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Showing posts sorted by relevance for query A BETTER WAY TO SEARCH FOR EXTRASOLAR PLANETS. Sort by date Show all posts
Showing posts sorted by relevance for query A BETTER WAY TO SEARCH FOR EXTRASOLAR PLANETS. Sort by date Show all posts

Wednesday, February 4, 2015

A BETTER WAY TO SEARCH FOR EXTRASOLAR PLANETS

Forty three years ago I used a tunable dye laser to catalyze/sterilize E. coli for my PhD Dissertation.  Three years later I worked for the NASA Ames Research Center on a project to design instruments to detect extrasolar planets.

Unfortunately, they had only a microwave interferometer in mind and passed on a concept I had advanced with Charles Townes (left, with his maser, and  right, my tunable laser) of the University of California at Berkeley to use the optical spectrum to not only find planets around other starts, but, as importantly, determine the atmospheric composition.  I again bring this subject up because last week Charles Townes passed away, and, coincidentally, a University of Hawaii researcher reported the day following that he had found three earth-like planets.  You will better understand my exasperation about this field after I provide some details.

This will be one of my more arcane and scientific postings ever, but I feel compelled to first point out that NASA astrophysicists and their kind are realistic about funding and their mission.  They feel uncomfortable and avoid any relationship with the looney tunes associated with flying saucers.  Similarly, their budgets are tiny, and the notion of trillion dollar Man on Mars efforts are beyond the pale.  Thus, while Carl Sagan's CONTACT (this is the entire 4 hr 39 minute audio book read by Jodie Foster) might be supportable, anything like Instellar and Star Wars are equally unrealistic, for while, yes, there are possible wormholes and so forth, the energy and technology required are beyond comprehension.

In some ways I was there at the beginning of the search for extrasolar planets (let me just called this SFEP) in the early 1970's.  Of course the modern search for extraterrestrial intelligence (SETI) began earlier in 1959 with the paper by Philip Morrison (right) and Giuseppe Cocconi, suggesting the microwave spectrum where signals might well be coming in from advanced civilians.  Cornell's Frank Drake actually performed Project Ozma (from Wizard of Oz--the field tends to get fanciful) in 1960 using a radio telescope in West Virginia to examine Tau Ceti and Epsilon Eridani, selecting 1.420 gigahertz as the frequency of opportunity, known as the water  hole, near where the hydrogen and hydroxyl  radicals have spectral lines (hint:  hydrogen plus hydroxyl equal water).  Of course he failed, but that is an entirely different pathway to actually doing something real.

Drake's (left) contention in those days was that it will be difficult to convince anyone to spend any money on SETI if our solar system had the only planets in the Universe.  So we needed to find a planet, call it an exoplanet or extrasolar planet, orbiting around any star somewhere in outer space.  Thus, NASA brought to the Ames Research Center in the Summer of 1976 20 faculty members from across the nation to design that first instrument to find that potential exoplanet.
For the reason that this group was headed by Jack Billingham and Barney Oliver (above in later life), who had previously run Project Cyclops, our team was commanded to design a microwave interferometer, which I didn't think was the ideal "telescope" for this particular application.  So they allowed me to find another option.  It was a grand summer of living in a Stanford married student apartment across the street from my freshman dormitory, golfing at the Palo Alto Muni, taking a wine-tasting course at night, watching the 1976 Olympics emanating from Montreal and, by the way, traipsing around northern California collecting info and talking to experts about an innovative way to find the first extrasolar planet.

I had just read a Science article by Charles Townes that planetary atmospheres lased.  He was already a hero of mine for he had won a Nobel Prize in 1964 and with his brother in law, Arthur Schawlow, who had come to Stanford University when I was junior there, had invented the laser, the instrument I used to conduct my PhD research.  So off I drove to Berkeley to meet with Professor Townes, who concurred with me that it might be possible to track the specific wavelengths of lasing extrasolar planets--we should be able to track planets circling stars at various discrete frequencies dependent on the atmospheric composition--thus also determining the life quality potential.  He said he would work with me on this project.  This a photo of Townes (above on the left) and Schawlow latter in life.  Alas, NASA ignored all our proposals, with a statement that the Hubble Telescope would soon fly to accomplish this task.

