Cosmic Diary Marchis

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Let’s be careful about this “SETI” signal

August 29, 2016

Several readers have contacted me recently about reports that a group of international astronomers have detected a strong signal coming from a distant star that could be a sign of a high-technology civilization. Here’s my reaction: it’s interesting, but it’s definitely not the sign of an alien civilization—at least not yet.

Jodie Foster in the movie “Contact”

Here’s why:

  1. The signal was first detected in May 2015 and has not repeated since. Unfortunately, although international protocols call for alerting the astronomical community to the detection of a mysterious signal, the observers chose not to do so. Sadly, their failure to observe this simple protocol likely hindered our ability to clarify exactly what caused the signal.
  2. The signal was detected by an antenna that is very complex—and one that a colleague of mine who is a radio astronomer said could have mislabeled a terrestrial signal (i.e, one from a satellite or airplane) crossing the side lobes of the beam when the observation was made. In other words, the pointing quality of this antenna is so uncertain that it may have captured what we call a false or “parasite” signal.
  3. HD 164595, the host star, is very similar to the sun (same color, size, and age). It’s ninety-one light years from Earth and has a known planet, HD164595 b, which is probably Neptune-like and orbits very close to its star every forty days. We have not yet detected an Earth-like or super-Earth-like planet around this star, and do not believe there is one. This is the case because this is what current theories on the formation of planetary systems tell us. But there is no reason why life could not exist on satellites of as-yet undetected icy giants in this system—but this moves us from fact to the realm of pure speculation.
  4. Finally, before getting too excited about a speculative and relatively old signal, we should recall the puzzle of fast radio bursts, or so called perytons. Astronomers detected and announced them in 2015, only to later conclude that they were nothing more than the signal from a nearby microwave oven which door was opened by impatient astronomers.

So how will I change my mind you may be wondering? Could we prove that this signal is a civilization which has been trying to communicate with us?

Following the mantra by Carl Sagan “Extraordinary claims require exceptional evidence” I will simply say that this signal should be first detected by another antenna somewhere else in the world. My colleagues at the SETI Institute are already working on it, and observed the star for several hours.

Observing the latest star of interest – HD164595 – with the Allen Telescope Array. https://t.co/CvDTwQFaVT #ATASETI pic.twitter.com/9rCZu5Bfzh

— Jon Richards (@jrseti) August 29, 2016

Then the signal should be analyzed to be certain that it is not coming from a human source. Finally, if the signal is detected repetitively, we can assume if E.T. wants to communicate with us, then the signal should have content. Whatever it could be, the digits of Pi, the first prime numbers, their encyclopedia or some images of themselves, we are quickly capable of finding out if this signal has indeed a meaning.

We are not there yet. It has happened in the past and tumultuous history of SETI that, for a few hours, astronomers thought to have discovered a signal (see “Aliens on Line 1”). As the technology evolves, and more searches are being conducted, we may discover more signals that look promising but at the end don’t pan out. But the search continues… in fact, in the scale the age of our solar system, it has just started.

Clear Skies,

Franck Marchis

Proxima Centauri b: Have we just found Earth’s cousin right on our doorstep?

August 24, 2016

What began as a tantalizing rumor has just become an astonishing fact. Today a group of thirty-one scientists, led by Guillem Anglada-Escude at the Queen Mary University of London, UK, announced the discovery of a terrestrial exoplanet orbiting Proxima Centauri. The discovery of this planet, Proxima Centauri b, is a huge breakthrough not just for astronomers but for all of us. Here’s why.

This artist’s impression shows a view of the surface of the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image to the upper-right of Proxima itself. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface.
Credit: ESO/M. Kornmesser

Astronomers know that exoplanets, or planets in orbit around stars other than our own, are numerous in our galaxy. NASA’s Kepler Space Telescope, which spent four years staring almost continuously at a tiny, distant patch of the sky, proved that there are on average two exoplanets per star in the Milky Way. That’s a lot of worlds! Kepler has also shown that most of our galaxy’s planets are indeed terrestrial—that is, like Earth or even bigger (so-called “super-Earths”). Unfortunately, the exoplanets discovered by Kepler are very distant—too far away for us to observe (and thereby study) using techniques available to most scientists today.

