SETI received a much needed boost this morning as Russian entrepreneur Yuri Milner, along with physicist Stephen Hawking and a panel including Frank Drake, Ann Druyan, Martin Rees and Geoff Marcy announced a $100 million pair of initiatives to reinvigorate the search. The first of these, Breakthrough Listen, dramatically upgrades existing search methods, while Breakthrough Message will fund an international competition to create the kind of messages we might one day send to other stars, although the intention is also to provoke the necessary discussion and debate to decide the question of whether such messages should be sent in the first place. With $100 million to work with, SETI suddenly finds itself newly affluent, with significant access to two of the world's largest telescopes -- the 100-meter Green Bank instrument in West Virginia and the 64-meter Parkes Telescope in New South Wales. The funding will also allow the Automated Planet Finder at Lick Observatory to search at...
Small Interstellar Probes, Riding Laser Beams – The Project Dragonfly Design Competition Workshop
Today we look beyond Pluto/Charon toward possible ways of getting a payload to another star. Centauri Dreams readers are familiar with the pioneering work of Robert Forward in developing concepts for large-scale laser-beamed missions to Alpha Centauri and other destinations. But what if we go smaller, much smaller? Project Dragonfly, in progress at the Initiative for Interstellar Studies, proposes to explore this space, and as Andreas Hein explains below, it was recently examined in a workshop giving student teams a chance to present their ideas. A familiar figure in these pages, Andreas received his master's degree in aerospace engineering from the Technical University of Munich and is now working on a PhD there in the area of space systems engineering, having conducted part of his research at MIT. by Andreas M. Hein The Project Dragonfly Design Competition, organized by the Initiative for Interstellar Studies (i4is) was concluded on the 3rd of July in the rooms of the British...
Unusual Charon Closeup
The latest view of Charon shows us a 390-kilometer strip of Pluto's largest moon with a unique feature, clearly visible below. We are looking at what Jeff Moore (leader of the New Horizons Geology, Geophysics and Imaging team, calls "a large mountain sitting in a moat." Moore is the first to admit that the scenario has geologists stumped. Image: This new image of an area on Pluto's largest moon Charon has a captivating feature -- a depression with a peak in the middle, shown here in the upper left corner of the inset. The image shows an area approximately 390 kilometers from top to bottom, including few visible craters. Credit: NASA-JHUAPL-SwRI. This view of Charon was taken at approximately 0630 EDT (1030 UTC) on July 14, 2015, about 1.5 hours before closest approach to Pluto, at a range of 79,000 kilometers. Again, notice the lack of craters here, reinforcing what we're learning about Charon's relatively young surface. I know we were all curious about Charon from the outset, but I...
First Post-Flyby Pluto Imagery
I'm on the road and don't have a lot of time for writing, but I want to go ahead and get these new Pluto images up. They're now available on the NASA site, and were introduced at the news conference at JHU/APL that just concluded. I'll also quote just a bit of the news release for each photo. New close-up images of a region near Pluto's equator reveal a giant surprise: a range of youthful mountains rising as high as 11,000 feet (3,500 meters) above the surface of the icy body. The mountains likely formed no more than 100 million years ago -- mere youngsters relative to the 4.56-billion-year age of the solar system -- and may still be in the process of building, says Jeff Moore of New Horizons' Geology, Geophysics and Imaging Team (GGI). That suggests the close-up region, which covers less than one percent of Pluto's surface, may still be geologically active today. This one I mis-typed in my Twitter coverage for those who were following it, but the correct number is 100 million years....
Pluto: Encounter and Aftermath
Exoplanet hunter Greg Laughlin (UC-Santa Cruz), who could make a living as a poet (if it were possible to make a living as a poet) wrote recently of his hope for a Pluto image " that will become a touchstone, a visual shorthand for distance, isolation, frigidity and exile." We haven't seen that one yet, but I suspect we will with one of the images we're still to receive showing New Horizons' view of a receding crescent Pluto again being folded into the deep. Last night's reacquisition of the New Horizons' signal sets us up for many weeks of data return, and provides a triumphant exclamation point on the flyby. Our spacecraft punched right through the orbital plane of Pluto's system and emerged unscathed. The joy and festivity apparent on those actually at JHU/APL and the wild and celebratory conversations on social media bring home how popular this diminutive spacecraft has become. What an accomplishment, and even now I'm wondering what advances in technology could do in an outer...
