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National Radio Astronomy Observatory

National Radio Astronomy Observatory

Search complete. 13 mentions across 9 episodes found for "National Radio Astronomy Observatory".

Oct 2, 2026

H. Paul ShuchGUEST
44:29
No, unfortunately not.
H. Paul ShuchGUEST
44:30
They were using the Arecibo dish, and they were borrowing time on a really nice big telescope in Australia, and they would rent time from the NIO, Green Bank, West Virginia.
H. Paul ShuchGUEST
44:46
Big stuff.
H. Paul ShuchGUEST
44:47
Well, because it's a long shot with your targeted search, the second search strategy is called the All-Sky Survey.
H. Paul ShuchGUEST
45:20
So NASA wasn't about to bet on one or the other.
H. Paul ShuchGUEST
45:23
They bet on both.
H. Paul ShuchGUEST
45:25
JPL got involved with one of the searches, and National Radio Astronomy Observatory got involved in the other search, and they had these both going on a three-year plan at $12 million a year.
H. Paul ShuchGUEST
45:36
That's, by the way, five cents per U.S. citizen per year.
Brennan ByrneHOST
4:50
Frank Drake studied astronomy, getting his PhD from Harvard in 1958.
Brennan ByrneHOST
4:55
His first job was at the National Radio Astronomy Observatory in Green Bank, West Virginia.
Brennan ByrneHOST
5:01
And it was there in 1960 where he would get that chance to detect those other civilizations in our universe that young Frank wondered about.
Brennan ByrneHOST
5:10
That year, he convinced the observatory director to give him $2,000 to conduct the first search for life outside our own planet.
Samantha ScibelliHOST
41:38
I'm Samantha Schibelli.
Samantha ScibelliHOST
41:39
I'm a postdoctoral fellow at the National Radio Astronomy Observatory in Charlottesville, Virginia.
Samantha ScibelliHOST
41:45
I'm interviewing Funga Hill, who was an undergraduate at the University of Arizona and now is starting graduate school at the University of Michigan.
Samantha ScibelliHOST
41:56
I want to start by asking first, Funga, how did you get interested in astrochemistry?
James Sobel KellyNARRATOR
3:49
The first serious effort to detect radio signals from alien civilizations in deep space was made in 1960, when the American astronomer Frank Drake conducted an experiment he named Project OSMA.
James Sobel KellyNARRATOR
4:03
Using a telescope at the National Radio Astronomy Observatory in West Virginia, Drake looked for signals at a precise location on the electromagnetic spectrum.
James Sobel KellyNARRATOR
4:14
1420 megahertz, known as the hydrogen line, because hydrogen atoms emit photons at that frequency.
James Sobel KellyNARRATOR
4:23
Because hydrogen is so abundant in the universe, the line is easy for radio telescopes to detect.