But Kepler is not our only tool for finding exoplanets. We can also use the radial-velocity method, which involves looking for the wobble a planet induces in its host star. This is an effective way to determine the mass of the planet and is not used only for distant stars. In the year 2000, for example, two astronomers announced the discovery of Epsilon Eridani b, a Jupiter-like exoplanet that we now call Aegir, orbiting around Epsilon Eridani, a bright star that’s only 10 light-years away. It was, until today, the closest exoplanet known. Now we now of one that’s far closer.

 

The most popular representation of America. published by Sebastian Münster’s Ptolemy edition of 1540 in Basle (Switzerland)

We also know of 3,374 exoplanets, an enormous large number, given that we discovered the first one only in 1995. Like the cartographers of the seventeenth century, who slowly build a map of our world, astronomers are drawing a map of our galactic neighborhood. We think we have a good handle on the location of nearby stars—that is, ones that are less than 50 light-years away. We know their distance size, temperature, and if they are multiple systems or single stars, for example; but ultimately what we would really like to add to this 3D map of the galaxy are the planets in orbit around these stars.

The Pale Red Dot group was particularly interested in finding planets around Proxima Centauri, the star closest to the Sun. Proxima Centauri is only 4.25 light-years away, so it’s literally in our cosmic backyard. Because of its small mass, it’s too faint to be seen with the naked eye, and was discovered only in 1915. At the end of the 1990s, astronomers tried to detect potential large planets in orbit around this star using the radial-velocity method and came back empty-handed.

In the article published today in Nature, a group of modern astronomers reported on what they learned by using two high-precision radial-velocity instruments: HARPS at the 3.6m telescope of La Silla and UVES at the VLT 8m class telescope, both part of the European Southern Observatory. Several of these observations were done as part of other programs that took place between 2000 and 2016, but from January 2016 to March 2016, the team collected what we call high-cadence data, a fancy way to state that the star was observed once per night to increase its chance of detecting a tiny variation in its motion o (~1 m/s, or the speed of a human walking) that might be caused by the presence of a small planet.

This artist’s impression shows the planet Proxima b orbiting the red dwarf star Proxima Centauri, the closest star to the Solar System. The double star Alpha Centauri AB also appears in the image between the planet and Proxima itself. Proxima b is a little more massive than the Earth and orbits in the habitable zone around Proxima Centauri, where the temperature is suitable for liquid water to exist on its surface.
Credit: ESO/M. Kornmesser

This ambitious program has paid off beyond our wildest dreams in that we have now unambiguously detected a planet with a minimum mass 1.3 times that of Earth orbiting the star right in the middle of the goldilocks zone (0.05 AU). I am not a specialist in RV measurement, but this detection seems quite convincing in that it has a false-alarm probability of less than 0.1% and uses a careful comparison of star activity (done by using additional small telescopes during the survey) that are known to mimic the signal of a planet. That is a very significant new data point to add in our cosmic map.

 Did we find a terrestrial planet?

We don’t know for sure. The planet’s MINIMUM mass is 1.3 x Mearth since we don’t really know the orientation of the orbital plane with respect to the observer (RV provides a measurement of m sin i, with i the inclination of the system with respect to us). Assuming random orientations of orbital planes, we have a 90% probability that the true mass is < 2.3x the minimum mass, so 3x Mearth. In short, this could be a super-Earth or something more exotic, like a baby-Neptune.

Have we found a cousin of Earth?

Not yet. We don’t know the composition of the planet—keep in mind that we haven’t seen it but only its effect on its star. Consequently, we don’t have much information on the planet itself, but we do have a constraint on its mass (see above) and its orbit (one year of Proxima Centauri b is 11.2 days). Since the planet does not transit its star, we don’t know yet its size, hence its density.

 Can life exist on this planet?

The planet is at the right place to have a temperature that allows the presence of liquid water on its surface. The question of habitability is however very complex. We need to confirm that this is a terrestrial planet. The best way to do that would be to directly image the planet using the giant telescopes equipped with extreme adaptive optics that are currently being built (i.e., the E-ELT, TMT, GMT). The angular separation between the star and the planet is 39 milli-arcsec, so a telescope as large as 30 m could resolve the system with the right instrument, detecting the planet and possibly giving us insights into its composition.

