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This blog collects supplemental data on lesser worlds of the solar system (like Pluto and Titan) that have not (yet) been included in our books. You may contribute to our blog with brief articles that we will on your request also translate for our monolingual audience. The only precondition: Your content must in some way relate to dwarf planets or large moons of the solar system.

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Freitag, 19. Januar 2018

NEW: Enceladus - Iceland of Space

Among the moons of the ringed planet, Saturn, little Enceladus was the primary target of the Cassini space probe other than huge Titan. And for good reason: Apart from Jupiter’s moon Europa, Enceladus is these days considered the most promising target in the quest for extraterrestrial life in the solar system. In this respect, the moons and dwarf planets of the outer solar system have left long-favoured planet Mars behind by now.
  Only the last ten years have made evident to us that cold worlds need not be frozen to the core and inanimate. Traces of past or even present activities like earthquakes, geysers, eruptions, snowfalls or even tidal surges can be found on locations from the innermost dwarf planet Ceres to its big brother Pluto far away behind the orbits of the large Jovian giants.
  NASA has made it a habit to claim ‘oceans’ in the netherworlds of icy bodies in and beyond the planetoid belt wherever it looks. It may sound encouraging at press conferences because it makes many an audience think of fish, jellyfish and coral. On Enceladus, alleged ‘geysers’ even spray water vapour into the sky, evoking mental images of the Yellowstone National Park, of Iceland or just of Andernach in Germany. Textbook articles, on the other hand, often refer more reservedly to those briny waters inside lesser worlds of the solar system as ‘liquid mantles’.
  Both approaches are justifiable, depending on whether you prefer to think in terms associated with water, like a biologist does, or rather like a physicist or volcanologist who prefers to emphasise the analogy of dynamic processes developing on Earth and elsewhere.
  We use the latter approach in this book. That way, dynamic phenomena on Enceladus can be described more succinctly, elaborating on the similarities with planets like Earth. For like our homeworld, this minor body is divided into a solid shell, a liquid mantle and, again, a solid core. The geysers, as we will see, closest resemble fissure vents of Iceland hurling molten lava up in long curtains of fire. It seems justified to call Enceladus the Iceland of Space: an Iceland of ice, water and vapour.
  Ice plays the role of basalt there, water assumes the role of magma. Volcanologists like to use terms such as cryovolcanism, cryomagma and cryolava to emphasise the differences in chemistry, while the physics stay the same.
  Given all the media attention Enceladus has received as the Cassini-Huygens spacecraft crisscrossed Saturn’s system from 2005 to 2017, we find it surprising that no book publisher has so far taken on this fascinatingly exotic world that looks like the backdrop of an imaginative sci-fi film.
  In view of the continuing success of our previous books on lesser worlds of the solar system: ‘Pluto & Charon’, ‘Titan - Pluto’s big brother’ and ‘Ceres - Pluto’s little sister’, we have therefore decided to close this gap in the German- and English-speaking markets. Readers who would like to penetrate deeper into the subject are encouraged to read forthcoming ‘Enceladus and the Icy Moons of Saturn’ (ISBN: 0816537070) scheduled to be published in the USA in June 2018 and aiming at the professional audience. Regarding our own series we would like to draw special attention to the ‘Titan’ volume, because it deals with elements of the Cassini-Huygens mission alluded to but not specified in this book.

Print or eBook: Enceladus - Iceland of Space
Sample chaptersEnceladus - Iceland of Space

Freitag, 15. Dezember 2017

NEU: Enceladus - Island des Weltraums

Wer noch ein Weihnachtsgeschenk für einen Hobbyastronomen sucht: Das 4. Buch aus unserer Serie ist heute online gegangen. Am kommenden Montag und Dienstag könnt ihr die Kindle-Version sogar gratis herunterladen. Die großformatige 4-Farb-Druckausgabe wird voraussichtlich im Lauf des Wochenendes bestellbar.

Klappentext:
"Den Voyager-Sonden erschien Enceladus wie ein frischer glatter Schneeball.

Erst die Cassini bemerkte, wie außergewöhnlich dieser kleine Saturnmond ist, dessen Klüfte Geysire in den Himmel spucken, als sei er das Island des Weltraums.

Inzwischen ist die Cassini in den Saturn gestürzt worden, doch was sie beobachtete, ist noch lange nicht verstanden. Woher kommt die Wärme, von der die Geysire des Enceladus ihre Energie beziehen? Woher die organischen Substanzen darin? Kann es in seinem Innern sogar Leben geben?

In diesem Buch werden die außergewöhnlichen Beobachtungen der Cassini erstmals gesammelt vorgestellt."

