Gaia spectroscopic view of the asteroid main belt and beyond

2021 ◽  
Author(s):  
Marco Delbo ◽  
Laurent Galluccio ◽  
Francesca De Angeli ◽  
Paolo Tanga ◽  
Alberto Cellino ◽  
...  
Keyword(s):  
Solar System ◽  
Preliminary Investigation ◽  
Planetary Science ◽  
Reflectance Spectra ◽  
Physical Parameters ◽  
The Novel ◽  
Main Belt ◽  
Compositional Gradient ◽  
Solar System Object ◽  
Science Community

<div class="">Asteroids reflectance spectra in the visible light will be one of the novel products of the Gaia Data Release 3 (DR3). These spectra are produced from Gaia observations obtained by means of the blue and red photometers — the so-called BP and RP, respectively. We will review the strategy adopted to produce asteroid reflectance spectra from BP-RP data, focusing on the choice of spectro-photometric calibrations computed taking into account solar system object astrometry and suitable lists of solar-analog stars.</div> <div class=""> </div> <div class="">Our preliminary investigation shows that we will be able to obtain reflectance spectra for asteroids as small as some km in the main belt, by exploiting the fact that each object has been observed multiple times by Gaia. We will show the capability of Gaia to probe the detailed compositional gradient of the main belt down to small sizes and to study correlations between spectral classes and other asteroid physical parameters, such as albedo and size.</div> <div class=""> </div> <div class="">Concerning the brightest asteroids, we expect to have substantial signal at wavelengths shorter than 450 nm, allowing Gaia to examine this region of the spectrum that has been poorly investigated by ground-based asteroid spectroscopic surveys. This region is characterised by the presence of a reflectance downturn that is diagnostic for the composition of classes of primitive asteroids, for instance those including the parent bodies of carbonaceous chondrites. These asteroids may have played an important role for the delivery of prebiotic compounds to Earth during the early phases of solar system' s history and, as such, are at the center of attention of the planetary science community. </div>

NASA Planetary Science and European Partnerships and Participations

2020 ◽  
Author(s):  
Doris Daou ◽  
Lori S. Glaze
Keyword(s):  
Solar System ◽  
Planetary Science ◽  
Solar Neighborhood ◽  
Science Division ◽  
International Partnership ◽  
Cosmic Vision ◽  
Space Agency ◽  
Science Community ◽  
International Participation ◽  
Italian Space Agency

<p>NASA’s Planetary Science Division (PSD) and space agencies around the world are collaborating on an extensive array of missions exploring our Solar System. Planetary science missions are conducted by some of the most sophisticated robots ever built and international collaboration is an essential part of what we do. NASA has always encouraged international participation on our missions both strategic (i.e., Mars 2020) and competitive (i.e., Discovery and New Frontiers) and other Space Agencies have reciprocated and invited us to participate in their missions.</p><p>More specifically, NASA has had a long and fruitful collaboration with ESA on their planetary missions. Currently, NASA is involved in the BepiColombo mission (1 instrument in the Italian Space Agency’s instrument suite), and the Jupiter Icy Moon Explorer mission (one instrument and parts of two others). In concert with ESA’s Mars missions we have an instrument on the Mars Express mission, the orbit-ground communications package on the Trace Gas Orbiter (launched in 2016) and part of the DLR/Mars Organic Molecule Analyzer instruments going onboard the ExoMars Rover. Likewise, NASA’s Mars 2020 rover includes several international payload elements: Spain’s Mars Environmental Dynamics Analyzer (MEDA); Norway’s Radar Imager for Mars' Subsurface Experiment (RIMFAX); and the US SuperCam has a significant contribution from France.</p><p>In 2016, ESA released a call for proposals in their 5<sup>th</sup> Medium-sized mission class (referred to as M5) as part of their Cosmic Vision program. ESA once again has been tremendous in welcoming possible cooperative proposals with NASA as in the EnVision orbital mission to Venus. EnVision would perform high-resolution radar mapping and atmospheric studies of Venus.</p><p>International partnerships are an excellent, proven way of amplifying the scope and sharing the science results of a mission otherwise implemented by an individual space agency. Looking forward, NASA’s Planetary Science Division is initiating the next Decadal Survey, led by the National Academies of Science, Engineering and Mathematics, that will identify priorities for strategic missions in the decade 2023-3032.  There are many exciting destinations within the solar system and these missions will provide new opportunities for international partnership.</p><p>The exploration of the Solar System is uniquely poised to bring planetary scientists, worldwide, together under the common theme of understanding the origin, evolution, and bodies of our solar neighborhood. NASA’s Planetary Science Division provides the planetary science community with opportunities to include international participation on NASA missions. NASA's Discovery and New Frontiers Programs provide U.S. scientists the opportunity to assemble international teams and design exciting, focused planetary science investigations that would deepen the knowledge of our Solar System. The most recent call for Discovery ideas will soon announce selections as part of Step 1 of the competitive process.  NASA continues to encourage the international science community to take full advantage of the many opportunities provided.</p>