However, it took another 14 years for the Hubble to attain orbit in 1990 and the first confirmation of an extrasolar planet did not come until 1992.  But what confounds me is that NASA took a brute force technic called transit.  There are various ways to do this, some a lot more elegant.  All the Hubble did was watch stars that changed light intensity because a planet was reducing the light on passage across the star.  That's it.  The good news is that it has probably three more years of life yet.  While you keep seeing a tab of $1.5 billion, $10 billion is closer to the truth as the money spent on Hubble.

Even worse, in my mind, is that the replacement, the Kepler Telescope, only costing $600 million, which became operational in 2009, also used transit, a clearly obsolete technique.  Kepler lost its second gear in May of 2013, but some ingenious effort by scientists from the Ames Research Center has allowed the spacecraft to function for a short while longer.   I hate to say even worse, but the next telescope, the Transiting Exoplanet Survey Satellite, said to be a 2017 launch, will also use transit, but at least will only cost of $200 million.  Feel free to multiply that figure by any number from two to ten.  

But, ah, then, the biggie in 2018, the $8.9 billion (no, make that $10 billion+, for expenses reached $8.8 billion two years agoJames Webb Space Telescope with also a special spectrometer that should be able to analyze planetary atmospheres.  You know, this sounds suspiciously like the Townes-Takahashi Planetary Abstracting Trinterferometer.  But ah, no, because the Webb will only be able to do this for Jupiter-sized planets.  Then why bother???  And that cost was estimated in 2011.

The progress of SFEP:


Have you been counting the dollars?  Don't think NASA has been sleeping, for there are on drawing boards WFIRST, SALSO, OpTIIX and more.  Read the article.  These are mere billion dollar projects, but the James Webb only had a cost of $2.6 billion in 2009 and has jumped to past $10 billion today.  Hubble?  Original cost, $400 million.  Today? $10 billion.


Thus far, from zero in 1976 to zero in 1991 to perhaps 2000 exoplanet confirmations today, there must be ten times that number in the process being identified.  But NASA missed the point.  Frank Drake just wanted one to justify funding for SETI.  Sure, we need be more certain about where to look in the future for Earth-sized potential, but some reasonable logic can be used to argue that there must be intelligent life out there, many far more sophisticated than ours, having had a several billion year head start.


Above are the types of stars being explored.  While we are small compared to the really large ones, our Sun is, actually, brighter than 95% of all the stars.  Those M-types, the smallest, less than half our mass, make up 75% of all the stars up there.

So, to summarize, there are 100 octillion stars in our Universe, that's one followed by 29 zeros, and, perhaps 1 with 24 zeros planets. Something wrong with the logic here, for that means only one planet per 10,000 stars, but these come from two points of view.  Anyway, that's a whole lot of space, so let us for now limit our search just to our Milky Way Galaxy--remember, light takes 100,000 years just to cross from one end to the other--where one estimate is that we have about ten trillion planets.  Could Earth have been the only planet to gain intelligent life?

Which leads me to the article mentioned in the first paragraph about UH astronomer Andrew Howard, quoted to have discovered:

Three Earth-size planets — one possibly with liquid water on its surface — have been found around a distant star with help from the Keck Observatory on Mauna Kea.

What great astrophysics right?  Well, the science used to suggest water was an observance that one of these three is 1.5 the size of Earth, and occupies the so-called "Goldilocks Zone," where water could exist.  Did they detect water?  Nope, the star, EPIC 201, is 150 light years away.  This means that if there is life there, and we make contact, each call will involve a 300 year + wait.  Three hundred years ago was 1715.  George Washington, our first president, was not born until 1732,  The transit technique of course only provides the rough size and location of an extrasolar planet, not the atmosphere.  But the jaded would remark, so what, Planet Earth did it already.

