The K2 mission's C16 and C17 observing campaigns -- each containing observations of one patch of the sky for an 80-day period -- have proven fruitful for astronomers at MIT. The institution's Ian Crossfield, working with graduate student Liang Yu, has brought new software tools developed at MIT to work, producing results just weeks after the mission's raw data for these observing runs were made available. Now we have nearly 80 new exoplanet candidates from C16, but we also have a method of fast analysis that should benefit future missions. Let's pause on method. The idea here is to speed up the analysis of light curves, the graphs showing the intensity of light from a star. Between them, C16 and C17 tracked about 50,000 stars, the analysis of whose light would normally take at least several months and perhaps as long as a year. Speed is of the essence because a faster planet identification process makes it possible for quick ground-based radial velocity follow-ups that might...
The Importance of an Eclipsing Charon
The quality of the image below isn't very high, but consider what we're looking at. This is the 'night side' of Pluto's moon Charon as viewed against a star field by the New Horizons spacecraft. We're looking at reflected light from Pluto --'Plutoshine' -- as the sole illumination of most of the surface. Who would have thought, in the 88 years since Clyde Tombaugh's discovery of Pluto, that we would see a Plutonian moon's dark side by Pluto's light? I wonder if there would have been a mission to Pluto at all if it hadn't been for James Christy. Working with astronomer Robert Harrington at the U.S. Naval Observatory Flagstaff Station (Arizona), Christy was situated just miles away from Lowell Observatory, where Pluto was discovered, when he noticed a strange elongation in images of the world. That was forty years ago, on June 22, 1978, during an effort to tighten up estimates of Pluto's orbit around the Sun. I suppose an astronomical analogue to this odd 'blob' on Christy's plates...
On Galactic Migration
Yesterday I looked at the prospect of using technology to move entire stars, spurred on by Avi Loeb's recent paper "Securing Fuel for Our Frigid Cosmic Future." As Loeb recounts, he had written several papers on the accelerated expansion of the universe, known to be happening since 1998, and the resultant 'gloomy cosmic isolation' that it portends for the far future. It was Freeman Dyson who came up with the idea that a future civilization might move widely spaced stars, concentrating them into a small enough volume that they would remain bound by their own gravity. This escape from cosmic expansion has recently been explored by Dan Hooper, who likewise considers moving stellar populations. Image: Harvard's Avi Loeb, whose recent work probes life's survival at cosmological timescales. I gave a nod yesterday to the star-moving ideas of Leonid Shkadov, who suggested a 'Shkadov thruster' that would use the momentum of stellar photons to operate, but Loeb pointed out how inefficient the...
Cosmic Engineering and the Movement of Stars
Avi Loeb’s new foray into the remote future had me thinking of the Soviet physicist Leonid Shkadov, whose 1987 paper “Possibility of Controlling Solar System Motion in the Galaxy” (citation below) discussed how an advanced civilization could get the Sun onto a new trajectory within the galaxy. Why would we want to do this? Shkadov could imagine reasons of planetary defense, a star being moved out of the way of a close encounter with another star, perhaps. All of this may remind science fiction readers of Robert Metzger’s novel CUSP (Ace, 2005), which sees the Sun driven by a massive propulsive jet. A more recent referent is Gregory Benford and Larry Niven’s novels Bowl of Heaven (Tor, 2012) and ShipStar (2014), in which a star is partially enclosed by a Dyson sphere and used to explore the galaxy. In 1973, Stanley Schmidt would imagine Earth itself being moved to M31 as a way of avoiding an explosion in the core of the Milky Way that threatens all life (Sins of the Fathers, first...
On Potentially Habitable Moons
Looking through a recent Astrophysical Journal paper on gas giants in the habitable zone of their stars, I found myself being diverted by the distinction between a conservative habitable zone (CHZ) and a somewhat more optimistic one (OHZ). Let's pause briefly on this, because these are terms that appear frequently enough in the literature to need some attention. The division works like this (and I'll send you to the paper for references on the background work that has developed both concepts): The OHZ in our Solar System is considered to be roughly 0.71 to 1.8 AU, which sees Venus as the inner cutoff (a world evidently barren for at least a billion years) and Mars as the outer edge, given that it appears to have been habitable in the early days of the system, perhaps some 3.8 billion years ago. 'Habitable' in both HZ categories is defined as the region around a star where water can exist in a liquid state on a planet with sufficient atmospheric pressure (James Kasting has a classic...
