Cosmic Call
Cosmic Call was a private initiative consisting of two sets of interstellar radio messages transmitted from the 70-meter RT-70 radio telescope at the Evpatoria Planetary Radar in Yevpatoria, Ukraine, in 1999 and 2003, aimed at nearby sun-like stars as part of active searches for extraterrestrial intelligence (METI).[1][2] The project was organized by Team Encounter, an American company led by Charles M. Chafer, with scientific contributions from Canadian physicists Yvan Dutil and Stéphane Dumas, who developed a binary primer to establish basic concepts in mathematics, chemistry, and linguistics for potential alien recipients.[3][4] Russian astronomer Alexander Zaitsev oversaw the transmissions at Evpatoria, utilizing the facility's 150 kW transmitter operating at 5.01 GHz with left circular polarization.[1][2] In the first transmission on May 24, 1999, and subsequent sessions from June 30 to July 1, 1999, messages totaling around 370,967 bits—including the Dutil-Dumas primer, the Arecibo message, binary images, and personal greetings—were sent at rates of 100 to 2,000 bits per second toward four target stars: HD 178428 (G5V, 68.3 light-years), HD 186408 (G2V, 70.5 light-years), HD 190360 (G6IV, 51.8 light-years), and HD 190406 (G1V, 57.6 light-years).[1][5] These targets were selected from the Catalog of Nearby Stars with potential for habitable exoplanets, with expected arrival times between 2051 and 2070.[3] The 2003 transmission, beginning on July 6, 2003, expanded the effort to five additional sun-like stars from the SETI Habitable Catalog: Hip 4872 (K5V, 32.8 light-years in Cassiopeia), Hip 7918 (G2V, 41.2 light-years in Andromeda), Hip 26335 (K7V, 37.1 light-years in Orion), Hip 43587 (G8V, 40.9 light-years in Cancer), and Hip 53721 (G0V, 45.9 light-years in Ursa Major).[2] This broadcast included an updated 500,472-bit scientific payload with the primer, bilingual glossaries, and the Arecibo message, transmitted at 400 bits per second over 53 minutes, followed by 220 MB of personal contributions—texts, images, audio, and video from thousands of participants—sent at 100 kbauds over 11 hours.[2][6] Arrival at these targets is anticipated between 2036 and 2049.[3] Funded through crowdfunding with costs estimated at $100,000, Cosmic Call represented one of the earliest major non-governmental METI efforts, involving about 20 collaborators and sparking debates on the risks and ethics of broadcasting to unknown civilizations.[3][7] The messages' content emphasized universality, drawing on prior interstellar signals like the 1974 Arecibo message, while the primer's design built on linguist Hans Freudenthal's Lincos system to progressively introduce concepts from basic numerals to human biology and technology.[4][6] No responses have been detected, and the project highlighted the challenges of interstellar communication, including signal detectability over vast distances.[3]Background
Project Origins
The Cosmic Call project originated in the late 1990s as a private initiative within the broader Messaging to Extra-Terrestrial Intelligence (METI) efforts, drawing inspiration from landmark interstellar communications such as the 1974 Arecibo message and the Voyager Golden Record launched in 1977.[3][5] Planning for the project began around 1998, when Canadian scientists Yvan Dutil, an astrophysicist who had recently completed his doctorate at Université Laval and was affiliated with the Defence Research and Development Canada - Valcartier, and Stéphane Dumas, a physicist with the Canadian government, developed a foundational primer for encoding human knowledge in a form suitable for potential extraterrestrial recipients.[6][5] Their work built on linguistic and informational principles to create a universal message language, marking a significant step in active SETI communication strategies.[3] The project was spearheaded by Team Encounter, a Texas-based startup founded by entrepreneur Charlie Chafer, which provided funding through a crowdsourcing model often described as a "people's space program."[3][2] With direct costs estimated at around $50,000 supplemented by small donations, Team Encounter coordinated the effort until it ceased operations in 2004.[3] Key collaborations included the Yevpatoria team at Ukraine's RT-70 radio telescope facility, led by Russian scientist Alexander Zaitsev, who oversaw logistical and operational aspects.[5][1] Additionally, the Institute of Radio Engineering and Electronics (IRE) of the Russian Academy of Sciences contributed expertise in radio engineering, facilitating the international assembly of scientists, engineers, and enthusiasts.[2] This organizational setup culminated in the first transmission on May 24, 1999, from the Evpatoria Planetary Radar in Crimea, Ukraine, establishing Cosmic Call as a pioneering example of privately funded METI endeavors.[6][1] The project's origins reflect a blend of scientific rigor and entrepreneurial vision, positioning it as a successor to government-led interstellar outreach while emphasizing accessible, collaborative innovation.[3][5]Objectives and Context
