What accounts for Pluto's interesting landscape? As we accumulate more and more data from New Horizons, we're seeing a wide range of geologic activity on the surface, most of it involving such volatile ices as nitrogen, carbon dioxide and methane. But look at the troughs and scarps -- some of them hundreds of kilometers long and several kilometers deep -- and you're seeing what are thought to be extensional faults. These are faults associated with the stretching of the dwarf planet's crust, and in the New Horizons imagery, they appear geologically young. We could look toward tidal interactions with Charon for an answer to what is driving tectonic activity on Pluto, but the Pluto/Charon system has reached what a new paper on the matter calls "the end point of its tidal evolution," with the two objects locked into a synchronous state that makes the prospect unlikely. But changes in the ice shell are another matter, and as Noah Hammond (Brown University) and his fellow researchers are...
Young Exoplanet Highlights Migration Theories
If our Solar System had a ‘hot Jupiter’ that migrated inward after Mars, Earth and Venus had formed, would any of the terrestrial planets have survived? It’s a question worth pondering given how many hot Jupiters we’ve turned up, raising the question of how these planets form in the first place. One possibility is formation in situ, close to the parent star. But there is also an argument for migration, with planets forming in cooler regions further out in the system and migrating inward as a result of interactions with the protoplanetary disk or other planets. Perhaps the planet known as K2-33b can help us with some of this. It is no more than 11 million years old, in an orbit that creates a transit every 5.4 days. With follow-up observations by the MEarth arrays on Mount Hopkins (AZ) and at the Cerro Tololo Inter-American Observatory in Chile, researchers led by Andrew Mann (University of Texas at Austin) have been able to determine that K2-33b is a Neptune-class world some five...
Toward Gravitational Wave Astronomy
The second detection of gravitational waves by the LIGO (Laser Interferometer Gravitational-Wave Observatory) instruments reminds us how much we gain when we move beyond the visible light observations that for so many millennia determined what people thought of the universe. In the electromagnetic spectrum, it took data at long radio wavelengths to show us the leftover radiation from the Big Bang, and we've used radio ever since to study everything from quasars and supernovae to interesting molecules in interstellar space. Infrared helps us penetrate dust clouds and see not only into star-forming areas but the galactic center. So much is learned by taking advantage of the enormous width of the electromagnetic spectrum, wide enough that, as Gregory Benford points out, visible light is a mere one octave on a keyboard fifteen meters wide. Ultraviolet tells us about the gaseous halo around the Milky Way and shows us active galaxies and quasars while helping us analyze interstellar gas...
FU Orionis: Implications of Sudden Brightening for Planet Formation
I would like to thank the many Centauri Dreams readers who contributed to the successful Kickstarter campaign to fund a year's worth of study of KIC 8462852. As I write, there is less than an hour to go, but we have already gone well over the needed $100,000 mark. Congratulations to Tabitha Boyajian, and thanks for all the work she and her colleagues have put into this effort. Now we have a year of observations ahead using the Las Cumbres Observatory Global Telescope Network. The long-term observations will be crucial because we don't know what to expect in terms of sudden dimming in this star's light curve. What a pleasure it is to write for this audience. Readers here have played a large role in pushing this project over the top, and we'll follow the work on KIC 8462852 closely in coming days. Meanwhile, have a look at Penn State's Jason Wright discussing 'Tabby's Star.' [youtube jjh0oK7ZyfM 500 416] Speaking of Unusual Stars… If KIC 8462852 is a star that some believe is...
Stéphane Dumas (1970 – 2016)
The interstellar community is a small one, and reporting the loss of one of our number is not easy. SETI researcher Stéphane Dumas, who had been working with Claudio Maccone on the application of the Karhunen-Loève transform (KLT) for SETI observations, has died unexpectedly at his home in Quebec. I remember a wonderful conversation with Stéphane at one of the 100 Year Starship meetings in Houston, where we got into a spirited exchange about interstellar propulsion. It was, alas, the only time I spent with the man, but he was also active on the advisory board for Jon Lomberg's One Earth Message project, and so we interacted electronically. Below is a video of Stéphane and Claudio Maccone presenting the latest work in mathematical SETI. You'll find Stéphane's talk at about 34:56 on the counter. [youtube djzCAc0pXx8 500 416]
Structure and Composition of a White Dwarf Planet
Given everything we're learning about planets around other suns, it's frustrating that we have so little information about the chemical composition of the rocky planets we've found thus far. Now we have a new study, announced at the San Diego meeting of the American Astronomical Society, that offers data on a 'planet-like body' whose surface layers are being consumed by the white dwarf SDSSJ1043+0855. Although it's been known for some time that the star has been devouring rocky material orbiting around it, the new work offers a striking view of the accretion process and the composition of what was once a differentiated body. At least, that's the best interpretation of the data taken from the Keck Observatory's HIRES spectrometer (installed on the 10-meter Keck I instrument) and the Hubble Space Telescope. White dwarf stars are the remains of stars like the Sun -- this one was once a few times the Sun's mass -- that have gone through their red giant phase and expelled all their outer...
