Exoplanetology Beyond Kepler

Useful synergies continue to emerge among our instruments as we ponder the future of exoplanet studies. Consider the European Space Agency’s PLATO mission (PLAnetary Transits and Oscillations of stars). Operating from the L2 Lagrangian point, PLATO will use 34 telescopes and cameras on a field of view that includes a million stars, using transit photometry, as Kepler did, to find planetary signatures. Working at optical wavelengths, PLATO will look for nearby Earth-sized and ‘super-Earth’ planets in the habitable zone of their stars. This mission is scheduled to be launched in 2024, an interesting date because it’s also the year that the European Extremely Large Telescope (E-ELT) is scheduled to see first light. Huge new installations like these, although ground-based, are so powerful that they should be able, with the help of adaptive optics, to study planetary atmospheres on the PLATO-discovered planets. Thus we get the best of both worlds, with repairable and upgradable ground...

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Voyager Update: Probing the Boundary

I always feel that my day starts right when a story involving the Voyagers crosses my desk. The scope, the sheer audacity of these missions in their day cheers me up, and the fact that they are still communicating with us is a continual cause for celebration. With Voyager 1 now moving beyond the heliosphere, we've got an interstellar craft on our hands, one that's telling us a good deal about the perturbed regions through which it moves. Every day that the Voyagers stay alive is a triumph for an inquisitive and exploring species, and one day we'll be launching their successor, targeting the local interstellar medium with instruments designed for the task. Image: This artist's concept shows NASA's Voyager spacecraft against a backdrop of stars. Credit: NASA/JPL-Caltech. The heliosphere is that 'bubble' blown by the particles of the Sun's solar wind in surrounding interstellar space. As such, it's a moving and malleable thing, flexing, flowing, contracting here, expanding there...

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Science Fiction and the Symposium

Science fiction is much on my mind this morning, having just been to a second viewing of The Martian (this time in 3D, which I didn't much care for), and having just read a new paper on wormholes that suggests a bizarre form of communication using them. More about both of these in a moment, but the third reason for the SF-slant is where I'll start. The 100 Year Starship organization's fourth annual symposium is now going on in Santa Clara (CA), among whose events is the awarding of the first Canopus Awards for Interstellar Writing. A team of science fiction writers will anchor what the organization is calling Science Fiction Stories Night on Halloween Eve. Among the writers there, I'm familiar with the work of Pat Murphy, whose novel The Falling Woman (Tor, 1986) caught my eye soon after publication. I remember reading this tale of an archaeological dig in Central America and the 'ghosts' it evokes with fascination, although it's been long enough back that I don't recall the details....

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Where We Might Sample Europa’s Ocean

No one interested in the prospects for life on other worlds should take his or her eyes off Europa for long. We know that its icy surface is geologically active, and that beneath it is a global ocean. While water ice is prominent on the surface, the terrain is also marked by materials produced by impacts or by irradiation. Keep in mind the presence of Io, which ejects material like ionized sulfur and oxygen that, having been swept up in Jupiter’s magnetosphere, eventually reaches Europa. Irradiation can break molecular bonds to produce sulfur dioxide, oxygen and sulfuric acid. And we're learning that local materials can be revealed by geology. A case in point is a new paper that looks at infrared data obtained with the adaptive optics system at the Keck Observatory. The work of Mike Brown, Kevin Hand and Patrick Fischer (all at Caltech, where Fischer is a graduate student), suggests that the best place to look for compounds indicative of life would be in the jumbled areas of Europa...

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Catching Up with the Outer System

We now pivot from Dysonian SETI to the ongoing exploration of our own system, where lately there have been few dull moments. Today the Cassini Saturn orbiter will make its deepest dive ever into the plume of ice, water vapor and organic molecules streaming out of four major fractures (the 'Tiger Stripes') at Enceladus' south polar region. The plume is thought to come from the ocean beneath the moon's surface ice, and while Cassini is not able to detect life, it is able to study molecular hydrogen levels and more massive molecules including organics. Understanding the hydrothermal activity taking place on Enceladus helps us explore the possible habitability of the ocean for simple forms of life. Image: This artist's rendering showing a cutaway view into the interior of Saturn's moon Enceladus. NASA's Cassini spacecraft discovered the moon has a global ocean and likely hydrothermal activity. A plume of ice particles, water vapor and organic molecules sprays from fractures in the moon's...