Marc Millis on Mach Effect Thruster, EmDrive Tests
Marc Millis spent the summer of 2017 at the Technische Universität Dresden, where he taught a class called Introduction to Interstellar Flight and Propulsion Physics, a course he would also teach at Purdue University last November. The former head of NASA's Breakthrough Propulsion Physics project and founding architect of the Tau Zero Foundation, Marc participated in the SpaceDrive project run by Martin Tajmar in Dresden, an effort that has been in the news with its laboratory testing of two controversial propulsion concepts: The Mach Effect Thruster and the EmDrive. Marc's review comments on modeling for the former were almost as long as Tajmar's draft paper. Described below, the SpaceDrive project is a wider effort that includes more than these two areas -- neither the EmD or MET thruster had reached active test phase during the summer he was there -- but the ongoing work on both occupies Millis in the essay that follows. by Marc Millis You may have noticed a renewed burst of...
Enter the ‘Clarke Exobelt’
It's interesting to consider, as Hector Socas-Navarro does in a new paper, the various markers a technological civilization might leave. Searching for biosignatures is one thing -- we're developing the tools to examine the atmospheres of planets around nearby stars for evidence of life -- but how do we go about looking for astronomical evidence of a technological society, one found not by detection of a directed radio or laser beacon but by observation of the stars around us? Various candidates have been suggested, the most famous being the Dyson sphere, in which an advanced civilization might choose to trap the energy output of its entire star, and we're in the era of searches for such objects, as witness the Glimpsing Heat from Alien Technologies effort at Penn State. But there are many other suggestions, ranging from detecting antimatter used for power or propulsion, analyzing Fast Radio Bursts for evidence of manipulation as a propulsion system, and looking at depletion of metals...
On Those Ceres Organics
I set off an interesting conversation with a neighbor when organic material was detected on Ceres, as announced last year by scientists using data from the ongoing Dawn mission. To many people, 'organics' is a word synonymous with 'life,' which isn't the case, and straightening that matter out involved explaining that organics are carbon-based compounds that life can build on. But organic molecules can also emerge from completely non-biological processes. So with that caveat in mind about this word, it's still interesting that organics appear on Ceres, especially since water ice is common there, and we know of water's key role in living systems. A new paper looks again at data from Dawn, whose detections were made with infrared spectroscopy using its Visible and Infrared (VIR) Spectrometer. The instrument, examining which wavelengths are reflected off Ceres' surface and which are absorbed, detected organic molecules in the region dominated by Ernutet Crater on Ceres' northern...
Protoplanets: The Next Detection Frontier
Some 4 million years old, the star HD 163296 is about 330 light years out in the direction of the constellation Sagittarius. When dealing with stars this young, astronomers have had success with data from the Atacama Large Millimeter/submillimeter Array (ALMA), teasing out features in protoplanetary disks filled with gas and dust, the breeding ground of new planets. As seen below, the ALMA imagery can be striking, a closeup look at a stellar system in formation. Image: ALMA image of the protoplanetary disk surrounding the young star HD 163296 as seen in dust. Credit: ALMA (ESO/NAOJ/NRAO); A. Isella; B. Saxton (NRAO/AUI/NSF). Tantalizingly, ALMA can show us rings in such disks, and the gaps that imply an emerging planet. But how do we know we're actually looking at planets, rather than other phenomena we're only now learning how to detect in such disks? New work from Richard Teague (University of Michigan) as well as a second effort by Christophe Pinte and team (Monash University,...
New Horizons from Within
Chasing New Horizons, by Alan Stern and David Grinspoon. Picador (2018), 320 pp. Early on in Alan Stern and David Grinspoon's Chasing New Horizons, a basic tension within the space community reveals itself. It's one that would haunt the prospect of a mission to Pluto throughout its lengthy gestation, repeatedly slowing and sometimes stopping the mission in its tracks. The authors call it a 'basic disconnect' between how NASA makes decisions on exploration and how the public tends to see the result. 'To boldly go where no one has gone before' is an ideal, but it runs up against scientific reality: ...the committees that assess and rank robotic-mission priorities within NASA's limited available funding are not chartered with seeking the coolest missions to find uncharted places. Rather, they want to know exactly what science is going to be done, what specific high-priority scientific questions are going to be answered, and the gritty details of how each possible mission can advance the...