A Long-Period Circumbinary World
Before getting into today's subject, the discovery of an interesting long-period circumbinary planet, I want to make another pitch for Centauri Dreams readers to support the Kickstarter campaign for Tabby's Star. I've written often about this mysterious star whose light curves are anomalous and demand further study. Trying to find out what's happening around KIC 8462852 means acquiring more data, and the Kickstarter campaign would provide an entire year of observations using the Las Cumbres Observatory Global Telescope Network. We're now down to 48 hours and of the $100,000 needed, about three-fourths has been raised. Coming down the homestretch, the remaining $24,000 should be achievable, but it looks to be a dramatic finish. If you haven't been following the KIC 8462852 story, you can check the archives here, or for a quick overview, see my article A Kickstarter Campaign for KIC 8462852. Whatever you can do to help would be hugely appreciated as we try to learn as much as possible...
Asteroids as Spacecraft
Rama is a name that resonates with science fiction fans who remember Arthur C. Clarke's wonderful Rendezvous with Rama (1973). The novel depicts a 50-kilometer starship that enters the Solar System and is intercepted by a human crew, finding remarkable and enigmatic things that I will leave undescribed for the pleasure of those who haven't yet read the book. Suffice it to say that among Clarke's many fine novels, Rendezvous with Rama is, along with The City and the Stars, a personal favorite. What a company called Made in Space Inc. has in mind is something different than Clarke's vision, though it too evokes names from the past, as we'll shortly see. Based in Mountain View, CA the company is embarking on an attempt to turn asteroids into small spacecraft that can move themselves to new trajectories. RAMA in this case stands for Reconstituting Asteroids into Mechanical Automata, and it proceeds by putting 'Seed Craft' on asteroids that will use materials found on the surface. This is...
The Use of Extraterrestrial Resources to Facilitate Space Science and Exploration
We get to the stars one step at a time, or as the ever insightful Lao Tzu put it long ago, ?"You accomplish the great task by a series of small acts." Right now, of course, many of the necessary ‘acts’ seem anything but small, but as Ian Crawford explains below, they’re a necessary part of building up the kind of space economy that will result in a true infrastructure, one that can sustain the exploration of space at the outskirts of our own system and beyond. Dr. Crawford is Professor of Planetary Science and Astrobiology in the Department of Earth and Planetary Sciences, Birkbeck College, University of London. Today he brings us a report on a discussion of these matters at the Royal Astronomical Society earlier this year. By Ian A. Crawford There is increasing interest in the possibility of using the energy and material resources of the solar system to build a space economy, and in recent years a number of private companies have been established with the stated aim of developing...
Hot Jupiters: The Missing Water Vapor
In late 2015, an international team led by David Sing (University of Exeter, UK) studied ten 'hot Jupiters' to try to figure out why some of these planets have less water in their atmospheres than expected from earlier modeling. Sing and company were working with transmission spectroscopy, possible when a planet transits its star and starlight is filtered by the planet's atmosphere. The team used data from the Hubble instrument as well as the Spitzer Space Telescope, covering wavelengths ranging from the optical into the infrared. A cloudy planet appears larger in visible light than in infrared, the difference in radius at the two wavelengths being used to show whether the atmosphere is cloudy or clear. The result, published in Nature, concluded that there was a correlation between hazy and cloudy atmospheres and scant detection of water. In other words, clouds were simply hiding the expected water vapor, and dry hot Jupiters were ruled out. It's an important finding because dry hot...
