Messaging Extra-Terrestrial Intelligence (METI) – A Local Search

Abstract: This paper examines the feasibility of an amateur approach to METI using cheaply available
lasers and optics. We suggest a novel variation in the search methodology, concentrating on contacting any
interstellar extraterrestrial probes that may be present in the solar system. Specifically, the Lunar poles and
Lagrange points L4 and L5. It is assumed that such a probe incorporates advanced artificial intelligence (AI)
at or beyond human level. Additionally, that it is able to communicate in all major languages and common
communications protocols. The paper is written in non-technical language with sufficient information to act as
a “how to” source for technically knowledgeable people.

Note: Any portion of this may be reproduced and used in any manner provided attributions “Dirk Bruere” and the
organization “Zero State” are included.  Other more technical versions of this are available.

Historical Introduction

On 16 November 1974 The radio telescope at Arecibo sent a brief
message to the M13 star cluster some 25,000 light years distant. It
comprised some 210 bytes of data sent at a bitrate of 10 bits per
second and a power of around one megawatt. The (colored) pictorial
representation is shown here. It is probably the best known attempt at
contacting extraterrestrial intelligence (ETI), even though it was not
serious, was not the first and by no means the last.

The first was a Morse code message sent from the USSR to Venus in
1962 which was even shorter. It is known in Russian as the Radio
Message “MIR, LENIN, SSSR”.

Latterly, in 2016 on 10 October 2016, at 20:00 UTC the Cebreros
(DSA2) deep-space tracking station of the European Space Agency
sent a radio signal towards Polaris, the Pole Star, which is
approximately 434 light years from Earth. The message consisted of a
single 27,653,733 byte, 866 second transmission. Again, it was not a
serious contact attempt, and was rather more a work of performance
art by Paul Quast.

A few, more serious, attempts have been made in the intervening
years i, targeted at more plausible planetary systems but none for any
sustained period of time.

So, enter METI ii or “Messaging Extra-Terrestrial Intelligence” who aim to start a serious
and comprehensive program of signaling various star systems some time in 2018 if they
can raise the estimated $1million per year needed to run the program. For once, judging
by their website, they intend to do it properly with a great deal of effort going into the
communications protocols of the messages themselves.

Laser Communication

And that is where we were until June 2017 and a paper iii written by Michael Hippke
examining the possible role of using the gravitational lensing effect of our sun to amplify
laser signals across interstellar distances. The surprising conclusion was that using optical
wavelength lasers and mirrors of only one-meter diameter, data could potentially be
transferred at a megabit per second rates using around one Watt of power over 4 light years.
This, to put it mildly, is spectacular especially since the receiving technology is potentially
within our ability, assuming we could locate a telescope some 600 astronomical units (AU)
from the sun. Unfortunately, our most distant spacecraft is Voyager 1 at about 140AU. He
also showed in a previous paper that the data rate drops to bits per second per watt using
a 39-meter receiving telescope and no lensing.

However, if we turn that around and assume that ETI has superior technology to us and
can implement suitable receivers, then to contact them we need only very modest laser
transmitters. Ones that are well within the budget of hobbyists and amateur astronomers.
The advantage of using lasers is more apparent, especially for amateurs, when we
consider beam divergence. Lasers can quite easily achieve divergences of less than one
milli-radian (mrad) which corresponds to one meter per kilometer. To achieve that with
microwaves at (say) 6GHz would necessitate a transmitter dish of approximately 65
meters diameter. A very expensive piece of radio astronomy kit. This also means that
power levels can be significantly less than would be needed for radio communication.
Nevertheless, there are serious caveats. These mostly concern the location and type of
transmitter. For example, to limit beam spread Hippke assumes a one-meter diameter
mirror and a beam spread of considerably less than a milliradian, so we are going to
assume a rather larger receiver at the ETI end in order to minimize beam requirements at
our end.

A much more serious problem is that the mirrors have to be aligned with each other.
Specifically, the transmitter should be relatively stationary in space, and not on a rotating
planet which is in turn circling its sun. If the latter is the case, the receiver will probably
only align at fixed intervals lasting no more than a few tens of milliseconds unless very
precise aiming technology is used.

However, there is a more interesting search regime far better suited to low budget than
attempting interstellar communications.

