Growing up in the American Midwest, I used to haunt the library in Kirkwood, Missouri looking for books on astronomy. I had it in mind to read all of them and I pretty much did, looking with fascination at fuzzy images of distant objects I yearned to see close up. What did Saturn look like from Titan? What would it be like to be close enough to see the Crab Nebula fill the sky? Breathtakingly, what would it look like to be inside one of the great globular clusters? Early on in Vernor Vinge’s A Fire Upon the Deep the character Ravna finds herself looking out a window at the entire Milky Way from a distance sufficient to view it whole: She’d guessed right: tonight the Galaxy owned the sky… Without enhancement, the light was faint. Twenty thousand light-years is a long, long way. At first there was just a suggestion of mist, and an occasional star. As her eyes adapted, the mist took shape, curving arcs, some places brighter, some dimmer. A minute more and … there were knots in the mist...
Fritz Zwicky On Moving Stars
The great Ukrainian mathematician Israil Moiseyevich Gelfand was famous for his weekly seminars in Moscow, where sudden switches in topics and impromptu presentations were the norm. Although his listeners had heard it many times, Gelfand liked to tell this story: In the early 20th Century, a man approaches a physicist at a party and says he can't understand how the new wireless telegraphy works. How is it possible to send a signal without using wires? The physicist tells him it is simple. "To understand wireless telegraphy, you must first understand how the wired telegraph system works. Imagine a dog with its head in London and its tail in Paris. You yank the tail in Paris and the head in London barks. That is wired telegraphy. Wireless telegraphy is the same thing except without the dog." It always got Gelfand a laugh, but he liked to use the story for a deeper purpose. According to Edward Frenkel, who in his youth attended and presented at some of Gelfand's seminars, Gelfand would...
Building the Bowl of Heaven
Because his new novel Shipstar had just reached the top of my reading stack, and because I had been writing about Shkadov Thrusters last week, I asked Gregory Benford if he could provide a deeper explanation of how these enormous structures might work. Greg had already noted in an email to me that a Shkadov Thruster is inherently unstable, and earlier discussions of the idea on Centauri Dreams had raised doubts about the acceleration possible from such a device. However, I’ve referred to what Benford and Larry Niven have created as a ‘modified’ Shkadov Thruster, and I was anxious to hear their thinking on what might be possible. Greg, an award-winning science fiction author and physicist, here offers his insights into -- and reservations about -- a propulsion scheme capable of moving stars. by Gregory Benford Physicist Leonid Shkadov first described in 1987 a stellar propulsion system made by putting an enormous mirror in a static, fixed position near a star. To stay there it had to...
Stars as Stellar Engines
I've always loved the idea of an O'Neill space habitat because of the possibility of engineering a huge environment to specification. That notion translates well to worldship ideas -- a multi-generational journey would certainly be easier to take in an environment that mimicked, say, a Polynesian island, than aboard something more akin to a giant metal barracks. But best of all is to take your environment with you, which is why the thought of moving entire stars and planets to another location has such appeal when we're talking on an intergalactic scale. Adam Crowl reminded us of the possibilities on Monday: In theory a tight white-dwarf/planet pair can be flung out of the Galactic Core at ~0.05c, which would mean a 2 billion year journey across every 100 million light-years. A white-dwarf habitable zone is good for 8 billion years or so, enough to cross ~400 million light-years. It'd be a 'starship' in truth on the Grandest Scale. Back in November of 1973, Stanley...
Intergalactic Travel via Hypervelocity Stars
We've been looking at not just interstellar but intergalactic crossings in the past few days, something of an homage to Carl Sagan, whose enthusiasm for continuous acceleration at 1 g and relativistic time dilation was immense in the years shortly after Robert Bussard's key paper on interstellar ramjets. Without a working ramjet and largely unaided by time dilation, we're faced with millions of years of flight time to reach M31. What to do? In a recent paper, discussed here by Adam Crowl on Monday, Robin Spivey ponders 'autonomous probes that spawn life upon arrival' as a way of reaching the Virgo cluster, which he wants to do for reasons Adam explained in his post. He's also counting on continuous acceleration at 1 g for these small 'seed ships,' but other than mentioning antimatter, he doesn't explore how this would be done, and we've seen the results Sagan and Iosif S. Shklovskii came up with for antimatter when they worked out the equations. Let's assume that the 'slow boat'...