Mittwoch, 19. April 2017

New release: "Ceres: Pluto's little sister"

When at New Year’s eve of 1801 - the first night of the new century - Guiseppe Piazzi watched through his telescope and saw a tiny point of light that no star map had registered, he could hardly gave anticipated how, by this discovery, he revolutionised our understanding of the structure of our solar system.
Up to then, only the sun, seven planets (the planet Uranus had been discovered by F. W. Herschel as late as 1781), their moons and a few comets had been known. When Ceres was discovered, it was first considered a comet, then it was classified as a planet. It was supposed that Ceres was that very world that had been predicted by astronomers for long to fill the gap between Mars and Jupiter. Within a short time, Pallas, Juno and Vesta were also discovered, that orbit in the same gap between Mars and Jupiter. Thus our planetary system grew to 11 planets. 38 years went by, however, until Astraea was found in 1845 (also between Mars and Jupiter), followed by Neptune in the year after. Now we reckoned even 13 planets.
When in 1847, the first detection of Hebe initiated a deluge of new discoveries, the true nature of these objects between Mars and Jupiter was finally acknowledged, and scientists coined the terms asteroids, planetoids or minor planets for them, took them out of the list of planets and numbered them by order of discovery, beginning with (1) Ceres. Now there were only eight major planets left, including Uranus and Neptune, while the number of minor planets steadily grew. When Clyde Tombaugh discovered Pluto in the vastness beyond Neptune in 1930, it was listed as a ninth planet.
Only sixty years after, in the nineties of the last century, evidence was found that the asteroid belt between Mars and Jupiter was paired with another belt of minor solar system bodies beyond Neptune, now called the Kuiper Belt. The objects there consist mainly of ice, mixed with silicates and organic compounds. Some of them are wider than 1000 km, meaning they are larger than Ceres. And only then it became obvious that Pluto is nothing else than another of these bodies, now called TNOs (Trans-Neptunian Objects) or KBOs (Kuiper Belt Objects).
In summer 2006, the International Astronomical Union, or IAU, during its general assembly in Prague decided for a new definition of the term planet. Since then, a planet of the sun has to meet two criteria: 1.) It must be in hydrostatic equilibrium on account of its gravity, i. e. be spherical. 2.) It must be the dominating object in its sphere of influence and have its orbit cleared of other objects.
Though Pluto is perfectly spherical, as the images of the New Horizons space probe have impressively shown us, it fails on the other criterion, because it shares its orbit, intersecting that of Neptune, with about a third of the newly discovered TNOs. Therefore Pluto was no more a planet. Not to degrade it too lowly, however, a new category was designed for it: the dwarf planets. Though they must fulfil the first criterion, to be spherical, they may share similar orbits with a variety of objects. Within the scope of this new definition, spherical Ceres, reckoned as a minor planet for 150 years, has suddenly become a dwarf planet.
Ceres is the largest body is in the asteroid belt between Mars and Jupiter. With a diameter of 1000 km, it is about twice as wide as the next largest asteroids, Pallas and Vesta. About one third of the total mass of the asteroid belt is included in the mass of Ceres.
Once it had been believed that the asteroids were fragments of a larger planet that had orbited between Mars and Jupiter and burst in a cosmic disaster. This hypothetical planet, however, could not have been very big: If you could assemble all the minor bodies of the asteroid belt on Ceres, its diameter would grow only by about half its current size. The asteroid belt simply does not contain enough material to provide for a larger planet. Its total mass amounts only to about half a thousandth that of Earth or about 4 % of the mass of our Moon. In the early stage of the solar system, the gravity of the rapidly growing proto-Jupiter had sucked too much material away from this area so that no proper planet could have developed there. Ceres is only a protoplanet that had not been given a chance to accrete into a true planet.
To understand these processes better, that is why the Dawn mission had been launched. (The name was chosen as a reference to the dawn of the solar system because the mission was intended to provide us insight into the origin of planets.) The camera on board of Dawn has been built in Germany, by the same team that had been in charge of the camera on the comet probe Rosetta. It is a masterpiece of German engineering that should make us proud and the product of long-standing experience with cameras on probes like Giotto or Mars Express. This should be underlined in an era of receding space budgets and fading interest in natural sciences. The camera has not only produced marvellous images of Ceres but, in the end, even saved the continuation of the Dawn mission because, when the US administration had stopped the Dawn project because it was surpassing the budgetary limit, it was just this international cooperation that yet kept the project alive.
Join a fascinating trip to Ceres in this book by Andreas Möhn and Metka Klemenčič with its impressive images: to a body that has not fully managed to become a true planet and has been caught in the protoplanetary stage yet given us thereby important knowledge about the dawn of our solar system and the origin of our own planet.
Dr Rainer Riemann
Heidelberg, in March 2017