Exploratory Scenario

This is a METI search that will be primarily focused on contact with self-replicating Von
Neumann (VN) style interstellar probes iv. There are strong arguments that over a time scale
of the order of thousands to a few million years, these are the best way of exploring the
galaxy by any intelligent technology-oriented species. Once one of these devices arrives in
a solar system it sets about creating sufficient infrastructure to both report back to its home
system (as well as possible siblings) and create a replica of itself for onward launch to
multiple other stars. Reasonably conservative capabilities are as follows:

  • They are very likely to outlive the species that sent them
  • They would almost certainly embody an artificial intelligence (AI) at or beyond
    Human level capability
  • They would be self-repairing and possibly have a lifetime in the tens of millions of
    years, barring accidents
  • They could exist around just about every star in the galaxy within ten million years

Using the kind of technology we might reasonably expect to appear sometime in the next
century or two, such as placing observatories at the gravitational focal point of our sun,
some 600AU out, we could view details on nearby extra-solar planets. And anyone out
there could do the same to us. As a consequence, Earth has likely been an interesting
place to view for the past 300 million years or so with its oxygen atmosphere and
vegetation. And vastly more interesting in the past 10,000 years since rectangular shapes
started appearing in the form of cities and fields. Rectangles generally do not occur
naturally. Then in the past 300 years, the atmosphere started to show signs of industrial
pollution followed 200 years later by radio and TV signals, intense radar pulses and the
unmistakable sign of nuclear bombs whose output peaked at around 1% of the total output
power of our sun.

If ETI exists, or has existed, within a few thousand light years there is a strong possibility
that their probes are already here, and have been for a considerable length of time.
This leads to a number of massively simplifying assumptions, again quite reasonable given
the scenario above. These are:

  • Since we are now searching within our solar system power levels can be vastly
  • Message transit times, in both directions, are no more than a few hours maximum
    and possible only seconds.
  • Any intelligent VN probe that has been examining Earth will have been monitoring
    our technological development and radio/TV output. As a consequence, it will almost
    certainly understand all the major languages both written and spoken as well as our
    communications protocols.

We need to consider beaming our messages at likely locations within our own solar
systems. For example, where would we place intelligent probes to wait out the ages and
watch developments on Earth? Among strong possibilities are the Lunar poles, Lunar
caverns which we now know exist v and the Lagrange points vi associated with Earth’s orbit,
particularly L4 and L5, where position can be held with little expenditure of energy. We
intend to beam laser messages to these points as part of the Zero State program.

But what messages? People have given much thought to creating a communications
system that can be decoded by ETI, as mentioned above with METI. However, we contend
that the answer is simple – we use English, and code in simple ASCII.

What has been lacking from Earth is a specific invitation to communicate or visit. It is this
that forms the core of our project.

How Far Can We Be Seen?

Suppose we want to do the crudest communication system possible – a laser doing Morse
Code. To the unaided Human eye, how far away could we see the beam? This depends on
several factors:

  • Beam Divergence
  • Beam power
  • Wavelength
  • Eye sensitivity

Taking these in turn…

The power we will assume to be one Watt since this level of power is quite economical,
and the wavelength to be either 532nm or 520nm, the latter being a pure diode output, not
frequency doubled.

It is also the approximate wavelength where the eye peaks in sensitivity, and in our project
is partly chosen for this reason. We could have gone for high power infrared in the tens of
watts, or maybe towards the blue/violent end of the spectrum. However, green is not only
easier and safer to work with, being highly visible, but is quite photogenic. From a safety
point of view you seriously do not want an invisible beam of blinding intensity sweeping
about. That would also be more difficult to aim and focus.

So we have an intensity of approximately one Watt per square meter at a distance of one
kilometer, with the intensity dropping off as the square of the distance. At 2 km we have
0.25W per square meter, and so on.

Finally, what is the maximum sensitivity of the dark adapted Human eye? It appears to be
about 100 photons per secondvii, but for the sake of argument we shall assume a level ten
times lower, or 1000 photons per second in a dark adapted eye whose aperture is 100
square millimeters. That gives us a minimum intensity requirement of 10^7 photons per
square meter per second. With each green photon carrying an energy of approximately
3.5e-19 Joules we get a required power density of 3.5e-12 Watts.

So, how far can our 1W green laser with a divergence of 1 mRad travel before we hit that
value? The answer is a little over 500,000km – further than the Earth-Moon separation. By
the time the beam gets there it will be illuminating a circle some 500km in diameter.
If we are looking back from the Moon via a modest telescope such a beam would appear
as a bright flickering point of monochromatic light. Even a 100mm diameter telescope
would improve visibility by more than 100 times.

If we wish to improve the numbers there are certain things we can do. If we increase the
power, it scales linearly in intensity at a given distance. If we increase the collimation to
(say) 0.5mRad the intensity quadruples, but the illuminated area decreases 75% as the
spot size halves.

Proof of Principle Equipment – Stage 1

The setup described below is an absolute minimum and has been put together simply to
illustrate how easy it can be, and how cheap.

WARNING! – The lasers described should be treated like a loaded firearms with the safety
off. Anyone around it should have eye protection goggles when it is operating or being
worked on. If it sweeps across your eyes it will cause instant permanent blindness. It can
also start fires. These are Class 4viii. You should also assume they will cause eye damage
out to 1km if the beam is not expanded.

