Alex McColgan

A signal, which later came to be known as BLC-1. Could the star closest to our own actually harbor advanced alien life? The signal was fascinating, as it could not easily be explained away by conventional sources. It lasted for several hours, which is longer than the time it normally takes a human satellite to pass by overhead. It had signal drift.

A signal, which later came to be known as BLC-1. Could the star closest to our own actually harbor advanced alien life? The signal was fascinating, as it could not easily be explained away by conventional sources. It lasted for several hours, which is longer than the time it normally takes a human satellite to pass by overhead. It had signal drift.

Its frequency was shifting, which implied possible movement relative to the telescope, so it likely wasn't coming from a stationary object creating interference on Earth. One of the most compelling things it had going for it was its thin, narrowband signal. In nature, radio waves are never so narrow in their range. They always fluctuate.

Its frequency was shifting, which implied possible movement relative to the telescope, so it likely wasn't coming from a stationary object creating interference on Earth. One of the most compelling things it had going for it was its thin, narrowband signal. In nature, radio waves are never so narrow in their range. They always fluctuate.

Its frequency was shifting, which implied possible movement relative to the telescope, so it likely wasn't coming from a stationary object creating interference on Earth. One of the most compelling things it had going for it was its thin, narrowband signal. In nature, radio waves are never so narrow in their range. They always fluctuate.

Unless there exists some natural source out there we've not discovered yet, the only thing that produces such a concise signal as this is technology, either human or alien. When no obvious explanations for existence could be found amongst human sources, naturally scientists wondered, could this be the signal from alien life they had been looking for?

Unless there exists some natural source out there we've not discovered yet, the only thing that produces such a concise signal as this is technology, either human or alien. When no obvious explanations for existence could be found amongst human sources, naturally scientists wondered, could this be the signal from alien life they had been looking for?

Unless there exists some natural source out there we've not discovered yet, the only thing that produces such a concise signal as this is technology, either human or alien. When no obvious explanations for existence could be found amongst human sources, naturally scientists wondered, could this be the signal from alien life they had been looking for?

Zusammen mit dem Wow-Signal, den wir in einem vorherigen Video gesehen haben, ist der BLC1 einer der stärksten Kandidaten für Signale, die von alienen Zivilisationen hergestellt werden können. Und trotzdem hat auch dieser Signal seine Vorteile. Wissenschaftler konnten ihn nicht mit irgendwelchen Gründen der offiziellen Interferenz von Technologie auf der Erde verbinden,

Zusammen mit dem Wow-Signal, den wir in einem vorherigen Video gesehen haben, ist der BLC1 einer der stärksten Kandidaten für Signale, die von alienen Zivilisationen hergestellt werden können. Und trotzdem hat auch dieser Signal seine Vorteile. Wissenschaftler konnten ihn nicht mit irgendwelchen Gründen der offiziellen Interferenz von Technologie auf der Erde verbinden,

Zusammen mit dem Wow-Signal, den wir in einem vorherigen Video gesehen haben, ist der BLC1 einer der stärksten Kandidaten für Signale, die von alienen Zivilisationen hergestellt werden können. Und trotzdem hat auch dieser Signal seine Vorteile. Wissenschaftler konnten ihn nicht mit irgendwelchen Gründen der offiziellen Interferenz von Technologie auf der Erde verbinden,

Aber nach einer kürzeren Beobachtung der Daten, gab es andere Radio-Wave-Signaturen, die auf anderen Tagen des Suchens entstanden sind, außer dass diese anderen Signale, egal in welcher Richtung der Teleskop beobachtet wurde, stattgefunden haben. Nichtsdestotrotz konnten sie die BLC-1-Signale von Proxima Centauri entdecken, mit späteren Observationen.

Aber nach einer kürzeren Beobachtung der Daten, gab es andere Radio-Wave-Signaturen, die auf anderen Tagen des Suchens entstanden sind, außer dass diese anderen Signale, egal in welcher Richtung der Teleskop beobachtet wurde, stattgefunden haben. Nichtsdestotrotz konnten sie die BLC-1-Signale von Proxima Centauri entdecken, mit späteren Observationen.

Aber nach einer kürzeren Beobachtung der Daten, gab es andere Radio-Wave-Signaturen, die auf anderen Tagen des Suchens entstanden sind, außer dass diese anderen Signale, egal in welcher Richtung der Teleskop beobachtet wurde, stattgefunden haben. Nichtsdestotrotz konnten sie die BLC-1-Signale von Proxima Centauri entdecken, mit späteren Observationen.

Also, obwohl sie nicht genau wissen, was mit dem Teleskop interferiert hat, um BLC-1 zu produzieren, sind die Chancen, es zu interferieren, allerdings ziemlich hoch. Let's take a look at another candidate, the somewhat mouthier SHGB02-14a.

Also, obwohl sie nicht genau wissen, was mit dem Teleskop interferiert hat, um BLC-1 zu produzieren, sind die Chancen, es zu interferieren, allerdings ziemlich hoch. Let's take a look at another candidate, the somewhat mouthier SHGB02-14a.

Also, obwohl sie nicht genau wissen, was mit dem Teleskop interferiert hat, um BLC-1 zu produzieren, sind die Chancen, es zu interferieren, allerdings ziemlich hoch. Let's take a look at another candidate, the somewhat mouthier SHGB02-14a.

When one of the first SETI experiments, Project OSMA, was started in 1960 by Frank Drake, it began on the basis that if alien life were to communicate with the rest of the universe, they would do so at frequency 1420 MHz. The logic behind this was that this was the frequency emitted commonly by hydrogen, one of the most widespread elements in the universe.

When one of the first SETI experiments, Project OSMA, was started in 1960 by Frank Drake, it began on the basis that if alien life were to communicate with the rest of the universe, they would do so at frequency 1420 MHz. The logic behind this was that this was the frequency emitted commonly by hydrogen, one of the most widespread elements in the universe.

When one of the first SETI experiments, Project OSMA, was started in 1960 by Frank Drake, it began on the basis that if alien life were to communicate with the rest of the universe, they would do so at frequency 1420 MHz. The logic behind this was that this was the frequency emitted commonly by hydrogen, one of the most widespread elements in the universe.