The odds are overwhelming that gazillions of exoplanets have the potential for life-supporting ecosystems.  And many of them could be at least 8 billion years older than us.  Let's get on with capturing extraterrestrial intelligence messages.  Simple step one:  remove the congressional language preventing NASA from doing any SETI work.  Simple step two:  give a billion dollars a year each to NASA and the SETI Institute to re-initiate the effort suggested in CONTACT.


In a decade--after expending $20 billion, less than what has thus far been consumed with current-transit-connected telescopic attempts--review the reality of SETI.  If the weight of science leans in the direction of the Fermi Paradox or the Proxmire Golden Fleece Award, than abandon the effort for another century or millennium.  While the visions of an Encyclopedia Galactica streaming past Planet Earth to provide magical solutions for our needs are enticing, it is possible that we are the only semi-intelligent life in our Universe.

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Thursday, March 4, 2021

MY LIFE IN LASERS AND HYDROGEN

    From Worldometer (new  COVID-19 deaths yesterday):


        DAY  USA  WORLD   Brazil    India    South Africa

June     9    1093     4732         1185       246       82
July    22     1205     7128        1293      1120     572
Aug    12     1504     6556        1242       835      130
Sept     9     1208      6222       1136      1168       82
Oct     21     1225      6849         571       703       85
Nov    25     2304    12025        620       518      118
Dec    30     3880    14748       1224       299     465
Jan     14     4142   15512        1151       189     712              
Feb      3      4005   14265       1209       107     398
          25       2414   10578       1582       119     144
Mar     2       1989      9490       1726       110     194
            3       2350   10838        1840        86       95

Summary:   Well, a turn for the worse.  Hopefully an anomaly.  Texas...Mississippi...no masks...why?


Well, this is March 4, and how's the Second Coming of Donald Trump progressing?  Where are those QAnon terrorists?  Why is the U.S. Capitol not being overrun again?  Why is the House of Representations so afraid about a second onslaught that it cancelled sessions for the rest of the week?

POLITICS!  Democrats just want to take advantage of this moment to better reinforce the minds of voters of how terrible Republicans are, Trump in particular.  The House is on danger leave only to underscore those brave Democrats in the Senate who are going to work under these stressful circumstances to insure that voters better appreciate them for passing the COVID-19 relief package to minimize evictions, hunger and contraction of this deadly virus.


About the topic of today, LASER is the acronym for the light amplification by stimulated emission of radiation.  The theory was developed by Charles Townes and Arthur Schawlow, and the first maser (the m being for microwave) was built by Theodore Maiman in 1960.  Townes was mostly at MIT and Schawlow at Bell Labs when they began their research in this field.  They both became Nobel laureates.  Schawlow joined Stanford when I was a junior there, and Townes went to Cal-Berkeley in 1967.  

My life entered Townes' when I spent some time on a Search for Extraterrestrial Intelligence (SETI) project for the NASA Ames Research Center, where the concept of laser light played a key role in linking me with his ideas.  Interestingly enough, as you will learn, my wife was a key factor in all of this.


So let me digress a bit, for I've entered the disposal stage of my life.  I am throwing away a lot of apartment clutter, starting with photo accoutrements and slides, of which I must have around 5000.  I'm sorting out which ones to digitize, and in my first batch to see if this actually worked, found some which I haven't seen in half a century, and didn't know they even existed.