In Search of Carbon Planets
The first generation of stars in the universe began to shine in an era when chemical elements like carbon and oxygen were not available. It was the explosion of these early stars in supernovae that began the process of enrichment, with heavier elements fused in their cores now spreading into the cosmos. Lower-mass stars and planetary systems began to appear as heavier elements could form the needed dust grains to build planetary cores. Avi Loeb (Harvard-Smithsonian Center for Astrophysics) and grad student Natalie Mashian have been looking at a particular class of ancient stars called carbon-enhanced metal-poor (CEMP) stars. Here the level of iron is about one hundred-thousandth as high as our Sun, a clear marker that these stars formed before heavy elements were widely distributed. These stars are interesting because despite their lack of iron and other heavy elements in comparison to the Sun, they are rich in carbon, an excess that leads to the possibility of planets forming around...
New Insights into Ceres’ Bright Spots
One reason for catching up with recent planetary science here in the Solar System is the upcoming arrival of Juno, which enters into polar orbit around Jupiter on July 4. Juno's arrival is a reminder that the past year has been packed with interesting news from places like Pluto/Charon (New Horizons), Comet 67P/Churyumov-Gerasimenko (Rosetta), and the topic of today's post, the intriguing dwarf planet Ceres, as studied by the orbiting Dawn spacecraft. But the recent Ceres news hasn't just involved Dawn. Paolo Molaro (INAF-Trieste Astronomical Observatory) had led a study looking at the bright spots Dawn found upon approaching Ceres last year. The data Molaro and team drew on came from the European Southern Observatory's 3.6-meter instrument at La Silla and its HARPS spectrograph, which have shown us not only the motion of the bright spots as Ceres rotates but also variations that indicate volatile material within them. The suggestion is that this material evaporates when exposed to...
Looking Back: Pluto’s Twilight Landscape
Friday's look at the possible composition of Pluto's Sputnik Planum took me into a deep enough dive on the two papers -- Pluto gets my full attention! -- that I ran out of time. I had planned to include the images below in that post, but we can do that this morning as a reminder that New Horizons shows no signs of running out of data. What caught my eye here was the possible presence of a cloud, which you can see at the top right of the left image, and in the top inset image. The wispy structure is tens of kilometers across (the entire inset measures about 230 kilometers) and if it is a cloud, it's the only one we've yet picked out of the New Horizons imagery. But if you consider the rest of the image, it would make sense that we could see a cloud here -- notice how the haze layers are brightened by the sunlight that grazes Pluto's surface at a low angle. Also in the top right inset, the southern parts of Sputnik Planum's nitrogen ice fields show up (click the image to enlarge),...
Explaining Sputnik Planum
It's been a week spent catching up with space mission news, focusing on Rosetta, Juno and today, New Horizons. Usually I ponder what I'm going to write each day on Centauri Dreams while I'm having breakfast, a quiet time to reflect on recent events. And if Jay Melosh (Purdue University) is to be believed, I might have taken inspiration from the dish of oatmeal sitting in front of me when it comes to Pluto. Because Melosh and grad student Alex Trowbridge led recent research that may explain what we see at Sputnik Planum. A bit of background before I return to that bowl of oatmeal. We've seen that Sputnik Planum has an unusual appearance, visible in the photo below, that shows patterned polygons. One way of explaining this is to invoke icebergs floating on a sea of nitrogen ice. Melosh and Trowbridge believe the polygons could be what are called Rayleigh-Bénard convection cells, which flag convection that occurs in a fluid that is being heated from below. Says Melosh: "Imagine...
Radio Map of Jupiter Anticipates Juno Findings
Interesting news about Jupiter this morning even as the Juno spacecraft crosses into the realm of Jupiter's gravity. It was six days ago that Juno made the transition into Jupiter space, where the gravitational influence of Jupiter now dominates over all other celestial bodies. And it will be on July 4 of this year that Juno performs a 35-minute burn of its main engine, imparting a 542 meters per second mean change in velocity to the spacecraft for orbital insertion. The spacecraft's 37 flybys will close to within 5000 kilometers of the cloud tops. I only wish Poul Anderson could be alive to see some of the imagery. I always think of him in relation to Jupiter because of his stunning 1957 story "Call Me Joe," describing the exploration of the planet by remote-controlled life forms (available in Anderson's collection The Dark Between the Stars as well as various science fiction anthologies). Image: Launched in 2011, the Juno spacecraft will arrive at Jupiter in 2016 to study the giant...