Unknown podcast

The Fermi Paradox Is More Terrifying Than We Thought

Sep 5 · 1 Mention

speaker_1NARRATOR
18:09
One year before Drake wrote his equation, he had already conducted the first modern search for extraterrestrial intelligence.
speaker_1NARRATOR
18:17
In the spring of 1960, Drake pointed the 85-foot radio telescope at the National Radio Astronomy Observatory in Greenbank, West Virginia, toward two nearby sun-like stars, Tau Ceti and Epsilon Eridani.
speaker_1NARRATOR
18:34
He called the project Ozma, after the princess of the fictional land of Oz, a distant and unreachable place filled with exotic beings.
speaker_1NARRATOR
18:43
For roughly 200 hours over several months, Drake listened for narrowband radio signals, the kind that natural astrophysical sources do not produce, that would indicate deliberate transmission by an intelligent civilization.
Stuart GaryHOST
8:25
In the meantime, another possibility is to point powerful telescopes at Enceladus and use those to try and get a spectroscopic reading of those tiny water and ice grains erupting into space from the tiger stripes.
Stuart GaryHOST
8:38
This report from the United States National Radio Astronomy Observatory.
Bryan ButlerSOUNDBITE_SPEAKER
8:43
Enceladus has geysers at its south pole.
Bryan ButlerSOUNDBITE_SPEAKER
8:49
It has what almost are the equivalent of geothermal geysers on the Earth.
Bryan ButlerSOUNDBITE_SPEAKER
9:44
So on Enceladus, is there some ocean where material is coming up through the crust and that's what's coming out in these geysers? So we'll be able to quite accurately measure the abundances of the different kinds of molecules that are in that, you know, that ring of material around Saturn.
Bryan ButlerSOUNDBITE_SPEAKER
10:04
And because it has such fine resolution, we'll actually be able to make an image of Enceladus and right over where the geysers are, we'll have, you know, the resolution to see precisely what's in that area, what's coming out, what the temperatures are, again, what the, the abundances are of the materials that are coming out.
Stuart GaryHOST
10:26
And in that report from the National Radio Astronomy Observatory, we heard from scientist Brian Butler.
Stuart GaryHOST
10:31
This is Space Time.
Stuart GaryHOST
7:55
In the meantime, another possibility is to point powerful telescopes at Enceladus and use those to try and get a spectroscopic reading of those tiny water and ice grains erupting into space from the tiger stripes.
Stuart GaryHOST
8:08
This report from the United States National Radio Astronomy Observatory.
Brian ButlerSOUNDBITE_SPEAKER
8:13
Enceladus has geysers at its south pole.
Brian ButlerSOUNDBITE_SPEAKER
8:19
It has what almost are the equivalent of geothermal geysers on the Earth.
Brian ButlerSOUNDBITE_SPEAKER
9:24
quite accurately measure the abundances of the different kinds of molecules that are in that, you know, that ring of material around Saturn.
Brian ButlerSOUNDBITE_SPEAKER
9:34
And because it has such fine resolution, we'll actually be able to make an image of Enceladus, and right over where the geysers are, we'll have, you know, the resolution to see precisely what's in that area, what's coming out, what the temperatures are again, what the abundances are of the materials that are coming out.
Stuart GaryHOST
9:55
And in that report from the National Radio Astronomy Observatory, we heard from scientist Brian Butler.
Stuart GaryHOST
10:01
This is Space Time.

Unknown podcast

The Dark Forest Theory_ Why One Signal to Aliens Could End Us

Sep 4 · 1 Mention

speaker_0NARRATOR
2:51
In 1961, astronomer Frank Drake attempted to put numbers to this intuition.
speaker_0NARRATOR
2:57
Working at the National Radio Astronomy Observatory in Greenbank, West Virginia, Drake developed an equation designed to estimate how many communicative civilizations might exist in our galaxy at any given time.
speaker_0NARRATOR
3:10
The Drake equation, as it became known, multiplied together a series of factors the rate of star formation in the galaxy, the fraction of stars with planetary systems, the fraction of those planets that could support life, the fraction where life actually develops, the fraction where intelligence emerges, the fraction that develop technology capable of sending detectable signals, and the average length of time such civilizations continue broadcasting.
speaker_0NARRATOR
3:39
The equation was never meant to produce a precise answer.
speaker_0NARRATOR
1:49
The telescope does not hear with ears, it hears with mathematics.
speaker_0NARRATOR
1:55
In the spring of 1960, a young astronomer named Frank Drake pointed an 85-foot radio telescope at the National Radio Astronomy Observatory in Greenbank, West Virginia, at two nearby sun-like stars.
speaker_0NARRATOR
2:12
Their names were Tau Ceti and Epsilon Eridani, and they were chosen because they were close, because they were similar to our own Sun, and because they seemed like reasonable places to begin.
speaker_0NARRATOR
2:26
Drake listened for narrow band radio signals at the hydrogen line frequency, 1420 MHz.

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