scholarly journals Rosuvastatin cocrystals: an attempt to modulate physicochemical parameters

2021 ◽  
Vol 7 (1) ◽  
Author(s):  
Venkata Deepthi Vemuri ◽  
Srinivas Lankalapalli
Keyword(s):  
Physicochemical Properties ◽  
Dissolution Rate ◽  
Functional Groups ◽  
Preliminary Investigation ◽  
Scale Up ◽  
Solvent Evaporation ◽  
Molar Ratio ◽  
The Novel ◽  
Formulation Development ◽  
Hydrogen Bond Interaction

Abstract Background The meager physicochemical properties like low solubility and low dissolution rate of rosuvastatin calcium remain as an obstruction for formulation development. In the present work, we explore the evolution of rosuvastatin cocrystal, which may offer the synergetic physico-chemical properties of the drug. Cocrystal crafting depends on two possible intermolecular interactions; heteromeric and the homomeric selection of compounds with complementary functional groups are contemplated as a possible cause of supramolecular synthons in cocrystal formation. Specifically, cocrystals of rosuvastatin with l-asparagine and l-glutamine with molar ratio (1:1) were fabricated by using slow solvent evaporation and slow evaporation techniques. Novel cocrystals of rosuvastatin-asparagine (RSC-C) and rosuvastatin-glutamine (RSC-G) cocrystals obtained by slow solvent evaporation were utilized for preliminary investigation and further scale-up was done by using the solvent evaporation technique. Results The novel cocrystals showed a new characteristic of powder X-ray diffraction, thermograms of differential scanning calorimetry, 1H liquid FT-NMR spectra, and scanning electron microscopy. These results signify the establishment of intermolecular interaction within the cocrystals. In both the novel cocrystals, rosuvastatin was determined to be engaged in the hydrogen bond interaction with the complementary functional groups of l-asparagine and l-glutamine. Compared with the pure rosuvastatin, RSC-C and RSC-G cocrystal showed 2.17-fold and 1.60-fold improved solubility respectively. The dissolution test showed that the RSC-C and RSC-G cocrystal exhibited 1.97-fold and 1.94-fold higher dissolution rate than the pure rosuvastatin in pH6.8 phosphate buffer respectively. Conclusion Modulation in the chemical environment, improvement in the solubility, and dissolution rate demonstrated the benefit of co-crystallization to improve the physicochemical properties of the drug. Graphical abstract

PLANETARY SCIENCE: How Neptune Pushed the Boundaries of Our Solar System

Science ◽  
2004 ◽  
Vol 306 (5700) ◽  
pp. 1302-1304 ◽  
Author(s):  
A. Morbidelli
Keyword(s):  
Solar System ◽  
Planetary Science

scholarly journals Astrometry of the solar system: the ground-based observations

2007 ◽  
Vol 3 (S248) ◽  
pp. 66-73
Author(s):  
J.-E. Arlot
Keyword(s):  
Solar System ◽  
Space Missions ◽  
Physical Characteristics ◽  
Physical Parameters ◽  
Dynamical Models ◽  
Long Period ◽  
Solar System Objects ◽  
Different Characteristics

AbstractThe main goal of the astrometry of solar system objects is to build dynamical models of their motions to understand their evolution, to determine physical parameters and to build accurate ephemerides for the preparation and the exploitation of space missions. For many objects, the ground-based observations are still very important because radar or observations from space probes are not available. More, the need of observations on a long period of time makes the ground-based observations necessary. The solar system objects have very different characteristics and the increase of the astrometric accuracy will depend on the objects and on their physical characteristics. The purpose of this communication is to show how to get the best astrometric accuracy.