Cometary Breakup and Reassembly
Yesterday's look at organic compounds on Comet 67P/Churyumov-Gerasimenko needs to be augmented today by a just released study of the comet with implications for how all comets evolve. But first, a renewed pointer to the Kickstarter campaign for KIC 8462852, the unusual star whose light curves continue to baffle astronomers. Please consider contributing to the project, which would raise enough money ($100,000) to support a year of observations. We're about halfway through the campaign but not yet at the halfway point in funds. Have a look at the information provided on the Kickstarter page, or in my essay A Kickstarter Campaign for KIC 8462852, which also has the relevant links. We know the light curves of 'Tabby's Star' are not periodic, so we need continuous monitoring to gain more data on what may be happening there. If we can raise the funds, the Las Cumbres Observatory Global Telescope Network, already supporting the project, can give us the multi-wavelength observations we need....
Rosetta’s Comet: Ingredients for Life
The thought that water and organic molecules might have arrived on the early Earth from the impacts of comets and asteroids has long been provocative, and our missions to nearby comets are now paying off with insights into the possibility. It was back in 2004 that the Stardust mission flew past Comet Wild 2, collecting dust samples that showed traces of the amino acid glycine. Possible contamination of the samples during their analysis left the question open, however. Now we have news that the European Space Agency's Rosetta mission has also found glycine -- a significant organic compound that appears in proteins -- at Comet 67P/Churyumov-Gerasimenko. The spacecraft's ROSINA instrument (Rosetta Orbiter Spectrometer for Ion and Neutral Analysis) detected glycine in October of 2014, with later measurements taken during the August 2015 perihelion event, where cometary outgassing was at its peak. Kathrin Altwegg (University of Bern), who led the study, calls this "...the first...
Kepler-62f: Models for Habitability
So often planets described as ‘potentially habitable’ turn out to be over-rated -- we look deeper into their composition and characteristics only to find that the likelihood of liquid water on the surface is slim. How to make more accurate calls on the matter of habitability? One way may be to combine orbital and atmospheric models, adjusting each with the known parameters of the planet in question. A new study does just that for the interesting world Kepler-62f. About 1200 light years from Earth in the direction of the constellation Lyra, Kepler-62f has a radius 40 percent larger than Earth’s, which puts it well below the 1.6 RE demarcation line that is increasingly thought to define the difference between Earth-like worlds and planets that are more like Neptune. We’re probably looking at a rocky planet here. It’s also a planet that orbits its K-class primary at a distance that could place it in the outer regions of the habitable zone (as defined, again, by the presence of liquid...
Interstellar Flight in Congressional Report
I hadn't planned the conjunction of the Breakthrough Starshot forum's opening here on Centauri Dreams and the interesting news out of the NASA budget for 2017, but some things just fall into your lap. In any case, what happened in Washington makes a nice follow-up to yesterday's post, considering that it calls up visions of fast probes to Alpha Centauri, and in a document coming out of the U.S. House of Representatives, of all things. As more than a few readers have noted, it's not often that we hear interstellar issues discussed in the halls of Congress. Call for a New Interstellar Study The specifics are that space-minded John Culberson (R-TX), who has championed space exploration with abandon, has made sure that NASA will look at the possibilities of interstellar travel. Culberson chairs the House of Representatives sub-panel in charge of NASA appropriations, and the call for interstellar study comes in a report that accompanies the bill establishing the agency's budget for the...
Breakthrough Starshot: ‘Challenges’ Forum Opens
Ever since coming back from the Breakthrough Discuss meeting in Palo Alto, I have been pondering the enormous issues the Breakthrough Starshot project will encounter. Getting a tiny spacecraft up to twenty percent of lightspeed is only the beginning of an effort that has to deal with power generation, a phased laser array of enormous strength and complexity, the miniaturization of critical components, lightsail integrity under thrust and much more. These topics were freely discussed in Palo Alto, and especially at the Yuri's Night party that Yuri Milner threw for the assembled conference goers. When I talked to Milner at the party, he suggested an idea that we have been working on ever since. In order to keep the discussion on the critical issues involving Breakthrough Starshot in front of the interstellar community, why not set up a linkage between the discussion areas of the Breakthrough site and Centauri Dreams? This site would maintain its usual structure and separate comments,...