The Cosmic Call project aimed to transmit deliberate, encoded radio messages to nearby stars that might host extraterrestrial intelligence, serving as a proactive initiative in Messaging Extraterrestrial Intelligence (METI).[5] This effort sought to initiate potential interstellar dialogue by encoding universal scientific principles and human cultural elements into signals detectable by advanced civilizations within approximately 100 light-years.[2] Motivated by the limitations of passive SETI searches, which listen for incoming signals without transmission, Cosmic Call emphasized active outreach to break the "Great Silence" and represent humanity's diversity through multimedia contributions from global participants.[8] The project promoted international collaboration, involving scientists from Canada, the United States, and Russia, and was funded through public donations as a "people's space program" rather than government resources, highlighting grassroots enthusiasm for cosmic communication.[2][7] Positioned within the evolution of interstellar messaging, Cosmic Call built on 20th-century precedents such as the Pioneer plaques affixed to spacecraft in 1972 and 1973, which carried physical depictions of humans and the solar system, and the 1974 Arecibo message, a binary-encoded radio signal sent toward the Messier 13 globular cluster.[5] Unlike the one-way, omnidirectional Voyager Golden Records launched in 1977, Cosmic Call employed targeted, directional radio transmissions to specific stellar systems, enabling more focused and repeated attempts at contact.[7] Ethical debates surrounded the project, particularly concerns over the risks of revealing Earth's location to potentially hostile extraterrestrial entities, with some critics arguing that such transmissions could invite unforeseen dangers without global consensus.[7] Despite these unresolved questions, the initiators, including Canadian scientists Yvan Dutil and Stéphane Dumas, prioritized outreach and informed international bodies under the Outer Space Treaty, proceeding without formal prohibitions.[5][9]Message Composition
Core Components
The Cosmic Call messages consisted of a scientific payload designed to convey universal knowledge, followed by personal contributions. The core scientific elements were common to both transmissions but varied in structure and additions between 1999 and 2003. Central was the Dutil-Dumas Message (DDM), a primer developed by Canadian scientists Yvan Dutil and Stéphane Dumas, introducing mathematical concepts like counting, prime numbers, arithmetic operations, geometry (including π and the Pythagorean theorem), physical constants (e.g., masses of electron and proton, derived from hydrogen spectrum), units, chemistry (elements up to 112 in 1999, 114 in 2003), astronomy (Solar System, Earth-Moon), biology (human figure, DNA, cells), and cosmology, ending with questions for recipients.[5] This primer established a shared foundation using verifiable principles.[10] Other core components included the Braastad Message (BM), a mathematical depiction of human biology, reproduction, family, and social structures; the Arecibo Message (AM), the 1974 binary pictorial from the Arecibo Observatory encoding numbers, DNA, human figures, solar system, and Earth's location; and the Encounter 2001 Staff Message (ESM), textual greetings and messages from project participants.[1] In Cosmic Call 1 (1999), the DDM used 23 pages of 127×127 pixel grids. The total scientific payload was approximately 371,000 bits (about 46 KB), including the DDM, BM, AM, ESM, and minimal personal texts/names.[1] Cosmic Call 2 (2003) featured an updated Dutil-Dumas Message 2 (DDM2 or Interstellar Rosetta Stone, ISR), consolidated into a single page for efficiency, with symbols reduced to 4×7 bits for numerals. It added the Bilingual Image Glossary (BIG), pixel-based icons reinforcing concepts like numbers and elements. The scientific payload totaled 500,472 bits, including triple repetitions of DDM2, AM, and BIG, plus single BM and TE Staff Message (updated ESM).[2] Personal contributions expanded significantly in Cosmic Call 2 as the Public Part (PP), a 220 MB archive of submissions from over 43,000 people in 50 countries, including texts, static images (landscapes, portraits, flags, animals), audio (natural sounds like bird calls and ocean waves, cultural music excerpts such as the Beatles' "Across the Universe" and David Bowie's "Starman"), and video/animations depicting human activities and daily life.[2][11] Selection was by an international team from Team Encounter (USA), the Institute for Radio-engineering and Electronics (Russia), and Canadian contributors, balancing universality and inclusivity.[2]Encoding and Design
