical observation from the ground becomes very difficult at the wavelengths of decametre or longer, which we shall refer as the ultralong…

天体物理仪器与方法 · 物理学 2020-11-26 Xuelei Chen , Jingye Yan , Li Deng , Fengquan Wu , Lin Wu , Yidong Xu , Li Zhou

Radio astronomy observational facilities are under constant upgradation and development to achieve better capabilities including increasing the time and frequency resolutions of the recorded data, and increasing the receiving and recording…

天体物理仪器与方法 · 物理学 2017-11-07 Tao An , Xiao Chen , P. Mohan , Bao-Qiang Lao

Radio Searches for Extra Terrestrial Intelligence aim at detecting artificial transmissions from extra terrestrial communicative civilizations. The lack of prior knowledge concerning these potential transmissions increase the search…

信号处理 · 电气工程与系统科学 2018-09-19 Gregory Hellbourg

We advocate international consultations on societal and technical issues to address the risk problem, and a moratorium on future METI transmissions until such issues are resolved. Instead, we recommend continuing to conduct SETI by…

天体物理仪器与方法 · 物理学 2011-04-26 John Billingham , James Benford

Many science missions require an unobstructed view of space and a stable thermal environment but lack the technical or programmatic resources to reach orbits that satisfy these needs. This paper presents a high Earth orbit in 2:1 resonance…

地球与行星天体物理 · 物理学 2013-08-09 Joseph W. Gangestad , Gregory A. Henning , Randy R. Persinger , George R. Ricker