Sagan’s Andromeda Crossing
When Carl Sagan and Iosif S. Shklovskii discussed travel to another galaxy in Intelligent Life in the Universe (Holden-Day, 1966), they considered the problem from the standpoint of the technologies then under discussion by theorists like Robert Forward and Robert Bussard. As I mentioned yesterday, the authors found hibernation interesting, drawing on the ideas of the Swedish biologist Carl-Göran Hedén, with whom Sagan was then in contact. But it was time dilation that took center stage in their book, and that required stunning velocities. To reach M31, the Andromeda galaxy, in a human lifetime would require a velocity of 0.99999 c. Behind the relativistic spacecraft on Earth, millions of years would have passed, but the same crew that departed would reach their destination. Here is Sagan discussing the matter. And a brief note: Sagan's practice was to interleave his own material with that of Shklovskii, so that while the names of both authors are on the title page, it's easy...
Deep Time: Targeting Another Galaxy
Interstellar flight isn't about possibility as much as it is about time. We know we can launch a payload to another star if we're willing to burn up enough millennia -- about seventy -- to get there in the form of a Voyager-style flyby. That's with today's technology, and we can extrapolate how the time frame can be shortened with improved materials and propulsion techniques. So as Robert Forward always pointed out, it's not that interstellar flight is impossible -- it's that it's very difficult, and our expectations of the kinds of missions possible have to adapt to that fact. Intergalactic flight, though, is such an immense undertaking that I've rarely discussed it in these pages. Is there any conceivable technology that might make such a thing possible? Well, Carl Sagan and Iosif S. Shklovskii considered the situation in Intelligent Life in the Universe (Holden-Day, 1966), working with the opportunity for time dilation opened up by special relativity. Accelerate at 1 g...
A View of the Deepest Future
Adam Crowl first appeared in Centauri Dreams not long after I opened the site to comments about nine years ago. His insights immediately caught my eye and challenged my thinking. I have always admired auto-didacts, and Adam is an outstanding example: "I don't work in this field nor did I especially train in it," he writes. "I did physics/maths/engineering study but my astrophysics, astrodynamics, planetology and interstellar propulsion knowledge is self-taught." The list of books in the various disciplines -- as well as science fiction -- by which he did this will, I hope, become a future Centauri Dreams article. Adam writes the Crowlspace blog, is active in Project Icarus, the re-design of the 1970's Project Daedalus fusion starship now in progress at Icarus Interstellar, and is a frequent participant on this site, often pointing me to papers I would otherwise have missed. The one he discusses today is, typically for Adam, a true mind-bender. by Adam Crowl The long-term fate of Life...
Woven Light: Lesson Arcs
Heath Rezabek continues his experiment in possible futures, science fiction with a collaborative bent exploring the archives that may one day preserve the story of our world and the sometimes mysterious processes that may bring them into being. by Heath Rezabek This is the fifth installment in a continuing series of speculative fiction here on Centauri Dreams. Feedback from prior installments helps shape the themes and direction of subsequent entries, but the purpose and focus of these pieces is to explore a timeline (or timelines) in which comprehensive, resilient archives of Earth's biological, scientific, and cultural record — deep archives for deep time — are developed through unexpected means. Woven Light (I) - Vessel Haven https://centauri-dreams.org/?p=29669 Woven Light (II) - Adamantine https://centauri-dreams.org/?p=29897 Woven Light (III) - Augmented Dreamstate https://centauri-dreams.org/?p=30128 Woven Light (IV) - Proteaa https://centauri-dreams.org/?p=30352...
Outer Planet Exploration Strategies
I'll wrap up this week's outer planet coverage with a look at recent Cassini flybys of Titan, but I also want to put these accomplishments in the context of what we might do with future missions to the ice giants Uranus and Neptune like the proposed ODINUS missions we looked at yesterday. One-off missions to explore a planet and its satellites collect highly detailed data, but comparative studies of the giant planets require accumulating datasets separated by decades. Are there alternatives? Let's hold that thought as we look at Cassini in this light. The flyby designated T-101 occurred on May 17 and was highlighted by Cassini beaming radio signals over Ligeia Mare and Kraken Mare, the two largest seas on Titan. The idea here is to bounce the signals off the surface of the lakes so that they are received by the ground stations of the Deep Space Network here on Earth. Image: Signals bounced off Titan can reveal important details about the moon's surface. Credit: NASA/JPL-Caltech....