To begin, just to underscore Pearl's involvement, I'll start by showing these just discovered photos in chronological stages.  The first one in 1963 soon after we were married when we were in Kilauea, Kauai, and our backyard was where South Pacific was filmed.  The second was a few years later at her family home in Hilo:

Then the third, just about exactly half a century ago, sitting in my biochemical laboratory at LSU:


She was the inspiration for my torturous path towards a PhD dissertation, which was indeed a rocky road.  The results were published in a 1975 issue of Applied Microbiology entitled: 

One day in 1969 she was reading a laser article in LIFE magazine and said, why don't you use a laser in your research?   Sorry I heard that, for I subequently suffered through three years of frustrating agony.  To begin, I came up with an idea to use a laser to sterilize microbiological processes.   I first had to build a tunable laser, for in those early days, you couldn't purchase one,  This product was too new.  But how to get the funds to do it yourself?  With my major professor, Barry Greenberg, we found a company, Milk Protein, which was interested in finding a better way to pasteurize milk.  They funded the hardware effort.

I bought the equipment and couldn't get the system to lase.  I was about to give up when I learned that two of my nephews had drowned in Utah.  So I went to their funeral.  On the flight back, looking out the window, a second inspiration just appeared in my mind, the clue on how to adjust the diffraction grating.  Went back to my lab, and this vision worked!

That was just stage one.  The only wavelengths I could get were in the visible range


The science in those days was limited to visible wavelengths, and I needed to get down to 265 nanometers for optimal dissociation of the DNA bond in E. coli.   Frequency doubling, or using monochromatic light at 530 nm to convert down to 265 nm was theoretically possible.  However, the available technology was only 0.01% efficient, which made the beam too weak to do anything.

The only solution was an exogenous photosensitizer (a dye) to transfer the energy to the bond.  Rhodamine 6G produced a range of 556-610 nm light, while Coumarin gave 441-475 nm  You would have thought that the Coumarin would have had a higher sterilization efficiency, being closer to the desired 265 nm wavelength.  The results were startling.  The R6G did induce killing of E. coli.  However, the Coumarin catalyzed growth.

We could never figure out why, but actually discovered a technique to enhance the growth of desirable bacteria using a laser attuned to a certain wavelength.  I wonder why no one or company has taken advantage of this potential for industrial products?  Anyone seeking a way to a fortune, look into this.

I did get my PhD in biochemical engineering, but I later realized that what I did was patently foolish.  Most doctoral students pick a topic where a professor already has funds to focus on a topic approved by a Federal agency.  In addition, the notion of finding your own funds to do research, then entering a field which had no precedent, was simply idiotic.  The younger person in my laboratory who was supposed to continue my work ended up developing a mathematical model, I think.  Never had to build or irradiate anything.  This is the smarter model in getting a PhD.  Only when you get into the real world do you need to actually do something tangible.


I should mention that Harry Toups was this individual, who today is running the laboratories in the LSU Chemical Engineering Department.  He and Margaret still communicate with me.  Maybe they can be convinced to join the around the world journey.  I also found a few slides of our days then, so someday I'll add photo here of us in those days.


So anyway, this laser experience a couple of years later led to me to work with Nobel Laureate Charles Townes (I drove from the Stanford campus to Berkeley for our encounters, actually spending most of my time golfing at Palo Alto Muni, watching the Summer Olympics on TV and taking a wine-tasting course) on a proposal to detect extrasolar planets on his contention that all planets with atmospheres absorb starlight, then, depending on conditions, show promise for stimulated emission at monochromatic wavelengths that would also define the gas itself.  Thus, even though the starlight is ten million times brighter, this light occupies the entire spectrum, while the reflected atmospheric lumens for a well defined monochromatic wavelength we determined should be trackable.  We would be able to see an exoplanet circle a planet outside our solar system.  You can read about what we were trying to do in this posting of six years ago entitled:

It was probably not a good idea to call this system the Planetary Abstracting Trinterferometer (or PAT for short).  But it probably did not make much difference for future funding because NASA had earlier made a determination that in searching for anything in outer space, they would use the microwave portion of the spectrum because signals are less diminished over long distances compared to visible light.  I closed that posting with:


In the meantime, my attitude has shifted, so I'm not advocating even bothering with PAT.  In 1976, yes, let's go confirm a planet outside our solar system.  Now?  Why bother to find any more, as we have found a thousand, (That was 8 years ago.  As of 28January2021, there were 4,341 confirmed and another 5,000 or so being analyzed) and astronomers have already said that there could be more than 100 billion Earth-like planets in our galaxy that could be home to life. Further, there could be 500 billion other galaxies in our Universe.  Let's instead expand our efforts to detect possible signals from aliens.  On with SETI!  Bring back Jodie Foster, sometimes known as Jill Tarter of the SETI Institute.  If you clicked on the Jodie Foster link, and want to hear more, go HERE.  Should you be as enamored of the notion of FIRST CONTACTthis video gives you the top ten films on this subject.  Contact is only #5.  What was #1?  Go ahead, take a look.

Then the following year I found myself at the Lawrence Livermore Livermore National Laboratory to work on laser fusion.  Fusion is the process our sun and all the stars use, with hydrogen as the fuel, to produce energy.  Man-made fusion utilizes isotopes of hydrogen, deuterium and tritium, because we are not able to meet the conditions existing at the core of the sun.  Alas, I thought, after a couple of summers there, that the technology was at least 30 years away from commercialization.  Recently, meaning 43 years later, fusion is still 30 years away, and that is being optimistic.


But taking everything into consideration, I thought, maybe there might be something to hydrogen, for it is the first element (one would think a divine clue), is most (73%) of the Universe, and if combined with oxygen, you get energy and water.  Surely, there is a message here.

Further, Hawaii's economy depended on air transport, and hydrogen, being the lightest jetfuel (or maybe even for a fast-moving dirigible, like Brutoco's Clipper), would be ideal for future jets.  Read my HuffPo of a decade ago.


Fortuitously, in 1979 I was asked to work for Senator Spark Matsunaga and drafted the first hydrogen bill that became law.  Later on, the Hawaii Natural Energy Institute, which I directed, became one of the Department of Energy's national hydrogen research and training centers, plus I chaired the Secretary of Energy's Hydrogen Technical Advisory Panel, which produced The Green Hydrogen Economy, setting the budget level for the next five years.  Incredibly enough, Congress exactly followed our recommendations to the point where in one year the hydrogen budget was higher than solar technology.  It then later occurred to me that one way to accelerate the hydrogen economy was to make this fuel free.  Some of my ideas are outlandish, but on analysis, actually make sense.

While SETI, World Peace, the Hydrogen Economy, Fusion and the Blue Revolution will probably not be actualized in my lifetime, I do take some pride in the initiation of a variety of potentially promising pathways for Humanity.  Most I believe will attain reality, but it might take a century, or more.  I hope the first floating city from the Blue Revolution, for one, will host the 2050 World Expo.

I've long wondered where I'd be if Pearl did not mention lasers to me, or I never met her.  Maybe I'd be richer or famous or homeless.  One's life can change with just any fateful decision.  Even today.


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Tuesday, November 24, 2009

CHAPTER 4: SEEKING THE LIGHT—SETI (Part 2)

The following continues the serialization of Chapter 4 on the Search for Extraterrestrial Intelligence (SETI) from SIMPLE SOLUTIONS for Humanity:


SETI in the 70’s


In 1971, Bernard Oliver of Hewlett-Packard and John Billingham of the National Aeronautics and Space Administration (NASA) Ames Research Center (ARC) conducted a summer workshop, and the group picked 1.42 GHz, the spectral line caused by interstellar hydrogen, and 1.66 GHz, caused by hydroxyl ions, called the “Water Hole,” as the ideal portion of space to conduct the search. For one, water symbolized life, and two, that band was relatively quiet. There is now that transitional link, for Book 1 featured a chapter reporting on hydrogen. Maybe there is something about hydrogen that goes beyond mere future sustainable utility.


In 1972, Oliver and Billingham authored a NASA study proposing an array of one thousand 100-meter telescopic dishes to pick up television and radio signals from neighboring stars. Project Cyclops was projected to cost $10 billion (which is $50 billion in 2009 dollars), but was never seriously considered. At this point in history, the U.S. Congress was not aware, or cared, that NASA was doing SETI work.