New Horizons: The Beauty of Hibernation
I've always had a great interest in Iceland, stemming from my studies of Old Norse in graduate school, when we homed in on the sagas and immersed ourselves in a language that has changed surprisingly little for a thousand years. There's much modern vocabulary, of course, but the Icelandic of 1000 AD is much closer to the modern variant than Shakespeare's English is to our own. Syntactically and morphologically, Icelandic is a survivor, and a fascinating one. New Horizons' journey to Kuiper Belt Object MU69 occasions this reverie because the mission team has named the object Ultima Thule, following an online campaign seeking input from the public that produced 34,000 suggestions. The word 'thule' seems to derive from Greek, makes it into Latin, and appears in classical documents in association with the most distant northern areas then known. In the medieval era, Ultima Thule is occasionally mentioned in reference to Iceland, and sometimes to Greenland, and may have been applied even...
Lightning in the Jovian Clouds
The longer we can keep a mission going in an exotic place, the better. Sometimes longevity is its own reward, as Curiosity has just reminded us on Mars. After all, it was only because the rover has been in place for six years that it was able to observe what scientists now think are seasonal variations in the methane in Mars' atmosphere. Thus the news that Juno will remain active in Jupiter space is heartening, and in this case necessary. The mission is now to operate until July of 2021, an additional 41 months in orbit having been approved. More time on station allows Juno to complete a primary science mission that had appeared in jeopardy. The reason: Problems with helium valves in the spacecraft's fuel system resulted in the decision to remain in the present 53-day orbit instead of the 14-day 'science orbit' originally planned, and that has extended the time needed for data collection. Thus the lengthening of operations there not only allows further time for discovery but...
Scouting Alpha Centauri at X-ray Wavelengths
One of the benefits of having Alpha Centauri as our closest stellar neighbor is that this system comprises three different kinds of star. We have the familiar Centauri A, a G-class star much like our Sun, along with the smaller Centauri B, a K-class star with about 90 percent of the Sun’s mass. Proxima Centauri gives us an M-dwarf, along with the (so far) only known planet in the system, Proxima b. Questions of habitability here are numerous. Along with possible tidal locking, another major issue is radiation, since M-dwarfs are known for their flare activity. As we learn more about the entire Alpha Centauri system, though, we’re learning that the two primary stars are much more clement. They may have issues of their own -- in particular, although stable orbits can be found around both Centauri A and B, we still don’t know whether planets are likely to have formed there -- but scientists studying data from the Chandra X-ray Observatory have found that levels of X-ray radiation are...
How Old Are Globular Clusters?
Some 150 globular clusters are associated with the Milky Way, great collections of stars inhabiting the galactic halo. Their stars have long been assumed to be ancient, making the question of life there intriguing: If life caught hold in these tightly packed clusters early in the universe’s evolution, could ancient civilizations have formed that might persist even today? I know of only one planet that has yet been found in a globular cluster, but we’re obviously early in the game, and planets have been discovered in open clusters, which are much less densely packed. Just how little we know about globular clusters, though, is made apparent by the work of Elizabeth Stanway (University of Warwick), whose new paper argues that such clusters could be billions of years younger than we have thought. Working with JJ Eldridge (University of Auckland), Stanway invokes a model called Binary Population and Spectral Synthesis (BPASS). In play here is the evolution of binary stars within globular...
A Gravitational Explanation for ‘Detached Objects’
Things always get interesting when the American Astronomical Society meets, which it is now doing in Denver, in sessions that will run until June 7. There should be no shortage of topics emerging from the meeting, but the first that caught my eye was a different approach to the putative world some are calling Planet Nine. Teasing out the existence of a planet at the outer edges of the Solar System has involved looking at gravitational interactions among objects that we do know about, and extrapolating the presence of a far more massive body. But the methodology may be flawed, if new work from Ann-Marie Madigan and colleagues at the University of Colorado Boulder is correct. At a press briefing at the AAS meeting, the team presented its view that objects like Sedna, an outlier that takes more than 11,000 years to complete an orbit around the Sun, should be considered in relation to other so-called 'detached bodies.' Almost 13 billion kilometers out, Sedna is one of a collection of...