Return to the Ice Giants
Once New Horizons has performed its flyby of Pluto/Charon and, let's hope, its reconnaissance of a Kuiper Belt object (KBO), what comes next in our exploration of the outer Solar System? Pushing further out, Innovative Interstellar Explorer grew out of a NASA 'Vision Mission' study and has been developed at Johns Hopkins University Applied Physics Laboratory by Ralph McNutt and team. Boosted by a Jupiter gravity assist, IIE would explore the interstellar medium some 200 AU and further from the Sun, using a plutonium-fueled 1 kW electric radioisotope power supply. And then there's Claudio Maccone's FOCAL mission, which would target the Sun's gravitational focus beginning at 550 AU, continuing well past 1000 AU for observations exploiting gravitational lensing effects. FOCAL has been the subject of intense study -- Maccone's 2009 book Deep Space Flight and Communications grew out of this decades-long work -- and with both IIE and FOCAL we have the prospect of making observations of the...
New Horizons: Hubble Hunts KBOs
My guess is that the public thinks of the Hubble Space Telescope largely in relation to deep space objects. The Hubble Ultra Deep Field is a case in point, a region of the sky in the constellation Fornax that is no more than a tenth of the width of a full moon, but one that contains 10,000 galaxies. An image of the HUDF augmented by near-ultraviolet data has had considerable play in the media, showing star birth in galaxies five to ten billion years ago. It's too lovely not to show here. Image: The Hubble Ultra Deep Field with near-ultraviolet data, a false-color image that is the result of data acquisition from 841 orbits between 2003 and 2012. Credit: NASA/ESA/Caltech/Arizona State. The HUDF attests to Hubble's range, but we also know from Hubble's studies of objects in our own Solar System that it can support ongoing planetary missions. Astronomers will now use the space observatory to help find tiny objects against the background of an immense starfield in Sagittarius. After...
What to Look for at Charon
Let me suggest that you mark August 25th on your calendar. It's the day we celebrate the 25th anniversary of Voyager 2's closest approach to Neptune in 1989. That would be reason enough to look back and remember -- marveling all the while at the Voyagers' continuing mission -- but it's also the day when New Horizons will cross the orbit of Neptune. At work, as principal investigator Alan Stern points out in his latest PI's Perspective, is 'cosmic coincidence not design,' but what a moment it will be as New Horizons moves at last into 'Pluto space.' 90 percent of the long journey is over, with a bit more than 300 million miles to go before the encounter with Pluto/Charon next summer. Newly awakened from hibernation, the spacecraft will be put through a complete checkout of its onboard systems and scientific instruments, as well as conducting its first optical navigation campaign to study the approach into Pluto. Stern also reports that the upcoming cruise science will include imaging...
Transcendence Going Interstellar: How the Singularity Might Revolutionize Interstellar Travel
Andreas Hein, who has appeared in these pages before on the subject of worldships, here speculates about a much different kind of traveling: The uploading of consciousness. Andreas is Deputy Director of the Initiative for Interstellar Studies (I4IS), as well as Director of its Technical Research Committee. He founded and leads Icarus Interstellar's Project Hyperion: A design study on manned interstellar flight. 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. He spent a semester abroad at the Institut Superieur de l'Aeronautique et de l'Espace in Toulouse, working on the numerical simulation of the hypervelocity impact of space dust on spacecraft antennas, and also worked at the European Space Agency Strategy and Architecture Office on stakeholder analysis for future manned space exploration. Today's essay is...
The Worldship of 1953
Les Shepherd's 1952 paper "Interstellar Flight" appears in the Journal of the British Interplanetary Society," a fitting place given Shepherd's active involvement in the organization. He would, in fact, serve the BIS as its chairman, first succeeding Arthur C. Clarke in that role in 1954, and returning in 1957 and again in 1965 for later terms of office. "Interstellar Flight" is one of those papers that turns people in new directions after they have read it, and we can see the gradual acceptance of travel between the stars as a possibility that does not violate the laws of physics beginning in its pages. Much less heralded but more widely seen was an adapted version of "Interstellar Flight" that appeared in Science Fiction Plus in April of 1953. The magazine was a revival of Hugo Gernsback's career as a science fiction publisher that ran for seven issues before its demise in December of the same year. Gernsback's name was revered in science fiction circles as the founder of Amazing...