The Cosmic Call messages were structured as sequential binary segments, starting with the core scientific primer (DDM or DDM2) to build foundational concepts, followed by other informational components (BM, AM, ESM/TE Staff, BIG in 2003), and personal elements, all in a unified binary stream with pauses and synchronization headers for reconstruction.[1] This used frequency-shift keying with +24 kHz for "1", -24 kHz for "0", centered at 5.010 GHz.[1] The DDM employed 127×127 pixel grid pages—23 in 1999—to encode concepts via noise-resistant 5×7 bitmap symbols as an "Interstellar Rosetta Stone," relying on universal truths. Each page had a 1-pixel border, binary headers for numbering and orientation, enabling reassembly via Fourier analysis if degraded. The 2003 DDM2 compressed to 4×7 for numerals while keeping the grid, enhancing efficiency.[5][10] Multimedia in personal messages (especially CC2) was encoded as black-and-white bitmaps for images/animations, waveform samples for audio, with self-descriptive metadata for dimensions, scales, and parameters. These followed the primers in the stream.[2] Design principles included triple repetition of scientific segments for error correction, slow rates (100 bps for CC1 core, 400 bps for CC2 scientific) for detectability, and culture-independent representations of math/physics. Symbols resisted rotation, mirroring, and errors, prioritizing universality.[1][5]Transmission Events
Cosmic Call 1
Cosmic Call 1 represented the inaugural deliberate Messaging to Extra-Terrestrial Intelligence (METI) effort following the end of the Cold War, marking a renewed push to actively communicate with potential extraterrestrial civilizations after a period dominated by passive SETI searches. Organized under the Encounter 2001 project, this transmission incorporated public input through calls for content contributions, engaging participants worldwide in shaping the message's personal elements. The effort aimed to bridge the "Great Silence" by sending structured information about humanity to nearby stars, emphasizing mathematical foundations and cultural snapshots.[8] The transmissions occurred over four sessions from May 24 to July 1, 1999, at the Evpatoria Deep Space Center in Ukraine, totaling approximately 16 hours of broadcast time. The first session targeted HD 186408 on May 24 from 16:20 to 20:15 UT, lasting about 3 hours and 55 minutes; subsequent sessions followed on June 30 for HD 178428 (16:45 to 20:40 UT) and HD 190406 (spanning June 30–July 1, 21:10 to 01:05 UT), and on July 1 for HD 190360 (01:22 to 05:17 UT), each also around 3 hours and 55 minutes. This multi-session approach ensured redundancy and coverage of multiple targets within logistical constraints of the facility.[1] The message sequence consisted of two main parts, with the core content repeated for reliability. Part I, transmitted three times per target at 100 bits per second, included the Dutil Message (DDM), Braastad Message (BM), Arecibo Message (AM), and Encounter 2001 Staff Message (ESM); the DDM briefly outlined essential mathematical concepts such as numbers from 0 to 9, basic operators (+, -, *, /), and binary encoding to establish a universal lexicon. Part II, sent once per target at 2000 bits per second, comprised names and personal messages from project participants, adding a human touch to the interstellar broadcast. This structure prioritized clarity and error resilience in the encoded signal.[1][6] In the immediate aftermath, transmission logs confirmed successful delivery of the full message sequence to the four targeted stars without detected errors during the sessions, validating the system's performance for future METI initiatives. The project team noted opportunities for hardware improvements, such as enhancing klystron durability, but reported no disruptions impacting the 1999 broadcasts.[1]Cosmic Call 2