 Can life thrive on this planet?

This planetary system is different from ours. Proxima Centauri is a M-type star that is known for sporadic flares, or outbursts of energy. Those luminous UV and X-ray flares could have sterilized the surface of the planet regularly and/or ejected a significant part of its atmosphere into space. The authors briefly discussed the possibility of habitability given the possible present of an extreme environment. I am betting that several follow-up papers on this topic will be published very soon. Astrobiology has taught us that life on Earth is resilient and can be found in extreme environments like deep oceans or protected from UV light in underground caves, so the possibility of a life somewhere in Proxima Centauri b cannot be rejected.

Ultimately, this discovery is a significant step on the road to mapping our galaxy. And it has given us a new world to explore, and one that is not too far away. We may not go there any time soon, but it will motivate us (and our funding agencies!) to design and build instruments to image and characterize this planet. What could possibly be more exciting than, in the not-too-distant future, get a picture of a terrestrial planet whose atmosphere we can see and on which we could possibly detect signatures of life? That monumental moment may come in the next decade, and will definitely happen faster now that we know where to point our telescopes.

Let me close by saying that it is astonishing that we were able to detect this small planet after only three months of observations. The Pale Red Dot group is planning similar campaigns for other nearby stars. In the future, for example, we may know if Alpha Centauri A and B, another nearby system composed of two stars almost identical to the sun, host a true cousin of the planet we call home.

We have no way of knowing where this quest will go, or when, or what it will find. But clearly, this could be the most astonishing journey in the history of humanity.

Clear skies,

Franck M.

Calling for a Better World – Remember to Vote

July 16, 2016
In English

Another attack this month, this time in Nice in the middle of the 14 July celebrations. First, the obvious: this attack, which targeted people and families watching fireworks, was despicable and inhuman. Of course, I send my thoughts to the victims and their families as well as to my colleagues and friends who live in Nice. But I am tired of being an impotent witness to this outbreak of violence everywhere in the world, and I absolutely refuse to remain silent. Like many people, I feel like I’m living a nightmare, in a polarized world in which a tiny minority of violent sociopaths want us to embrace ideas from another time whatever the cost to us, our loved ones, our values, and our dignity as human beings. I hope that this stops and that we find a solution and learn, once and forever more, to live together in peace. But we are living in a very difficult time and we must prepare for many setbacks and tragedies.

The events in Nice also make it imperative that we learn certain key lessons. We, the citizens of free nations going about our daily business, are paying a huge price for wars launched in the first decade of this century by radical and ignorant politicians who manipulated their nations into engaging in a war without end, a war that accomplishes nothing except awakening extremism and hatred in the minds of the weak, the ignorant, and the alienated.This year and next, we can begin to correct this colossal and tragic mistake when we exercise our precious freedom to vote for a government of our own choosing. When we make that choice, we must reject divisive candidates who thrive on the poison of isolationism and xenophobia. Together, we must choose peace, unity and brotherhood. This is what we owe not only to ourselves and our loved ones, but also to the hundreds of victims of these attacks—the men, women, and children; the blacks, Latinos, Asians, and whites; the straight and gay, old and young; the Americans, French, Belgians, Turks and many, many others. They were all human beings whose lives suddenly and tragically ended during a summer evening’s fireworks display, or on the way home from a long trip, or while going to work, or while simply listening to music or enjoying the company of loved ones. Remember them when you vote. Remember them when you hear hatred spewed by radical politicians. Remember above all not to succumb to the easy path of stupidity and violence. We may be weary—but we are always stronger when we act together to fight for human freedom and dignity.

This is what the people of France knew in 1789. This is what the people of the United States knew in 1776. This is what the people of the Soviet Union knew in 1991. And today we must know in—our bones and in our hearts—that this is our only hope for turning tragedy into triumph.

