Mars Adapting

As Clausewitz observed, “In war more than anywhere else, things do not turn out as we expect.” The essence of war is a competitive reciprocal relationship with an adversary. Commanders and institutional leaders must recognize shortfalls and resolve gaps rapidly in the middle of the fog of war. The side that reacts best (and absorbs faster) increases its chances of winning. Mars Adapting examines what makes some military organizations better at this contest than others. It explores the institutional characteristics or attributes at play in learning quickly. Adaptation requires a dynamic process of acquiring knowledge, the utilization of that knowledge to alter a unit’s skills, and the sharing of that learning to other units to integrate and institutionalize better operational practice. Mars Adapting explores the internal institutional factors that promote and enable military adaptation. It employs four cases, drawing upon one from each of the U.S. armed services. Each case was an extensive campaign, with several cycles of action/counteraction. In each case the military institution entered the war with an existing mental model of the war they expected to fight. For example, the U.S. Navy prepared for decades to defeat the Japanese Imperial Navy and had developed carried-based aviation. Other capabilities, particularly the Fleet submarine, were applied as a major adaptation. The author establishes a theory called Organizational Learning Capacity that captures the transition of experience and knowledge from individuals into larger and higher levels of each military service through four major steps. The learning/change cycle is influenced, he argues, by four institutional attributes (leadership, organizational culture, learning mechanisms, and dissemination mechanisms). The dynamic interplay of these institutional enablers shaped their ability to perceive and change appropriately.

As Clausewitz observed, "In war more than anywhere else, things do not turn out as we expect." The essence of war is a competitive reciprocal relationship with an adversary. Commanders and institutional leaders must recognize shortfalls and resolve gaps rapidly in the middle of the fog of war. The side that reacts best (and absorbs faster) increases its chances of winning. Mars Adapting examines what makes some military organizations better at this contest than others. It explores the institutional characteristics or attributes at play in learning quickly. Adaptation requires a dynamic process of acquiring knowledge, the utilization of that knowledge to alter a unit's skills, and the sharing of that learning to other units to integrate and institutionalize better operational practice. Mars Adapting explores the internal institutional factors that promote and enable military adaptation. It employs four cases, drawing upon one from each of the U.S. armed services. Each case was an extensive campaign, with several cycles of action/counteraction. In each case the military institution entered the war with an existing mental model of the war they expected to fight. For example, the U.S. Navy prepared for decades to defeat the Japanese Imperial Navy and had developed carried-based aviation. Other capabilities, particularly the Fleet submarine, were applied as a major adaptation. The author establishes a theory called Organizational Learning Capacity that captures the transition of experience and knowledge from individuals into larger and higher levels of each military service through four major steps. The learning/change cycle is influenced, he argues, by four institutional attributes (leadership, organizational culture, learning mechanisms, and dissemination mechanisms). The dynamic interplay of these institutional enablers shaped their ability to perceive and change appropriately.

The most comprehensive look at our relationship with Mars—yesterday, today, and tomorrow—through history, archival images, pop culture ephemera, and interviews with NASA scientists Mars has been a source of fascination and speculation ever since the ancient Egyptians observed its blood-red hue and named it for their god of war and plague. But it wasn't until the 19th century when “canals” were observed on the surface of the Red Planet, suggesting the presence of water, that scientists, novelists, filmmakers, and entrepreneurs became obsessed with the question of whether there’s life on Mars. Since then, Mars has fully invaded pop culture, inspiring its own day of the week (Tuesday), an iconic Looney Tunes character, and many novels and movies, from Ray Bradbury’s Martian Chronicles to The Martian. It’s this cultural familiarity with the fourth planet that continues to inspire advancements in Mars exploration, from NASA’s launch of the Mars rover Perseverance to Elon Musk’s quest to launch a manned mission to Mars through SpaceX by 2024. Perhaps, one day, we’ll be able to answer the questions our ancestors asked when they looked up at the night sky millennia ago.

The tranquility of Mars is disrupted by humans who want to conquer space, colonize the planet, and escape a doomed Earth.

Rendered in gorgeous, full-color art by Dennis Calero, Ray Bradbury's The Martian Chronicles: The Authorized Adaptation graphically translates fourteen of Bradbury's famous interconnected science-fiction stories, turning an unforgettable vision of man and Mars into an unforgettable work of art. The Earthmen came by the handful, then the hundreds, then the millions. They swept aside the majestic, dying Martian civilization to build their homes, shopping malls, and cities. Mars began as a place of boundless hopes and dreams, a planet to replace an Earth sinking into waste and war. It became a canvas for mankind's follies and darkest desires. Ultimately, the Earthmen who came to conquer the red-gold planet awoke to discover themselves conquered by Mars. Lulled by its ancient enchantments, the Earthmen learned, at terrible cost, to overcome their own humanity.