Closest Approach!
Closest approach for New Horizons was at 0749:57 EDT (1149:57 UTC), with closest approach to Charon at about 0806 EDT. Mission operations manager Alice Bowman told the media briefing that we arrived at Pluto 72 seconds early and 70 kilometers closer than the aiming point, all of which was well within mission specs. Nice work. I've found Twitter the best place to keep up, along with NASA TV for the media briefings. The #PlutoFlyby hashtag has been so active that it's sometimes hard to read the messages, a heartening demonstration of the powerful sentiment this mission invokes. I also track @New Horizons2015, @NASANewHorizons, @AlanStern and, of course, @elakdawalla -- Emily Lakdawalla's work has been definitive. The Twitterverse has been exploding. And here is the latest image, showing 4 kilometers per pixel, about 1000 times higher than Hubble can provide. Much better still to come. Here we're sixteen hours from closest approach, at a distance of 766,000 kilometers. Note the varying...
New Horizons Countdown
We're under the 24 hour mark for the Pluto flyby. NASA will offer a news briefing for New Horizons (check NASA TV), covering mission status and what to expect during flyby, at 1030 EDT (1430 UTC) today, a schedule change that moves the time up by half an hour. On Tuesday morning, the agency will present a live program called Arrival at Pluto Countdown starting at 0730 (1130 UTC). Remember that closest approach to Pluto is scheduled to occur at approximately 0749 (1149 UTC) on Tuesday, when the spacecraft comes within 12,500 kilometers of the surface. Gathering data, the spacecraft will be out of communication for much of that day. Image: Pluto as seen from New Horizons on July 11, 2015. Credit: NASA/JHUAPL/SWRI You can check NASA's television coverage and media activities here, but I'll also send you to Emily Lakdawalla's page at The Planetary Society, where the indefatigable reporter has gathered in one place everything known about the schedule and other sources of information....
Charon: A Rugged, Cratered Surface
A chasm in Charon's southern hemisphere turns out to be longer and deeper than Earth's Grand Canyon, says William McKinnon (Washington University, St. Louis), deputy lead scientist with New Horizon's Geology and Geophysics investigation team. "This is the first clear evidence of faulting and surface disruption on Charon. New Horizons has transformed our view of this distant moon from a nearly featureless ball of ice to a world displaying all kinds of geologic activity." Image: Chasms, craters, and a dark north polar region are revealed in this image of Pluto's largest moon Charon taken by New Horizons on July 11, 2015. Credit: NASA/JHUAPL/SWRI. The most prominent crater, near Charon's south pole, is almost 100 kilometers across, and evidently the result of a geologically recent impact. This NASA news release adds that the darkness of the crater floor may be the result of a different kind of icy material being exposed, less reflective than the ices on the surface. Another possibility:...
Last Look at Pluto’s ‘Far Side’
The side of Pluto that always faces its large moon Charon is the side that New Horizons won't see when it makes its close flyby on July 14. That makes the image below what principal investigator Alan Stern is calling "the last, best look that anyone will have of Pluto's far side for decades to come." Image: New Horizons' last look at Pluto's Charon-facing hemisphere reveals intriguing geologic details that are of keen interest to mission scientists. This image, taken early the morning of July 11, 2015, shows newly-resolved linear features above the equatorial region that intersect, suggestive of polygonal shapes. This image was captured when the spacecraft was 2.5 million miles (4 million kilometers) from Pluto. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute. Four dark spots seem to be connected to the dark belt in Pluto's equatorial region, their fairly regular spacing a source of considerable curiosity. The large areas are estimated to...
New Horizons: Detecting Geology
Pluto's surface is beginning to be revealed, with the first signs of geological features, as principal investigator Alan Stern explains: "Among the structures tentatively identified in this new image are what appear to be polygonal features; a complex band of terrain stretching east-northeast across the planet, approximately 1,000 miles long; and a complex region where bright terrains meet the dark terrains of the whale. After nine and a half years in flight, Pluto is well worth the wait." Image: Tantalizing signs of geology on Pluto are revealed in this image from New Horizons taken on July 9, 2015 from 3.3 million miles (5.4 million kilometers) away. At this range, Pluto is beginning to reveal the first signs of discrete geologic features. This image views the side of Pluto that always faces its largest moon, Charon, and includes the so-called "tail" of the dark whale-shaped feature along its equator. (The immense, bright feature shaped like a heart had rotated from view when this...