The basic equipment list is relatively straightforward – example sources are UK but may
be obtained cheaply elsewhere:

• A computer with a USB interface
• A terminal emulator program such as Realtermix or similar
• A USB to TTL converter cable x
• A battery based stabilized power supply for the laser module
• High power laser module 1 Watt or greater xi
• A telescopic rifle sight (scope)
• A GOTO telescope
• Various Weaver rail fittings and adapters
• A low power sighting laser
• Laser safety goggles

Less straightforward is any metalwork or optical interfacing of the laser module, however,
the use of a scope with integral Weaver rails simplifies things considerably. The scope
needs an attachment to the GOTO telescope, and the rest of the equipment attaches to
the scope.

The next problem is that of holding the telescopic sight on target, which is where a
motorized equatorial mount, or GOTO mount is required. Both will compensate for the
rotation of the Earth and hold on a previously acquired target with accuracy much better
than the assumed mrad (for scale, the diameter of the full moon in the sky is about 9 mrad)
A GOTO telescope is fully computerized and will automatically move to designated targets
either by name or celestial coordinates.

The first step is to securely attach the laser module co-axially to the telescopic sight so
that you can see through the scope where the beam strikes. To do this you need a
deserted area where you can aim the beam at a target some 100 meters distant and
adjust optics and mechanical attachment so that the beam is aligned and parallel to the

At this point you can examine the beam quality. With modules such as the above it will not
be around spot. More likely it will be an image of the emission diode structure. Not ideal,
but good enough for now.

The pictures below show the scope, sighting laser and Class 4 laser complete with a DIN
rail that is used to attach all this to the telescope. In this instance, it is mounted on a
camera tripod for alignment work.

Illustration 1: Left Side of the Lasers and Optics


Illustration 2: Right Side of the Lasers and Optics


Illustration 3: Front view of the Lasers and Optics

Proof of Principle Equipment – Stage 2

So, how do we improve upon this? Well, the answer is obvious. Rather than relying on the
beam straight from the laser passing through the supplied focusing lens we use custom
optics to expand and collimate the beam. This at once gives us better control over the
divergence and by expanding the beam makes it somewhat safer by reducing areal power

Next, we add a receiver to the telescope eyepiece.

This consists of a bandpass optical filter centered at the wavelength of the laser
transmitter. Again, this assumes that any VN probe is quite capable of transmitting on the
received wavelength at a power level comparable to, or greater than, our own.
The necessary electronics, including a high sensitivity photodiode, is not prohibitively

Final equipment and Message Format

The above describes a minimal setup both from a cost and capability point of view. A more
suitable laser system would be one using a far higher power, and a receiving telescope
with a mirror at least 200mm diameter (8” reflector).

The choice of lasers is wide, but if we limit the choice to minimize atmospheric absorption
and costly optics that leaves visible and near infrared (NIR).

One possibility stands out. That is a Q-switched Nd:YAG laserxii, with around a 200W continuous,

1MW pulsed, output at 1064nm normally used as an industrial cutter. The
output can if necessary be frequency doubled to 532nm green but with loss of power.

This should be able to communicate with its equivalent to a distance beyond the orbit of

Such systems typically cost under $15k, although the optics, beam guides and alignment
equipment will add significantly to this price. Needless to say, such a beam in free space is
spectacularly dangerous if mishandled.

Additional requirements will include an electric generator or power source in the kilowatt
region, water cooling and a trailer if the equipment has to be moved to an open air site
before use.

All together we intend to budget around $30,000 for the hardware. Location is as yet
undecided, although a strong possibility is Provo, Utah in the USA given its clear skies and
weather. Britain is a poor second in this respect. Plus, we may locate it at the
TransHumanist Housexiii available to Zero State House Adar. However, much depends on
location and local laws.

The message format with Q-switched pulses would be somewhat different from the
existing setup. The coding would be provided by the timing between the pulses, or by the
timing between successive pulse trains. Again, data rate would be low because we are not
attempting to communicate anything complex. Just attract attention.

Zero State seeks collaboration from like-minded engineers and scientists, and sponsorship
for this project, which after initial hardware costs are met should incur very low running

Ethical Considerations

On 13 February 2015, scientists (including Geoffrey Marcy, Seth Shostak, Frank Drake,
Elon Musk and David Brin) at a convention of the American Association for the
Advancement of Science, discussed Active SETI and whether transmitting a message to
possible intelligent extraterrestrials in the Cosmos was a good idea; one result was a
statement, (which was not signed by Seth Shostak or Frank Drake), that a “worldwide
scientific, political and humanitarian discussion must occur before any message is sent” xiv
We believe that this is not, and should not be the case for local METI. We should issue the
invitation to communicate now. It is beyond reasonable doubt that if any ETI capable of
receiving these messages lies within our solar system or a few tens of light years, then
they already know of our existence.


iv Journal of the British Interplanetary Society, Vol.33, pp. 251-264 1980
vii S. Hecht, S. Schlaer and M.H. Pirenne, “Energy, Quanta and vision.” Journal of the Optical Society of America, 38, 196-208