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Why SETI Keeps Looking

How do you feel about a universe that shows no signs of intelligent life? Let’s suppose that we pursue various forms of SETI for the next century or two and at the end of that time, find no evidence whatsoever for extraterrestrial civilizations. Would scientists of that era be disappointed or simply perplexed? Would they, for that matter, keep on looking? I suspect the latter is the case, not because extraterrestrial civilizations would demonstrate that we’re not alone, but because in matters of great scientific interest, it’s the truth we’re after, not just the results we want to see. In my view, learning that there was no other civilization within our galaxy -- at least, not one we can detect -- would be a profoundly interesting result. It might imply that life itself is rare, or even more to the point, that any civilizations that do arise are short-lived. This is that tricky term in the Drake equation that refers to the lifespan of a technological civilization, and if that...

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KIC 8462852: Enter ‘Gravity Darkening’

Back from my break, I have to explain to those who asked about what exotic destination I was headed for that I didn’t actually go anywhere (the South Pacific will have to wait). The break was from writing Centauri Dreams posts in order to concentrate on some other pressing matters that I had neglected for too long. Happily, I managed to get most of these taken care of, all the while keeping an eye on interstellar news and especially the interesting case of KIC 8462852 (for those just joining us, start with KIC 8462852: Cometary Origin of an Unusual Light Curve? and track the story through the next two entries). Whatever the explanation for what can only be described as a bizarre light curve from this star, KIC 8462852 is a significant object. While Dysonian SETI has been percolating along, ably studied by projects like Glimpsing Heat from Alien Technologies, the public has continued to see SETI largely in terms of radio and deliberate attempts to communicate. Tabetha Boyajian and...

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No Posts Until 26 October

As mentioned in Friday's post, I'm taking a week off. The next regular Centauri Dreams post will be on Monday the 26th. In the interim, I'll check in daily for comment moderation. When I get back, we'll be starting off with a closer at Jason Wright's recent paper out of the Glimpsing Heat from Alien Technologies project at Penn State, with a focus on interesting transiting lightcurve signatures and how to distinguish SETI candidates from natural phenomena.

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KIC 8462852: The SETI Factor

I had no idea when the week began that I would be ending it with a third consecutive post on Dysonian SETI, but the recent paper on KIC 8462852 by Tabetha Boyajian and colleagues has forced the issue. My original plan for today was to focus in on Cassini’s work at Enceladus, not only because of the high quality of the imagery but the fact that we’re nearing the end of Cassini’s great run investigating Saturn’s icy moons. Then last night I received Jason Wright’s new paper (thanks Brian McConnell!) and there was more to say about KIC 8462852. Actually, I’m going to look at Wright’s paper in stages. It was late enough last night that I began reading it that I don’t want to rush a paper that covers a broad discussion of megastructures around other stars and how their particular orbits and properties would make them stand out from exoplanets. But the material in the paper on KIC 8462852 certainly follows up our discussion of the last two days, so I’ll focus on that alone this morning....

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What’s Next for Unusual KIC 8462852?

I want to revisit the paper on KIC 8462852 briefly this morning, as I’m increasingly fascinated with the astrophysics we’re digging into here. The fact that the star, some 1480 light years away, is also a candidate for further SETI investigation makes it all the more intriguing, but all my defaults lean toward natural processes, if highly interesting ones. Let’s think some more about what we could be looking at and why the ‘cometary’ hypothesis seems strongest. Remember that we’re looking at KIC 8462852 not only because the Kepler instrument took the relevant data, but because the Kepler team took advantage of crowdsourcing to create Planet Hunters, where interested parties could sign up to study the light curves of distant stars on their home computers. KIC 8462852 has been causing ripples since 2011 because while we do seem to be seeing something passing between its light and us, that something is not a planet but a large number of objects in motion around the star. Some of the...

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KIC 8462852: Cometary Origin of an Unusual Light Curve?

Dysonian SETI operates under the assumption that our search for extraterrestrial civilizations should not stop with radio waves and laser communications. A sufficiently advanced civilization might be visible to us without ever intending to establish a dialogue, observed through its activities around its parent star or within its galaxy. Find an anomalous object difficult to explain through conventional causes and you have a candidate for much closer examination. Is KIC 8462852 such a star? Writing for The Atlantic, Ross Andersen took a look at the possibilities yesterday (see The Most Mysterious Star in Our Galaxy), noting that this F3-class star puts out a light curve indicating not a planetary transit or two, but a disk of debris. That wouldn't be cause for particular interest, as we've found numerous debris disks around young stars, but by at least one standard KIC 8462852 doesn't appear to be young. In a paper on this work, Tabetha Boyajian, a Yale University postdoc, and...

