How long would the "message" need to be to transmit the entire Human Genome into deep space using the Hydrogen Line frequency?
See:
How big is the human genome?The size of genomes differs from one organism to the next. It seems likely that a human would have much more DNA than a fly, because humans are so much larger and more complex. However, the complexity of each genome is not necessarily related to its size.
The Human Genome Project is involved in determining the exact order of the DNA bases of the entire human genome. The human genome contains more than 3.4 billion base pairs and between 20 000 and 25 000 genes.
The U.S. Department of Energy Human Genome Project Information Web site illustrates the size of the human genome by estimating that it would take "about 9.5 years to read out loud (without stopping) the more than three billion pairs of bases in one person's genome sequence". {Source: Human Genome Projects Information}.
Another example of the immensity of the human genome is given by the Centre for Integrated Genomics:
"If our strands of DNA were stretched out in a line, the 46 chromosomes making up the human genome would extend more than six feet {close to two metres}. If the ... length of the 100 trillion cells could be stretched out, it would be ... over 113 billion miles <182 billion kilometres>. That is enough material to reach to the sun and back 610 times." {Source: Centre for Integrated Genomics}
More:
http://nature.ca/genome/03/a/03a_11a_e.cfmWhat is the Hydrogen Line?Dear Dr. SETI:
What is the hydrogen line, and why are radio or RF transmissions prohibited at this frequency? Thanks for any info.
The hydrogen line (1420.40575 MHz) is the precession frequency of neutral hydrogen atoms, the most abundant substance in space. It happens to fall in the quietest part of the radio spectrum, what's known as the Microwave Window. Although there may not seem to be a lot of loose hydrogen atoms about (there's perhaps one per cubic centimeter of interstellar space), the interstellar medium contains a lot of cubic centimeters. So these individual atoms chirping away at 1420 MHz make a powerful chorus, which is readily detected by even small radio telescopes.
Hydrogen line radiation was first detected by Harvard grad student Harold Ewen and his professor, Edward Purcell, in 1951. Their instrumentation, a simple waveguide horn antenna about a meter across driving a crude diode mixer, is now on display at the National Radio Astronomy Observatory (NRAO), Green Bank WV. It's also been memorialized in song.
Why is the hydrogen line protected spectrum? It's a great frequency for observing the structure of the universe, and some of the best and most detailed Milky Way radio maps have been made on the hydrogen line. It is probably the world's most popular radio astronomy frequency, and the International Telecommunications Union (ITU) has the good sense to protect it.
In 1959 two scholars (Philip Morrison at Cornell University and Frank Drake at NRAO) independently recognized that the hydrogen line would be a likely frequency for interstellar beacons. They reasoned that more advanced civilizations would reason that young civilizations (like ours) might already be listening there. Based upon that circular reasoning, Morrison went on to co-author the world's first modern SETI article ("Searching for Interstellar Communications," Nature 184(4690):844-846, September 19, 1959), and Drake conducted a the first modern SETI study, "Project Ozma," a hydrogen line search of two nearby Sun-like stars for possible artificial signals.
More:
http://www.setileague.org/askdr/hydrogen.htm