En Francais

Encore un attentat ce mois ci, cette fois à Nice en plein 14 juillet visant des familles qui regardaient un feu d’artifice. Je vais écrire l’évidence, dire combien cette attaque est abjecte et inhumaine, j’envoie bien sûr mes pensées aux victimes et à leur famille ainsi qu’à mes collègues et amis qui vivent à Nice. Je suis néanmoins fatigué d’être le témoin impuissant de ce déchaînement de violence partout dans le monde et je refuse de rester silencieux. Comme beaucoup j’ai l’impression de vivre un cauchemar, dans un monde polarisé dans lequel une petite minorité d’imbéciles  violents veulent à tout prix nous faire accepter leurs idées d’un autre temps quelqu’en soit le prix humain. Je souhaite que ça s’arrête et que nous trouvions une solution pour de nouveau apprendre à vivre ensemble. Cela va être très difficile et il faut se préparer à des déconvenues et des difficultés.

Néanmoins nous devons tirer les leçons de ce qu’il s’est passé. Nous payons les effets secondaires des guerres modernes qui ont été initiées dans les années 2000 par des politiciens radicaux et ignorants qui ont manœuvré les opinions pour se lancer dans une guerre sans fin, une guerre qui ne mène à rien à part éveiller l’extrémisme dans les têtes les plus faibles.

Cette année et l’année prochaine beaucoup d’entre nous irons voter. Nous aurons alors à choisir entre des candidats diviseurs qui déverseront le venin de l’isolationnisme et de la xénophobie. J’espère que tous ensemble nous choisirons la politique de la paix, de rassemblement et de fraternité. Nous leur devons bien ça aux centaines de victimes de ces attentats, aux femmes, enfants, à ces hommes, blacks, latinos, blancs, straight, homosexuels, vieux, jeunes, Français, Américains, Belges, Turques… Ces êtres humains dont la vie s’est arrêtée un soir d’été en regardant un feu d’artifice, en rentrant d’un long voyage, en allant travailler, ou en écoutant de la musique. Pensons à eux lorsque nous irons voter. Pensons à eux lorsque nous écouterons les discours de haine de politiciens radicaux et ne nous laissons pas succomber à la bêtise et la violence. Nous sommes épuisés mais nous sommes toujours plus forts tous ensemble.

C’est ce que nous avons appris en 1789 en France, c’est aussi ce que les habitants des colonies anglaises d’Amériques on comprit en 1776, et plus récemment ceux qui ont brisé les chaines de l’Union Soviétique en 1991.  Aujourd’hui nous devons garder en tête que tous ensembles nous pouvons transformer une tragédie en triomphe.

The Triple Asteroid (87) Sylvia

June 15, 2016

Another beautiful simulation of the triple asteroid system (87) Sylvia and its two moons Romulus and Remus made in collaboration with the California Academy of Sciences.

(87) Sylvia was discovered in 1866 by N.R. Pogson, a British astronomer located in Madras, India. This main-belt asteroid is large with a diameter of ~150 km. That’s all we knew until recently.

In 2005, we discovered two moons around the asteroid that we baptized Romulus and Remus, sons of the Rhea Sylvia and founder of Rome. Both moons are very small with a diameter estimated to ~20 and ~7 km. The primary is irregular with a diameter of 193 x 129 x 124 km. Both moons orbit around the primary describing a coplanar and almost circular orbit.

From a long term study of their orbit we concluded that the primary is possibly differentiated, made of a dense core of ice. How the moons have formed is still unclear. They could be the product of a catastrophic disruption of a large asteroid early in the history of the  solar system.

The triple asteroid (87) Sylvia and its two moons Romulus and Remus from Franck Marchis on Vimeo.

(87) Sylvia is the first triple asteroid ever discovered. I have a fond memory of the day, I presented this discovery at the ACM conference in August 2005 at Buzios, Brazil, simultaneously with the publication in Nature. It was a very special moment in my career.

Today we know six  triple asteroids in the asteroid main-belt (45 Eugenia, 87 Sylvia, 93 Minerva, 130 Elektra, 216 Kleopatra, 3749 Balam)and there are probably more of them waiting to be discovered with the next generation of space-based and ground-based telescopes.

Clear Skies,

Franck M.