As an assistant professor of engineering, I then teamed with the resident futurist at the University of Hawaii, James Dator, and the National Aeronautics and Space Administration, on “Earth 2020: Visions for Our Children’s Children,” where in the summer of ‘74 we brought to Hawaii noted lecturers of national stature in topics related to Planet Earth, the environment and space, and weekly filled a two thousand seat auditorium. We also conducted a workshop for forty or so secondary and university faculty.


Having been thusly enlightened with this course, many of them went on to become principals, a university president, a provost, and elected public officials. Professor Dator later gained fame as Secretary General, then President, of the World Futures Study Federation. Identical summer workshops were held at San Jose State University and San Diego State University, with the advanced planning final report prepared by faculty from all three workshops. There was also a lot of cross-fertilization with the leaders of Project Cyclops. The information and curricula we generated became the standard instructional tools for a large number of teachers in Hawaii and California in the growing field of environmental consciousness. Remember, this was more than a third of a century ago.


Having thus been exposed to the SETI field, in 1976 I joined 19 other university faculty members from across the nation at NASA's Ames Research Center in Mountain View, California, on Project Orion, to detect an extrasolar planet (or exoplanet, used interchangeably), that is, a planet revolving around another star, spearheaded, of course, by Oliver and Billingham. The first question asked of Cornell Professor Frank Drake was: “Extraterrestrial intelligence? How do you know there are even other planets outside our solar system?” So the faculty group was tasked to design a system to accomplish this feat. Why me? Well, I had an idea on how to do this, plus I long harbored visions that the cure for cancer and the solution to world peace might be beaming unto Planet Earth from advanced civilizations.


Originally, in the mid 1800’s, stars were classified by hotness (Class I for white and blue, down to Class IV for red and Class V). Early in the 1900’s, the Harvard classification was adopted, ranking stars by luminosity—O, B, A, F, G, K, and M—Oh Be A Fine Girl, Kiss Me.


F and G type suns seem best suited for planets. Our Sun is in the latter category, and the guess is that there is a 7% chance for a solar system, while the former is 1.3 to 1.5 solar masses, with a 10% chance of planets. Planets do not form in binary star systems, and have a higher probability of creation in galactic arms where heavy elements are located. There is a 20-30% chance towards the external portion of a galaxy, where we are located.


How does a planet form? Well, more and more, astronomers are seeing disks surrounding stars. Very simply, the dust agglomerates into planets. Thus, first find a planet, any planet. Then, find planets where life is possible. These sites should be:


o older than 3 billion years;

o with a star smaller than 1.5 times our Sun mass;

o having a stable location between galaxy spiral arms; and

o in a solar system which is singular, that is, without a binary star.


While most of the team went on to design an interferometric system to indirectly do the job, a few of us were allowed to pursue other directions. Indirect means to measure something else. That is, as you can’t see that extrasolar planet, the starlight being so intense relative to the reflection from the planet, measure the orbit wobble of the star, with the pattern mathematically being fitted for possible planets. Direct means somehow block out the starlight and see that extrasolar planet, or, better yet, actually measure and track something, anything, from the planet itself. I was the only one to take this latter option, for I like to see what I’m doing, and the optical spectrum was my choice.


That same previously mentioned (in Chapter 2) Charles Townes, who had won the Nobel Prize for the laser, and who will later be mentioned in Chapter 10 for being awarded the 2005 Templeton Prize (generally given to a noted scientist who has religious predilections), happened to just arrive at the University of California Berkeley from the Massachusetts Institute Technology in 1976, and had published a paper speculating that planetary atmospheres lased (that is, flashed a well-defined color like in a typical laser, representing the gaseous molecule undergoing this phenomenon).