Nominated as one of America’s best-loved novels by PBS’s The Great American Read Six days ago, astronaut Mark Watney became one of the first people to walk on Mars. Now, he's sure he'll be the first person to die there. After a dust storm nearly kills him and forces his crew to evacuate while thinking him dead, Mark finds himself stranded and completely alone with no way to even signal Earth that he’s alive—and even if he could get word out, his supplies would be gone long before a rescue could arrive. Chances are, though, he won't have time to starve to death. The damaged machinery, unforgiving environment, or plain-old "human error" are much more likely to kill him first. But Mark isn't ready to give up yet. Drawing on his ingenuity, his engineering skills—and a relentless, dogged refusal to quit—he steadfastly confronts one seemingly insurmountable obstacle after the next. Will his resourcefulness be enough to overcome the impossible odds against him?

Seventeen wide-ranging essays explore the evolving scientific understanding of Mars, and the relationship between that understanding and the role of Mars in literature, the arts and popular culture. Essays in the first section examine different approaches to Mars by scientists and writers Jules Verne and J.H. Rosny. Section Two covers the uses of Mars in early Bolshevik literature, Wells, Brackett, Burroughs, Bradbury, Heinlein, Dick and Robinson, among others. The third section looks at Mars as a cultural mirror in science fiction. Essayists include prominent writers (e.g., Kim Stanley Robinson), scientists and literary critics from many nations.

All around you in every moment you are surrounded by the most magical and mystical beings. They are too small, of course, for you to see as single individuals. But in groups you know them as the physical matter of your daily life. They form all of your physical life as you know it. Particles - who might be considered either atoms or portions of atoms - consciously view the vast spectrum of reality, yet also have a sense of personal memory like your own linear memory.These particles remember where they have been and what they have done in their infinitely long lives. Particles, then, have a unique and unusual perspective. In reading this book, understand that some of them will have similar points of view, but others will have quite extraordinary and unexpected points of view. Expect the unexpected!

From Habitability to Life on Mars explores the current state of knowledge and questions on the past habitability of Mars and the role that rapid environmental changes may have played in the ability of prebiotic chemistry to transition to life. It investigates the role that such changes may have played in the preservation of biosignatures in the geological record and what this means for exploration strategies. Throughout the book, the authors show how the investigation of terrestrial analogs to early Martian habitats under various climates and environmental extremes provide critical clues to understand where, what and how to search for biosignatures on Mars. The authors present an introduction to the newest developments and state-of-the-art remote and in situ detection strategies and technologies that are being currently developed to support the upcoming ExoMars and Mars 2020 missions. They show how the current orbital and ground exploration is guiding the selection for future landing sites. Finally, the book concludes by discussing the critical question of the implications and ethics of finding life on Mars. Edited by the lead on a NASA project that searches for habitability and life on Mars leading to the Mars 2020 mission Presents the evidence, questions and answers we have today (including a summary of the current state of knowledge in advance of the ESA ExoMars and NASA Mars 2020 missions) Includes contributions from authors directly involved in past, current and upcoming Mars missions Provides key information as to how Mars rovers, such as ExoMars and Mars 2020, will address the search for life on Mars with their instrumentation

Martian surface contains diverse lithologies (from sedimentary rocks to mafic-ultramafic igneous rocks) and ground patterns. These rocks record the late-stage evolution on the Martian surface from a temperate environment with bodies of liquid water to the current cold and hyper-arid environment. The constraints on the key parameters and processes for water-rock interaction, sedimentation of materials, and geomorphological development can provide important insights into the environmental change and habitability on the Martian surface. However, due to the difficulty in accessing Martian samples and limited remote-sensing data available from the Martian surface, most of the mysteries on Mars remain unraveled. In this proposed research topic we will focus on geological settings on Earth that are similar to the conditions on Mars. These Mars analogs are employed to infer possible processes on Mars and their impact on habitability and the search for life. The Mars analogs on Earth span a variety of environments, such as the super-arid sedimentary plains (e.g., the Qaidam Basin in the north of the Tibetan Plateau, the Mojave Basin in the USA, and the Atacama Desert in South America), the subsurface fracture waters in Precambrian cratons (e.g., the Canadian Shield, the Fennoscandian Shield, and the Kaapvaal Craton), high salinity localities (e.g. Laguna de Tírez, salt mines, and deep-sea brines) as well as extremely cold and highly radiative environments (e.g., polar regions, thin atmosphere). These settings on Earth are more accessible for collecting high-quality mineralogical, geochemical, geochronological, and microbiological data by the state-of-the-art facilities. These data can provide a solid cornerstone for us to understand the cycles of water and other life-essential elements, and their impact on habitability and biodiversity in extreme environments on Earth as well as the limits of life and the detection of biosignatures. Such research can also provide vital insights on the search for life on other planets and moons.