In 1960 the first such program, Project Ozma, led by American astronomer Frank Drake at the National Radio Astronomy Observatory in Green Bank, W.Va., focused on the nearby stars Epsilon Eridani and Tau Ceti. Since then some 50 searches, most of limited duration and concentrating on stars similar to the sun, have been conducted without success. In 1992 the High Resolution Microwave Survey (HRMS) was initiated. Using radio telescopes around the world in a planned ten-year search, HRMS envisioned a two-pronged approach. One group was to focus on solar-type stars within 100 light-years of Earth; the other was to conduct an all-sky survey. HRMS was halted by a funding cutback in 1993, but privately raised funds were used by the SETI Institute beginning in 1995 to conduct a search of nearby solar-type stars. Project Phoenix, as it is now called, monitors only microwave frequencies because there are few natural sources of emissions in that range and researchers hope that extraterrestrials would recognize that range as a quiet region of the electromagnetic spectrum suited to sending a message.
In addition to the listening efforts of the radio astronomers, other forms of contact have been attempted. Various coded messages have been broadcast in the hope that an extraterrestrial civilization might also have a SETI program. Gambling on a chance encounter with an extraterrestrial civilization, the U.S. space probes Pioneer 10 and 11 each carry an engraved plaque with a message from the earth, and Voyager 1 and 2 each have a recorded message of words and music. All four of these space probes have left the solar system and will travel in interstellar space indefinitely.
See also E. Ashpole, The Search for Extraterrestrial Intelligence (1990); D. Swift, SETI Pioneers: Scientists Talk about Their Search for Extraterrestrial Life (1990); F. Drake and D. Sobel, Is Anyone Out There? The Scientific Search for Extraterrestrial Intelligence (1992).
The Columbia Encyclopedia. Copyright © 2001-09 Columbia University Press. All rights reserved.
Seti I, d. 1290 B.C., king of ancient Egypt, of the XIX dynasty; son and successor of Ramses I. He succeeded to the throne c.1302 B.C. Invading Palestine and Syria, Seti I reduced them again t...
Abydos, ancient city of Egypt, c.50 mi (80 km) NW of Thebes, near modern El Balyana. Associated in religion with Osiris, Abydos became the most venerated place in Egypt. It was the favorite bu...
Pharaoh [Heb., from Egyptian,=the great house], title of the kings of ancient Egypt. Of the pharaohs in the Bible, Shishak is Sheshonk I, Neco or Necoh is Necho, and Hophra is Apries. Many sch...
Merneptah, d. c.1215 B.C., king of ancient Egypt, of the XIX dynasty; son and successor of Ramses II. He succeeded (1224 B.C.) to the throne when he was already advanced in years. He quelled a...
Belzoni, Giovanni Battista, 1778–1823, Italian adventurer and antiquities dealer. He lived (1803–12) in England and there invented a hydraulic machine, which he attempted to introduce into Egy...
Nubia, ancient state of NE Africa. At the height of its political power Nubia extended, from north to south, from the First Cataract of the Nile (near Aswan, Egypt) to Khartoum, in Sudan. It e...
Dynasties of Ancient EgyptOld Kingdom (or Old Empire)DynastyYearsFamous RulersI3110–2884 B.C.MenesII2884–2780 B.C.III2780–2680 B.C.SnefruIV2680–2565 B.C.Khufu (Cheops), Khafre, Menkaure. Age o...
Ramses, Rameses, or Ramesses, name of several kings of ancient Egypt of the XIX and XX dynasties. The kings of the XX dynasty, all named Ramses but the first, are often, on that account, calle...
Egyptian architecture, the architecture of the ancient Egyptians, formulated prior to 3000 B.C. and lasting through the Ptolemaic period (323–30 B.C.). Scant tree growth prevented the extensiv...
Mummy, dead human or animal body preserved by embalming or by unusual natural conditions. As a rule mummies are from ancient times. The word is of Arabic derivation and refers primarily to the...
|
|