New Horizons: Flyby Schedule, Images
New Horizons makes its closest approach to Pluto, at approximately 12,500 kilometers above the surface, at 0749 EDT (1149 UTC) on Tuesday July 14. Be aware that for much of that day, we'll be out of communication with the spacecraft while it's busy gathering data. About 2102 EDT (0102 UTC on the 15th), we should receive a confirmation of a successful flyby -- the spacecraft is scheduled to send a preprogrammed signal that it has survived the close approach. Then the data flow begins and will continue for months. NASA offers the schedule for the flyby here, with information on NASA TV coverage. We should be looking at close-up images of Pluto and hearing early reactions from the science team by mid-afternoon of Wednesday the 15th. And of course it will be possible to follow the mission on Facebook or on Twitter (also #PlutoFlyby). The nail-biting time will be the wait on the 14th for the signal announcing a successful transit of the system. It doesn't take a large object to silence a...
Detection of Pebbles in a Circumstellar Disk
Not long ago we looked at a new paper from Alan Boss that modeled interactions in young protoplanetary disks (A Disruptive Pathway for Planet Formation). The idea here is that as dust grains and larger objects bump into each other on the way to forming planetesimals, a mechanism must exist to keep them from spiraling into their star. Boss' models show explosive phases in young stars that lead to gravitational instabilities of the sort needed to scatter these small objects outward and preserve their prospects for forming into planetesimals, and perhaps one day, planets. Watching infant solar systems form is akin to studying embryology in animal species, a chance to understand the myriad interactions that affect growth and set it in particular directions. Now we have work out of the University of St. Andrews, recently presented at the National Astronomy Meeting in Llandudno, Wales, that announces the discovery of a ring of small rocks circling the star DG Tauri, a 2.5 million year old...
The Exploratory Imperative
If you're a long-time reader of this site, you doubtless share my fascination with the missions that are defining our summer -- Dawn at Ceres, Rosetta at comet 67P/Churyumov-Gerasimenko, and in the coming week particularly, New Horizons at Pluto. But have you ever wondered why the fascination is there? Because get beyond the sustaining network of space professionals and enthusiasts and it's relatively routine to find the basic premise questioned. Human curiosity seems unquenchable but it's often under assault. 'Why spend millions on another space rock?' was the most recent question I've received to this effect, but beyond the economics, there's an underlying theme: Why leave one place to go to another, when soon enough you'll just want to go to still another place even more distant? The impulse to explore runs throughout human history, but it's shared at different levels of intensity within the population. I find that intriguing in itself and wonder how it plays out in past events....
End of an Era in Planetary Exploration?
While both Alan Stern and Glen Fountain admitted to having anxious moments over the weekend when New Horizons went silent, it became clear at yesterday's news conference that those moments were short and quickly subsumed with ongoing duties. Stern is principal investigator for New Horizons, and the man most closely identified with making the mission a reality, while Fountain is project manager for New Horizons at JHU/APL in Maryland. It was Stern who pointed out that the spacecraft has been in safe mode a number of times already. Nine times, as a matter of fact, since launch, although as of yesterday we are back in the realm of normal operations. So the circumstances were not unfamiliar even if this safe mode came so close to destination that it raised inevitable concern and a flutter of worry on Twitter. Stern said he was in the control center six or seven minutes after getting the call that something was wrong. It also turns out that this was the first safe mode occurrence in which...
New Horizons: A ‘Timing Flaw’ Scare Resolved
You get to expect the unexpected when writing about space probes, but somehow what New Horizons did to my weekend completely blind-sided me. Running a routine check of email before (I thought) sliding into the rest of a relaxing work break, I found messages about the glitch on the Pluto-bound spacecraft. Sunday turned into an all-screens-on exercise in checking multiple feeds and waiting for news. The problem with New Horizons brought to mind a short story I wrote many years ago about an unmanned probe sent to Epsilon Indi on a 90-year journey. The probe is within a month of encounter when all goes silent and Earth controllers can only wait to see what happens. The point of the story (it was called "Merchant Dying," published in Charlie Ryan's Aboriginal Science Fiction in the July/August 1987 issue) was that spacecraft going to another star are going to need autonomous repair capabilities we can only dream of today. New Horizons is a long way out, but we can still work with it...