The English translation is online and available for a sample read:
https://www.academia.edu/32503897/Leseprobe_Ceres_GB.pdf
The complete printed book is available here: https://www.amazon.com/dp/1545462933/ref=sr_1_1…

Donnerstag, 22. September 2016

Für alle, die die fehlerhafte Kindle-Version heruntergeladen haben

Hinweis:

Alle Leser, die die fehlerhaft formatierte Kindle-Version von Amazon heruntergeladen haben, erhalten am Samstag, dem 22.09., die Gelegenheit, ihre Datei kostenlos auszutauschen. Auch alle anderen dürfen an diesem Tag noch einmal zugreifen, bevor "Pluto & Charon" bei KDP Select endgültig aussteigt: https://www.amazon.de/Pluto-Charon-Horizons-fernsten-Weltenweiten/dp/1534633529


Am 1. Oktober wird das e-Book dann endlich auch für ePub-Reader zugänglich gemacht!


Und hier noch ein aktueller Beitrag zu unserem liebsten Zwergplaneten:

"Aus Daten der Raumsonde "New Horizons" weiß man, dass der Zwergplanet Pluto eine herzförmige Region auf seiner Oberfläche besitzt. Darin befindet sich ein Gletscher aus gefrorenem Stickstoff mit Kohlenstoffmonoxid und Methan.
Die Wissenschaftler haben nun die atmosphärischen Bedingungen auf dem Zwergplaneten simuliert, um die Entstehung dieses Gletschers zu erklären. Im Magazin "Nature" berichten sie, dass eine vier Kilometer tiefe und 1000 Kilometer weite Senke für das Eis verantwortlich sei. In dieser Region sei die Atmosphäre Plutos am dichtesten, was wiederum günstige Bedingungen für das Eis schaffe.
Aus der Simulation ging außerdem hervor, dass das Eis auf der Nordhalbkugel Plutos in den nächsten zehn Jahren schmelzen werde. Sollte das tatsächlich eintreten, wäre das eine Bestätigen der Simulationsergebnisse, heißt es von den Forschern."
(http://www.deutschlandfunk.de/meldungen-liste-forschung-aktuell.1508.de.html?drn:date=2016-09-20&drn:news_id=658298)

Äh ... von Schmelzen steht in dem Nature-Artikel aber nichts, lieber Deutschlandfunk. Da heißt es nur, der Eispanzer würde sich periodisch ausdehnen und zusammenziehen.

Donnerstag, 15. September 2016

"Pluto & Charon" - now for the last time for free!


For the last time before it will drop out of KDP Select, we offer the English kindle-version of "Pluto & Charon" for free. You may download the latest eBook file on either Friday, 16 or Saturday, 17, from here: https://www.amazon.com/Pluto-Charon-Horizons-spacecraft-farthest/dp/1534960740 and see for yourself what the printed edition would look like if you had it lying on your desk.
The eBook edition will be made available for ePub-readers as well on 1 October, 2016.



"In this book its two authors have managed to present the intriguing results of New Horizons’ Pluto flyby in a mode that non-professionals will understand, without waiving appropriate scientific accuracy."
(Dr. R. Riemann, astrophysicist, University of Heidelberg, Germany)

 #Pluto #Newhorizons #Solarsystem #NASA

Donnerstag, 28. Juli 2016

Nullpreisaktion: Die deutsche eBuch-Ausgabe nur dieses Wochenende kostenlos!

Nach der englischen zieht die deutsche eBuch-Ausgabe von "Pluto & Charon" nach: Am kommenden Wochenende, dem 30. und 31. Juli 2016, ist die kindle-Version unseres Bildbandes zur Raumsondenmission New Horizons vorübergehend kostenlos abrufbar. Verschaffen Sie sich einen Eindruck, wie der Band aussehen würde, wenn Sie ihn auf Papier vor sich hätten. ;-)

Bei dieser Gelegenheit möchte ich auch auf den Vortrag zu Pluto und seinen Monden hinweisen, der am Montag, dem 10.10.2016, um 20:00 Uhr bei der Astronomischen Gesellschaft Urania in der Volkssternwarte auf der Martin-Niemöller-Schule am Moltkering, Wiesbaden, stattfinden wird. Hier werden Sie auch die Gelegenheit erhalten, mehr über die neuesten Auswertungen des immer noch andauernden Datenflusses zwischen der Raumsonde New Horizons und der Erde zu erfahren, die erst nach Redaktionsschluss des vorliegenden Buches publiziert wurden. Ein Live-Videomitschnitt des vorausgegangenen Vortrags am 16. März 2016 ist hier abrufbar: 



Da nach einer ePub-Ausgabe gefragt wurde: Die wird es auch geben, allerdings erst ab Oktober 2016, wenn die Exklusivrechte beim Programm KDP-Select abgelaufen sind.