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A Mission to Jupiter’s Trojans

Back in 2011, a four planet system called Kepler-223 made a bit of a splash. Researchers led by Jack Lissauer (NASA Ames) at first believed they were looking at two planets that shared the same orbit around their star, each circling the primary in 9.8 days. These co-orbital planets were believed to be in resonance with the other two planets in the system. If the finding were confirmed, it would indicate that one planet had found a stable orbit in a Lagrange point -- the L4 and L5 Lagrange points lie 60° ahead and behind an orbiting body. We call an object sharing an orbit like this a trojan, as shown in the figure below, which depicts the best known trojans in our system, the asteroids associated with Jupiter. Image: Jupiter's extensive trojan asteroids, divided into 'Trojans' and 'Greeks' in a nod to Homer, but all trojans nonetheless. Credit: "InnerSolarSystem-en" by Mdf at English Wikipedia - Transferred from en.wikipedia to Commons. Licensed under Public Domain via...

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Pluto’s Circumbinary Moons

Kepler-47 is an eclipsing binary some 4900 light years from Earth in the direction of the constellation Cygnus. It's a system containing two transiting circumbinary planets, meaning the planets orbit around the binary pair rather than around one or the other star. That configuration caught the eye of Simon Porter, a postdoc at the Southwest Research Institute, because the configuration is so similar to another circumbinary system, the one involving four small moons around Pluto/Charon. In both cases, we have a binary at the center of the orbit. Porter writes about the configuration in this post from the New Horizons team. In the case of Pluto, the binary could be considered a binary planet, with Charon the other half of the duo. Both are orbited by a system of four moons, each of them less than 50 kilometers in diameter, the moons orbiting around the system's center of mass. New Horizons, the gift that keeps on giving, has already sent some striking images of these small moons, but...

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SETI: A Networked Galaxy?

We often conceive of SETI scenarios in which Earth scientists pick up a beacon-like signal from another star, obviously intended to arouse our attention and provide information. But numerous other possibilities exist. Might we, for example, pick up signs of another civilization's activities, perhaps through intercepting electromagnetic traffic, or their equivalent of planetary radars? Even more interesting, as Brian McConnell speculates below, is the idea of listening in on a galactic network that contains information not just from one civilization but many. As Centauri Dreams readers know, McConnell and Alex Tolley have been developing the 'spacecoach' concept of interplanetary travel, discussed in the just published A Design for a Reusable Water-Based Spacecraft Known as the Spacecoach (Springer, 2015). It's a shrewd and workable way to get us deep into the Solar System. Today McConnell turns his attention to a SETI network whose detection could offer a big payoff for a young...

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A Comparative Look at Solar Systems

With almost 2000 exoplanets now confirmed, not to mention candidates in the thousands, it's amazing to recall that it was just twenty years ago that the first planet orbiting a main sequence star beyond the Solar System was found. Continued work on the world revealed that 51 Pegasi b is about half as massive as Jupiter, though 50 percent larger. Orbiting its star in roughly four days, the planet is some fifty light years from Earth. Thus we began to learn not just that exoplanets were out there, but that their environments could be truly extreme -- remember that it was just in 1992 that planets were found around the pulsar PSR 1257+12. Without any evidence other than my imagination, I grew up believing that most stars should have planets, and just assumed that their stellar systems were more or less like our own. There should be a few planets too close to their star for life to exist, and several gas giants out at the outskirts of the system, and somewhere in between there should be...

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AU Mic: Intriguing Features in a Protoplanetary Disk

The European Southern Observatory's SPHERE instrument is turning up interesting things around the star AU Microscopii. Surrounded by a large dusty disk, the star is young enough to raise the interest of those studying how planets form. What has turned up are structures that Anthony Boccaletti (Observatoire de Paris) describes as 'arch-like, or wave-like,' a structure that his research team has never seen before. The issue is addressed in a new paper in Nature, which discusses five wave-like arches at different distances from the star. Fortunately, AU Mic is a well studied star, with abundant Hubble imagery taken in 2010 and 2011 available for comparison. The results of that comparison are striking: The features do indeed show up on the Hubble imagery, but they show distinct change with time, meaning they are in rapid motion. "We reprocessed images from the Hubble data and ended up with enough information to track the movement of these strange features over a four-year period,"...