Breakthrough Starshot Sail RFP
Breakthrough Starshot held an 'industry day' on Wednesday May 23rd devoted to its lightsail project to take nanocraft to another star, framing the release of a Request for Proposals during its early concepts and analysis phase. The RFP focuses on the sail itself, investigating sail materials and stability under thrust. Step A proposals are due June 22, step B proposals on July 10, with finalists to be notified and contracts awarded this summer. The intent of the RFP is laid out in documents and slides from the meeting that Breakthrough has now placed online. From the RFP itself: The scope of this RFP addresses the Technology Development phase - to explore LightSail concepts, materials, fabrication and measurement methods, with accompanying analysis and simulation that creates advances toward a viable path to a scalable and ultimately deployable LightSail. We've been talking about Breakthrough Starshot in these pages for a long time, as a search through the archives will reveal. The...
Dawn at Ceres: Imagery from a Changing Orbit
I'm looking forward to the buildup as New Horizons gets ever closer to Kuiper Belt Object MU69 and whatever surprises will attend the flyby. But the ongoing operations of the Dawn spacecraft orbiting Ceres equally command the attention. The image below is one of the first images Dawn has returned in more than a year, a stark view of surface features taken on May 16 of this year. The altitude here is 440 kilometers -- for scale, the large crater near the horizon is about 35 kilometers wide. The foreground crater is about 120 kilometers from that crater, within a jumbled landscape suggestive of ancient terrain underlying the more recent impact. Image: On the way to its lowest-ever and final orbit, NASA's Dawn spacecraft is observing Ceres and returning new compositional data (infrared spectra) and images of the dwarf planet's surface, such as this dramatic image of Ceres' limb. Dawn has returned many limb images of Ceres in the course of its mission. These images offer complementary...
Galactic Habitability and Sgr A*
Yesterday I looked at evidence for oxygen in a galaxy so distant that we are seeing it as it was a mere 500 million years after the Big Bang. It’s an intriguing find, because that means there was an even earlier generation of stars that lived and died, seeding the cosmos with elements heavier than hydrogen and helium. It’s hard to imagine the vast tracts of time since populated with stars and, inevitably, planets without speculating on where and when life developed. But as we continue to speculate, we should also look at the factors that could shape emerging life in galaxies like our own. Tying in neatly with yesterday’s post comes a paper from Amedeo Balbi (Università degli Studi di Roma “Tor Vergata”), working with colleague Francesco Tombesi. The authors are interested in questions of habitability not in terms of habitable zones in stellar systems but rather habitable zones in entire galaxies. For we know that at the center of our Milky Way lurks the supermassive black hole Sgr...
Star Formation at ‘Cosmic Dawn’
When life first arose in the universe is a question to which we have no answer. A key problem here is that without knowing how rare -- or common -- life's emergence is, we can't draw conclusions about where (or when) to find it. One thing that is accessible to us, though, is information about when stars began the process of producing the elements beyond hydrogen and helium that are constituents of our own living systems. And on that score, we have interesting news from an international team of scientists about extremely old galaxies. Led by Takuya Hashimoto and Akio Inoue (Osaka Sangyo University), the researchers have gone to work on a galaxy known as MACS1149-JD1, using data acquired from the Atacama Large Millimetre/Submillimetre Array (ALMA) and the European Southern Observatory's Very Large Telescope (VLT). The team's paper in Nature confirms that the galaxy is some 13.28 billion light years away. Thus we see it as it appeared when the universe was about 500 million years old....
Pluto: A Cometary Formation Model
The ongoing work of mining New Horizons' abundant data from the outer system continues at a brisk pace. But missions occur in context, and we also have discoveries made at comet 67P/Churyumov-Gerasimenko by the European Space Agency's Rosetta probe to bring to bear. The question that occupies Christopher Glein and Hunter Waite (both at SwRI) is how to explain the chemistry New Horizons found at Pluto and what it can tell us about Pluto's formation. At the heart of their new paper in Icarus is the question of Pluto's molecular nitrogen (N2), which plays a role on that world similar to methane on Titan, water on Earth and CO2 on Mars. All are volatiles, meaning they can move between gaseous and condensed forms at the temperature of the planet in question. We've learned that solid N2 is the most abundant surface ice visible to spectroscopy on Pluto, as witness the spectacular example of Sputnik Planitia. Image: NASA's New Horizons spacecraft captured this image of Sputnik Planitia...