Cultural Evolution: The View from Deep Space
I didn't have the chance to meet Mark Lupisella at the first 100 Year Starship symposium in Orlando, but the publication of Cosmos & Culture: Cultural Evolution in a Cosmic Context in 2013 made me wish I had sought him out. Co-edited with Steven J. Dick (about whom there are so many interesting things to say that I'll have to carry over into a future post with them), Cosmos & Culture offers essays from scientists, historians and anthropologists about the evolution of culture both on Earth and, most likely, beyond it. These are, of course, issues we've been considering recently in the work of Cameron Smith and Kathleen Toerpe, and in a broader sense they inform many of the SETI and astrobiology discussions we have here. Then Clément Vidal, who is an author and a post-doctoral researcher at the Free University of Brussels, passed along the paper I missed in Orlando, Lupisella's "Cosmocultural Evolution: Cosmic Motivations for Interstellar Travel." To be fair to myself, we all...
Putting the ‘Giggle Factor’ to Rest
Can we overcome our preconceptions about extraterrestrial life? Kathleen Toerpe thinks the answer is yes, for we're moving from the era of ill-informed jokes about 'little green men' to a widening appreciation of our place in the cosmos. Dr. Toerpe is the Deputy CEO for Programs and Special Projects at the Astrosociology Research Institute and editor of The Journal of Astrosociology. She also serves as a NASA/JPL Solar System Ambassador, one whose educational efforts on behalf of space exploration have revealed that the younger generation is familiar with and inspired by the subject, a fact that gives this essay its welcome patina of optimism. The recent hearings on SETI in the U.S. House of Representatives show that, for some at least, old attitudes die hard, but ongoing research into astrobiology and SETI is likely to make the 'giggle factor' seem positively prehistoric within our lifetimes. by Kathleen D. Toerpe, PhD Flip through any newsfeed these days, and it seems that humanity...
Kepler-56: Misaligned Planets Around a Swelling Star
Although I'm sure I'll refer to various papers presented at the American Astronomical Society this week in future entries, I'll close our current look at the Boston meeting with word of two planets that will be falling into their star in short order (at least as astronomers measure time). Kepler-56b and Kepler-56c have a predicted era of death, some 130 million and 155 million years from now respectively. I can't think of any other exoplanets about which we've been able to make such statements, making this a system worth watching as we ponder our own Sun's future. Just as the Sun will one day enlarge to red giant status, threatening the inner planets, so Kepler-56 is growing, already reaching four times the size of the Sun. The star has a long way to go as it continues its outward expansion, and the two planets in question are in a perilous position, with Kepler-56b orbiting the host star every 10.5 days, and Kepler-56c every 21.4. Gongjie Li (Harvard-Smithsonian Center for...
Three Regimes of Planet Formation
On Tuesday I mentioned the work of Lars A. Buchhave, an astronomer at the Harvard-Smithsonian Center for Astrophysics (CfA), in connection with the Kepler-10c discovery. The latter is the so-called ‘mega-Earth’ now found to be seventeen times as massive as our own planet, with a diameter of about 29,000 kilometers. A larger population of solid planets with masses above 10 times that of Earth was suggested in the Kepler-10c paper (see Introducing the ‘Mega-Earth’ for more on this), with reference to Buchhave’s ongoing work. Let’s take a closer look at what Buchhave is doing, because the intriguing fact is that planets four times the size of Earth and smaller comprise about three-quarters of the planets found by the Kepler mission. How large a role does the metallicity of the host star play in planet formation? At the ongoing meeting of the American Astronomical Society in Boston, Buchhave explained his research methods, which involve measuring ‘metals’ -- in astronomical parlance the...
Probing an Ancient Planetary System
The red dwarf known as Kapteyn's Star -- the name comes from the 19th Century Dutch astronomer Jacobus Kapteyn -- is about thirteen light years from Earth in the southern constellation of Pictor, close enough that a small telescope can pick it out. Kapteyn's efforts at cataloguing the star in 1898 revealed that it had the highest proper motion of any star then known, a position it lost with the discovery of Barnard's Star in 1916. Because I find stellar encounters interesting, I'll note that about 11,000 years ago, Kapteyn's Star would have come within seven light years of the Sun. It has been moving away from us ever since. Kapteyn's Star belongs to the galactic halo, a dispersed population of stars on elliptical orbits that wraps around the galactic disk and bulge. It is the nearest known halo star to the Sun. We now know, through the efforts of an international research team, that at least two planets are found here. Kapteyn c is a 'super-Earth' with an orbit of 121 days, while...