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Habitability Index Ranks Exoplanets

If we had a space-based instrument fully capable of analyzing an exoplanet's atmosphere in place right now, where would we find our best targets? The goal, of course, is to pluck out the signature of biological activity, which means we're looking at planets in the habitable zone of their stars, that region where liquid water can exist on the surface. Right now there aren't many planets that fit the bill, but the day is coming when there will be hundreds, then thousands. How we optimize our search time and choose the targets with the most likely pay-off is a major issue. Which is where a new metric called the 'habitability index for transiting planets' comes into play. Developed by Rory Barnes and Victoria Meadows (University of Washington), working with research assistant Nicole Evans, the index is an attempt to prioritize the selection process, looking at those exoplanets that should be at the top of our list. Says Barnes: "Basically, we've devised a way to take all the...

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Unusual Orbits for Unusual Missions

Our choice of orbits can create scientifically useful space missions that can be operated at lower cost than their more conventional counterparts. How this has been done and the kind of missions it could enable in the future is the subject of James Jason Wentworth's essay. An amateur astronomer and interstellar travel enthusiast, Wentworth worked at the Miami Space Transit Planetarium and volunteered at the Weintraub Observatory atop the adjacent Miami Museum of Science. Now making his home in Fairbanks (AK), he was the historian for the Poker Flat Research Range sounding rocket launch facility. His space history and advocacy articles have appeared in Quest: The History of Spaceflight magazine and Space News. by J. Jason Wentworth In the 1990s, then NASA Administrator Daniel S. Goldin introduced the "Better, Faster, Cheaper" paradigm for space missions. While NASA's subsequent experiences led many engineers to modify that to "Better, Faster, Cheaper--choose two," the goal of low cost...

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Woven Light: The Orphan Obscura

Heath Rezabek began exploring Vessel, an evolving strategy for preserving Earth's cultures and biology, in these pages back in 2013. A librarian and writer in Austin TX, Heath went on to push these ideas into the realm of science fiction, in the form of a series of excerpts from a longer work that is still emerging. The concluding post in this sequence appears below, though you'll be hearing more about 'Woven Light.' A novel is emerging from this haunting look at how, at various points in our future and with a wide range of technologies, we will interact with the artifacts and stored experience of our past. Heath's helpful synopsis begins the post. by Heath Rezabek For some time, I have had in hand the final chapter – for now – of the Woven Light speculative fiction series as published on Centauri Dreams from 2013 to present. At Paul’s invitation, I am prefacing the final installment with some notes on the series as a whole. The series began as a way to explore ideas surrounding the...

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An Asteroid Deflection Investigation

Yesterday's post on what we're learning about Rosetta's comet (67P/Churyumov-Gerasimenko) briefly touched on the issue of changing the orbit of such bodies for use in resource extraction. Moving the comet Grigg-Skjellerup is part of the plot of Neal Stephenson's novel Seveneves, where the idea is to support a growing human population in space with the comet's huge reserves of water. Just how hard it would be to move a comet is made clear by how a proposed near-term mission approaches the question of deflecting a small asteroid. The mission, discussed at the ongoing European Planetary Science Congress in Nantes, is called AIDA, for Asteroid Impact and Deflection Assessment. A joint mission being developed by the European Space Agency and NASA, AIDA is actually a two-pronged affair. ESA is leading the Asteroid Impact Mission (AIM), while NASA is behind the Double Asteroid Redirection Test (DART). The plan is to rendezvous with the asteroid (65803) Didymos and its tiny satellite (known...

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Charter

In Centauri Dreams, Paul Gilster looks at peer-reviewed research on deep space exploration, with an eye toward interstellar possibilities. For many years this site coordinated its efforts with the Tau Zero Foundation. It now serves as an independent forum for deep space news and ideas. In the logo above, the leftmost star is Alpha Centauri, a triple system closer than any other star, and a primary target for early interstellar probes. To its right is Beta Centauri (not a part of the Alpha Centauri system), with Beta, Gamma, Delta and Epsilon Crucis, stars in the Southern Cross, visible at the far right (image courtesy of Marco Lorenzi).

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If you'd like to submit a comment for possible publication on Centauri Dreams, I will be glad to consider it. The primary criterion is that comments contribute meaningfully to the debate. Among other criteria for selection: Comments must be on topic, directly related to the post in question, must use appropriate language, and must not be abusive to others. Civility counts. In addition, a valid email address is required for a comment to be considered. Centauri Dreams is emphatically not a soapbox for political or religious views submitted by individuals or organizations. A long form of the policy can be viewed on the Administrative page. The short form is this: If your comment is not on topic and respectful to others, I'm probably not going to run it.

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