As an aside, there is something karmic coupling the afterlife with SETI, as Science Digest, in its October 1985 issue on “The 20 Greatest Unanswered Questions of Science,” featured on its front cover, English-born and Princeton professor Freeman Dyson, the 2002 Templeton Prize awardee. Dyson was asked the question, “Are We Alone in the Universe?” He responded, “engaging in mathematical calculations on the probability of intelligent life elsewhere in the universe is not a worthwhile exercise. The universe may be crawling with life. The answer is: Wait and see.” Dyson had previously worked on a different Orion Project, but that was around 1960, and it had to do with using nuclear pulse propulsion for space-flight.


Anyway, returning to the discussion, a Jupiter-size planet cannot be seen revolving around a typical Sun-size star tens of light years away because the starlight is so much brighter by 5 to 10 orders of magnitude (meaning 10 to that power, or in the inverse, the light from an extrasolar planet is from 1/100,000 to 1/10,000,000,000, or one ten billionth that of the star). However, if the planetary atmosphere lased, then these spiked discrete frequencies, first, might well be detectable because you would know exactly which monochromatic colors to check (the lasing frequency of those gases that would be found in planetary atmospheres), thus, also, this would accordingly give the atmospheric composition. Conversely, if no lasing is detected, then that planet has no atmosphere, and can summarily be deleted from future consideration regarding the potential for harboring life. My PhD dissertation experience, which included building a tunable laser before you could purchase one, provided this spark of imagination. I went to see Professor Townes, and he graciously provided encouragement.


My final report to NASA was called “To See the Impossible Dream: the Planetary Abstracting Trinterferometer (note the acronym, PAT),” with a Man from La Mancha symbol on the cover. I of course quoted Miguel de Cervantes:


To Man, the Don Quixote of the universe

May he succeed in his impossible dream.


At first I thought David Black, the NASA coordinator, reacted to my paper as being some kind of joke, but I now understand that optical searches were not company policy. That is, as it makes a lot more technical sense to measure the microwave spectrum for actual alien signals, NASA seemed wedded to focusing only on that particular technology, even for detecting extrasolar planets. Why microwave? These signals can travel further in space (less degradation) than optical ones.


Anyway, Black surmised that the Hubble Telescope would be soon to fly and find such exoplanets. Hubble was actually deployed 14 years later, and only in 2008 (32 years later) detected a planet orbiting a star. This telescope was serviced one final time later in 2009 for operation until 2013, when the James Webb Space Telescope is expected to be launched. Without an orbit reboost, the Hubble could plunge to Earth sometime soon after 2019. In any case, the prevailing convention then, as now, was to explore and receive the microwave band, so anything resembling optical searches did not meet the accepted requirements.


Either way, there is a timing concern, as, more and more, new commercial communications satellites will cloud the radio spectrum, especially in the range of the most promising detection channels. Thus, SETI will soon need to move into outer space if the focus is to continue traditional interferometry measurement techniques on Earth.


Two final bits about the ‘70’s, in 1975, the U.S. Congress published “The Possibility of Intelligent Life Elsewhere in the Universe.” In 1978, Senator William Proxmire (D-Wisconsin) selected NASA’s SETI program for one of his famous Golden Fleece Awards. The following year found me in Washington, D.C. as U.S. Senator Spark Matsunaga’s Special Assistant on Energy. Little did I know that while helping to solve our second energy crisis, one of my more interesting tasks would be related to SETI.

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At one point today, the Dow Jones Industrials dipped more than 100 points. However, the DJI ended down only 17 at 10,434, while world markets were also mostly lower. Gold continued to set world records, jumping $9/toz to $1169. Crude oil is now around $77/barrel.

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Tropical Typhoon Nida, at 115 MPH, was at first heading in the general direction of Guam, located 200 miles away, but now looks to move towards southern Japan, perhaps in a week. There is a tropical depression now affecting Mindanao (southern Philippine island). Tropical Cyclone Bongani, at 40 MPH, is moving west, just north of Madagascar.

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