Cosmic Call 2, conducted on July 6, 2003, marked the second major interstellar transmission effort by the METI project, consolidating all messages into a single day of broadcasting from the Evpatoria Planetary Radar facility in Ukraine.[2] The event featured a structured sequence of components, beginning with three repetitions of the Digital Data Message 2 (DDM2), an improved version of the original Dutil-Dumas message that addressed encoding issues from Cosmic Call 1 by varying line numbers per page instead of the uniform 127x127 format used previously.[2] This was followed by three repetitions each of the Arecibo Message (AM) and Bilingual Image Glossary (BIG), then the Braastad Message (BM), Encounter 2001 Staff Message (ESM), and concluding with the Personal Messages (PP) segment.[2] Most scientific components transmitted at 400 bits per second, while the PP segment operated at a higher data rate of 100,000 bits per second to accommodate its expanded multimedia content.[2] The transmission lasted approximately 11 hours for the PP segment alone, which included a significantly larger dataset than the first Cosmic Call, featuring 220 MB of text, photographs, audio recordings, and video clips organized into 24 folders contributed by the public.[2] Overall scientific messages spanned about 53 minutes, building on lessons from the 1999 effort by incorporating more diverse and voluminous personal elements to better represent human culture.[2] Five Sun-like stars were targeted: HIP 4872, HIP 7918, HIP 26335, HIP 43587, and HIP 53721, selected for their proximity and potential habitability.[2] This event responded to increasing global interest in METI initiatives during the early 2000s, serving as an international collaboration that integrated prior messages into a unified broadcast.[2] Funded through public contributions as part of Team Encounter's "people's space program," it represented the project's final major transmission before the sponsoring startup ceased operations in 2004 due to funding challenges.[3]Technical Specifications
Equipment Used
The Cosmic Call transmissions utilized the RT-70 radio telescope, a 70-meter diameter dish located at the Center for Deep Space Communications in Yevpatoria, Ukraine.[12] This facility, originally constructed as part of the Soviet Union's planetary radar network during the Cold War era, was designed for both radio astronomy observations and high-power radar operations supporting space missions.[13] The RT-70's large parabolic antenna provided a substantial effective area of approximately 2,500 square meters, enabling focused beam transmission over interstellar distances.[2] Supporting the telescope was a high-power transmitter system capable of delivering up to 150 kW of output power, with a stable frequency standard for coherent signal generation.[2] This transmitter was integrated with digital signal processing units to handle the modulation of encoded messages onto the carrier wave.[2] The setup included control systems managed by local personnel and international collaborators, ensuring precise alignment and operation during broadcasts.[14] In operation, the RT-70 dish was mechanically repositioned to point sequentially toward designated celestial coordinates for each transmission segment, allowing efficient coverage of multiple destinations over the course of the events in 1999 and 2003.[3] The facility's radar capabilities also facilitated on-site verification of transmitted signal strength and beam characteristics through integrated receiving systems.[13] The RT-70's dual-purpose design for planetary radar and deep-space communication imposed certain operational constraints, such as shared scheduling with scientific radar experiments, which limited availability for dedicated METI activities.[5] Following the 2003 Cosmic Call event, geopolitical shifts, including the 2014 annexation of Crimea by Russia, rendered the site inaccessible for further international METI collaborations, and the facility was ultimately destroyed in late August 2025 amid ongoing conflict.[12]Signal Parameters
The Cosmic Call transmissions utilized a carrier frequency of 5.01 GHz within the C-band spectrum.[1][2] For Cosmic Call 1 in 1999, the precise carrier was 5010.024 MHz, while Cosmic Call 2 in 2003 maintained the same nominal frequency of 5.01 GHz.[1][2] This microwave allocation facilitated propagation through Earth's atmosphere with minimal absorption and reduced susceptibility to natural radio noise sources.[1] Modulation employed frequency shift keying (FSK) principles to encode binary data, with a deviation of ±24 kHz from the carrier.[1][2] In Cosmic Call 1, the scheme was ternary, distinguishing "0" (–24 kHz shift), "1" (+24 kHz shift), and "pause" (no shift) to represent message elements reliably against potential jamming.[1] Cosmic Call 2 simplified to binary FSK, assigning +24 kHz to "1" and –24 kHz to "0" for the scientific and personal message segments.[2] This approach ensured robust signal integrity over interstellar distances by leveraging the stability of frequency modulation in the klystron-based transmitter.[1] The resulting signals were narrowband, occupying approximately 50 kHz of bandwidth to enhance detectability amid cosmic background noise.[1][2] The transmitter output power was 148–152 kW in Cosmic Call 1 and up to 150 kW average in Cosmic Call 2, resulting in an effective isotropic radiated power (EIRP) of approximately 10^{12} W.[1][2][13] Bit rates varied to balance data volume and transmission efficiency: Cosmic Call 1 used 100 bits/s for the initial pictorial message (Part I, repeated three times per session) and 2000 bits/s for the compressed repeat (Part II).[1] Cosmic Call 2 employed 400 bits/s for scientific content and escalated to 100,000 bits/s (100 kbauds) for the high-volume personal messages.[2] Transmission durations were tailored to antenna pointing toward each target star, typically spanning 3–4 hours per session in Cosmic Call 1 and 53 minutes for scientific portions plus about 11 hours total for personal data in Cosmic Call 2, using left-circular polarization throughout.[1][2]Targeted Stars
