Back in the days when Clyde Tombaugh was using a blink comparator to search for 'Planet X,' finding a new object in the outer Solar System was highly unusual. Uranus had been found in 1781, Neptune in 1846, and I suppose I should add Ceres in 1801, although it's a good deal closer than the other two. The real point is that the Solar System seemed straightforward in Clyde Tombaugh's day. There were eight planets and an asteroid belt. It wouldn't be until 1943 that Kenneth Edgeworth argued that the outer system might have 'a very large number of comparatively small bodies,' with Gerard Kuiper publishing his own speculations in 1951. Estonian astronomer Ernst Öpik first described what we now know as the Oort Cloud in 1932, with Jan Oort, a Dutch astronomer, reviving the idea in 1950. The Oort Cloud was a way to explain why comets behave the way they do. Oort believed that there must be a cometary 'reservoir' far away from the Sun -- he chose 20,000 AU as a likely range because of the...
A Relatively Nearby Earth-Sized Planet
Given my abiding interest in red dwarf stars and the planets that circle them, I always keep an eye on what's happening with the MEarth project. Two arrays of robotically controlled telescopes are involved in MEarth (pronounced 'mirth'), one at the Fred Lawrence Whipple Observatory on Mt. Hopkins (AZ), the other a cluster of eight at the Cerro Tololo Inter-American Observatory in Chile. Both these arrays are controlled from MEarth's offices in Cambridge (MA). MEarth is all about observing nearby M-dwarfs in the hunt for Earth-class planets. My fascination in these stars is simply a result of the numbers. We've learned that M-dwarfs comprise as much as 80 percent of the stars in the Milky Way. Earth is not, in other words, orbiting the most common type of star out there. We also know that M-dwarfs host planets. If we learn that conditions on such worlds can support life, then we've dramatically expanded the search space for astrobiology. The prospect of a living world, probably...
Quantifying KIC 8462852 Power Beaming
Plasma physicist James Benford, CEO of Microwave Sciences, is well known here on Centauri Dreams. Today he is joined by his son Dominic, whose work focuses on the development of ultrasensitive technologies for far-infrared through millimeter-wave astronomy. The younger Dr. Benford is Program Scientist for NASA's WFIRST mission, which is designed to conduct major surveys in the near-infrared to answer fundamental questions on the nature of dark energy, the distribution of dark matter, the occurrence of planets around other stars, and even to enable the direct imaging of planetary systems. Previously, Dominic was Chief Scientist for the Cosmic Origins Program Office, as well as Deputy Mission Scientist for WISE, the Wide-field Infrared Survey Explorer. In today's entry, the Benfords look at the SETI Institute's recent observations of KIC 8462852 and analyze the detectability of power beaming at these distances. by James and Dominic Benford The recent report from the SETI Institute of...
Alpha Centauri Planet Reconsidered
Finding a habitable world around any one of the three Alpha Centauri stars would be huge. If the closest of all stellar systems offered a blue and green target with an atmosphere showing biosignatures, interest in finding a way to get there would be intense. Draw in the general public and there is a good chance that funding levels for exoplanet research as well as the myriad issues involving deep space technologies would increase. Alpha Centauri planets are a big deal. The problem is, we have yet to confirm one. Proxima Centauri continues to be under scrutiny, but the best we can do at this point is rule out certain configurations. It appears unlikely, as per the work of Michael Endl (UT-Austin) and Martin Kürster (Max-Planck-Institut für Astronomie), that any planet of Neptune mass or above exists within 1 AU of the star. Moreover, no 'super-Earths' have been detected in orbits with a period of less than 100 days. This doesn't rule out planets around Proxima, but if they are there,...
SETI: No Signal Detected from KIC 8462852
I've mentioned before that I think the name 'Tabby's Star' is a wonderful addition to the catalog. It trips off the tongue so much more easily than the tongue-twisting KIC 8462852, and of course it honors the person who brought this unusual object to our attention, Yale University postdoc Tabetha Boyajian. 1480 light years away, Tabby's Star is an F3 with a difference. It produces light curves showing objects transiting across its face, some of them quite large, and the search is on to find an explanation that fits within the realm of natural causes. Five articles about Tabby's Star have already appeared in these pages, with the most likely explanation being some kind of cometary activity, an answer that seems to satisfy no one. We've also consulted both Boyajian's paper on the subject and a paper by Jason Wright and colleagues out of the Glimpsing Heat from Alien Technologies project at Penn State. The light curves we're looking at do fit the scenario of a 'Dyson swarm,' a cluster...
A 3D Look at GJ 1214b
An old friend used to chide me about the space program, asking good-naturedly enough why it mattered to travel nine years to get to a place like Pluto (this was not long after the New Horizons launch). 'Just another rock,' he would say. 'Why go all that way to look at just another rock?' Although we had many disagreements, Abe was one of the shrewdest people I've ever known. I had met him when he was in his sunset years, but in his prime he had run a large financial operation, been the subject of a story on the front page of the Wall Street Journal and had made a serious fortune in real estate speculation. So what about this 'just another rock' meme? Abe died a few years back but I think about him in relation to things like yesterday's story on Charon. The point is, it's not just another rock. It's this particular rock. And maybe it's not a rock at all; maybe it's a ball of icy slush. And maybe, as we've learned, it's a seriously interesting thing that surpasses expectation. Each...
Unusual Crater on Charon
Another surprise from New Horizons, in a year which will surely see a few more before it ends. After all, we have a long flow of data ahead as the spacecraft continues to return the information it gathered during the July flyby of Pluto/Charon. Now we focus on Charon and the crater being called Organa, which produced an anomaly when scientists studied the highest resolution infrared compositional scan of the moon available. This crater and some of the surrounding materials show infrared absorption at about 2.2 microns, indicating frozen ammonia. Not far away on Charon's Pluto-facing hemisphere is Skywalker crater, which under infrared scrutiny shows the same composition as the rest of Charon's surface. Here water ice -- not ammonia -- dominates. As this JHU/APL news release notes, ammonia absorption was first detected on Charon as far back as 2000, but what we're seeing here is unusually concentrated. In any case, why is Organa so different from Skywalker and the rest of Charon's...
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...
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...
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....
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...
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...
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...
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...
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.
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....
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...
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...
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...
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...