The Spacecoach Equation
My view is that the spacecoach, the subject of renewed discussion below by Brian McConnell and a design he and Alex Tolley have created, is the most innovative and downright practical idea for getting crews and large payloads to the planets that I've yet encountered. It's low-cost and uses ordinary consumables as propellant, dramatically revising mission planning. Brian and Alex have continued refining the concept, as explained below in Brian's essay on a modified version of the rocket equation. Have a look and you'll see that planning long duration missions or missions with larger crews becomes a much more workable proposition because more consumables translate into more propellant. Could the spacecoach be our ticket to building a space-based infrastructure, with unmistakable implications for even deeper space? by Brian S McConnell The spacecoach, first introduced here in Spaceward Ho! and A Stagecoach To The Stars and on spacecoach.org, is based on the idea of using consumables...
Thoughts on DE-STAR and Laser Sailing
Last week we looked at DE-STAR (Directed Energy Solar Targeting of Asteroids and Exploration), an ambitious program for developing modular phased arrays of kilowatt class lasers. The work of Philip Lubin (UC-Santa Barbara), DE-STAR is envisioned as a way to scale up a space-based system for asteroid mitigation. And in a new NIAC grant, Lubin will study an off-shoot called Directed Energy Propulsion for Interstellar Exploration (DEEP-IN) as a way of driving tiny 'wafer' probes on interstellar journeys. Reading about these ideas, Jim Benford responded with the comments below. A plasma physicist and president of Microwave Sciences (Lafayette, CA), Dr. Benford's work on microwave beaming to sailcraft has included laboratory experiments at JPL with brother Greg that I've written about in these pages. Here are his thoughts on DE-STAR's beaming methods and the issues they invoke. by James Benford The calculations presented by the DE-STAR group are basically a revisit of the work of Bob...
Methane Detection as New Horizons Closes
As I write, we're thirteen and a half days out from the Pluto/Charon encounter. New Horizons will make its closest approach to Pluto at 0749 EDT (1149 UTC) on July 14. All of which has had me reading Pluto-related science fiction that I missed along the way, including most recently Wilson Tucker's "To the Tombaugh Station." The story, which ran in the July, 1960 issue of Fantasy and Science Fiction, is a murder investigation that includes a journey to the station of the title, which had been established to investigate a 'Planet X' still further out in the system. Isaac Asimov has an essay on Pluto in this issue as well. Image: The cover of the July, 1960 Fantasy and Science Fiction shows a generic moon landing scene by artist Mel Hunter. But if you look at it with our post-1978 (discovery of Charon) eyes, it could be seen as an imaginative take on a Pluto landing, with the Earth on the horizon being replaced by Charon. Given the prominence of "To the Tombaugh Station" on the cover, I...
A Disruptive Pathway for Planet Formation
Planet formation can be tricky business. Consider that our current models for core accretion show dust grains embedded in a protoplanetary disk around a young star. Mixing with rotating gas, the dust undergoes inevitable collisions, gradually bulking up to pebble size, then larger. As the scale increases, we move through to planetesimals, bodies of at least one kilometer in size, which are large enough to attract each other gravitationally. Some planetesimals break apart through subsequent collisions, but a few grow into protoplanets, then planets themselves. It's a reasonable theory that fits what we see around young stars as solar systems take hold. But what Alan Boss (Carnegie Institution for Science) has been working on is a question raised by the process: How do the dust grains and objects smaller than planetesimals keep from being drawn into the protostar before they can become large enough to attract the materials they need to grow? The pressure gradient of the gas in the disk...
A Planet Reborn?
Objects that seem younger than they ought to be attract attention. Take the so-called 'blue stragglers.' Found in open or globular clusters, they're more luminous than the cluster stars around them, defying our expectation that stars that formed at about the same time should develop consistent with their neighbors. Allan Sandage discovered the first blue stragglers back in 1953 while working on the globular cluster M3. Because blue stragglers are more common in the dense core regions of globular clusters, they may be binary stars that have merged, but a number of theories exist, most of them focusing on interactions within a given cluster. Image: The center of globular cluster NGC 6397, in an image taken by the Hubble Space Telescope. Credit: Francesco Ferraro (Bologna Observatory), ESA, NASA. Now we may have found a planet that seems to be younger than it ought to be. Michael Jura (UCLA) and team report on the results in the Astrophysical Journal Letters, making the case that a...