Selection Criteria
The selection of target stars for the Cosmic Call project was methodically designed to prioritize proximity and potential habitability, ensuring the signals could reach viable candidates within a practical timeframe while aligning with early understandings of exoplanetary systems. Primary criteria focused on stars within 100 light-years, a distance that allows the radio signals—traveling at the speed of light—to arrive within a century, thereby enabling conceivable future interactions, and supports a detectable signal-to-noise ratio at the transmission rate of 100 bits per second using modest receiving antennas.[5] A core emphasis was placed on Sun-like stars of G and K spectral types (such as G2V, G5V, and K7V), which exhibit stability and are more likely to host planetary systems suitable for life, including those with detected planets or otherwise stable configurations. This choice was grounded in scientific data from 1990s exoplanet discoveries, particularly via the radial velocity method, which revealed Jupiter-mass planets around solar analogs and informed assessments of habitability potential.[5] Known hostile environments, such as those near highly variable or metal-poor stars, were deliberately avoided to focus on systems with favorable conditions for long-term planetary stability.[5] The selection process was led by project astronomers Yvan Dutil and Stéphane Dumas, who drew from authoritative catalogs including the Gliese Catalogue of Nearby Stars for proximity data and the Hipparcos catalogue for precise astrometry and spectral classifications of solar-type stars within the target volume. Targets were filtered for Earth observability, requiring declination greater than 15° to ensure accessibility from the Northern Hemisphere transmission site, and positioned in sky regions with balanced coverage, such as near the galactic plane (galactic longitude l < 90°, latitude |b| < 15°) where sun-like star density is elevated based on prior SETI surveys like META.[5][1] Further constraints minimized interstellar scintillation by favoring galactic longitudes l ≥ 50°, optimizing signal clarity.[5] Final refinements incorporated metallicity and stellar age to evaluate planet-formation likelihood and system longevity, with expert consultation from astronomers like Kevin Apps of the University of Sussex. This rigorous approach, rooted in the SETI Institute's target lists, aimed to maximize detection probabilities by advanced extraterrestrial civilizations while symbolically extending humanity's message to the nearest cosmic neighbors, yielding four targets in Cosmic Call 1 and five in Cosmic Call 2.[5][1]Target List and Timelines
The Cosmic Call project directed its interstellar messages toward a select group of nearby Sun-like stars, chosen for their potential to host habitable exoplanets, with transmissions aligned to point the 70-meter antenna at Evpatoria toward each target during dedicated sessions.[1][2] The signals propagate at the speed of light, so estimated arrival dates are calculated by adding the star's distance in light-years to the transmission year, accounting for the specific transmission date where applicable.[10] For Cosmic Call 1 in 1999, four stars were targeted over three transmission sessions in May and June–July.[1]| Star Name | Constellation | Distance (ly) | Transmission Date | Estimated Arrival |
|---|---|---|---|---|
| 16 Cyg A (HD 186408) | Cygnus | 70.5 | May 24, 1999 | November 2069 |
| 15 Sge (HD 190406) | Sagitta | 57.6 | June 30, 1999 | February 2057 |
| HD 178428 | Sagitta | 68.3 | June 30, 1999 | October 2067 |
| Gl 777 (HD 190360) | Cygnus | 51.8 | July 1, 1999 | April 2051 |
| Star Name | Constellation | Distance (ly) | Transmission Date | Estimated Arrival |
|---|---|---|---|---|
| GJ 49 (Hip 4872) | Cassiopeia | 32.8 | July 6, 2003 | April 2036 |
| GJ 208 (Hip 26335) | Orion | 37.1 | July 6, 2003 | August 2040 |
| 55 Cnc (Hip 43587) | Cancer | 40.3 | July 6, 2003 | May 2044 |
| HD 10307 (Hip 7918) | Andromeda | 41.5 | July 6, 2003 | September 2044 |
| 47 UMa (Hip 53721) | Ursa Major | 45.9 | July 6, 2003 | May 2049 |