Assembling aliens to explore the Solar System

2021 ◽  
Author(s):  
Catarina Leote ◽  
Sérgio Pereira ◽  
João Retrê ◽  
Pedro Machado ◽  
Gabriella Gilli ◽  
...  
Keyword(s):  
Solar System ◽  
Learning Strategies ◽  
Science Communication ◽  
Planetary Science ◽  
Lessons Learned ◽  
Board Game ◽  
Whole Process ◽  
Informal Educators ◽  
Low Exposure ◽  
Challenging Situation

<p><strong>Assembling aliens to explore the Solar System</strong></p> <p>After analysing the school curricula until 7th grade (13 years old), we concluded that, at least in Portugal, there is a limited coverage of astronomy subjects. This situation is also often accompanied by limited training of primary and medium school teachers and limited availability of resources in their mother tongues, as language can also be a barrier for the use of existing resources. In addition, some astronomy concepts require a level of abstract thinking that might be discouraging for some children. The end result is that some children will have a low interest in astronomy, not only because of their personal preferences but as a consequence of low exposure to the subject or a negative perception towards it. To address this situation, the Science Communication Group of Instituto de Astrofísica e Ciências do Espaço (IA) developed a board game about the Solar System, aimed at children from 6 to 12 years old, and adapted to both formal and informal educational contexts. This project, “Help your Alien – A Solar System Game”, was funded in 2019 by the Europlanet Society through its Public Engagement Funding Scheme.</p> <p><strong>Why a board game?</strong></p> <p>By opting for a board game instead of a digital platform, we made the conscious decision of valuing the power of storytelling and social interaction as engaging and focus-promoting learning strategies, unlike the information and stimuli overload sometimes present in digital environments. Another choice made to make the game as appealing and relatable to our target public as possible was to start with a more familiar perspective, biology, as children of this age group will certainly be familiar with “animals” and their characteristics. We made a leap forward towards astrobiology, and created imaginary aliens somehow adapted to their planets and moons. While trying to assemble these imaginary creatures, in a 3-piece puzzle, the game players have to gather information about different objects of the Solar System and discover the home planet of their assembled aliens.  Another reason for creating a board game was the possibility of reaching different publics, in particular those perhaps not immediately interested in astronomy. With “ET – A Solar System Adventure”, we hope to engage children but also their families (parents, grandparents, siblings…), just for the sake of playing, while exposing them to knowledge about the Solar System.</p> <p><strong>Development of the game</strong></p> <p>The game was developed in a collaborative creative process by members of the Science Communication Group and researchers in Planetary Sciences of the IA, combining knowledge in science communication and different publics with scientific knowledge. Even though the game mechanics was inspired in already existing and well-tested games, the whole process of creating this game involved many challenges, from defining the level of complexity while keeping the game engaging, to the adventure of “creating” aliens somehow physiologically adapted to different planets and moons of the Solar System. Mistakes were made and the team had to adapt to the unexpected challenging situation of a pandemic. This resulted in many lessons learned that we hope to share with the community. The game is now at its final stages of production, with the prototype being converted into a polished version with professional illustration and design. A “Print and Play” version in Portuguese and English will soon be made available online on our website. Physical copies will also be produced depending on funding.</p> <p>In our presentation, we will present our game, as well as the premises and goals behind it, its development process, the challenges found along the way, the lessons learned and some strategies to cope with the “new normality” imposed by Covid-19, while advancing the project. We hope the presentation of “ET – A Solar System Adventure” in the EPSC2021 will help to promote this tool for planetary science education among formal and informal educators and to find international collaborations for the translation and local promotion of the game, as well as additional funding for the production of physical copies in different languages.</p>

Trans-Neptunian Dwarf Planets

2021 ◽  
Author(s):  
Bryan Holler
Keyword(s):  
Solar System ◽  
Surface Composition ◽  
Planetary Science ◽  
Chemical Diversity ◽  
Asteroid Belt ◽  
Dynamical Structure ◽  
Forthcoming Article ◽  
Cold Temperatures ◽  
Dwarf Planets ◽  
Physical And Chemical

This is an advance summary of a forthcoming article in the Oxford Research Encyclopedia of Planetary Science. Please check back later for the full article. The International Astronomical Union (IAU) officially recognizes five objects as dwarf planets: Ceres in the main asteroid belt between Mars and Jupiter; and Pluto, Eris, Haumea, and Makemake in the trans-Neptunian region beyond the orbit of Neptune. However, the definition used by the IAU applies to many other trans-Neptunian objects (TNOs) and can be summarized as any nonsatellite large enough to be rounded by its own gravity. Practically speaking, this means any nonsatellite with a diameter >400 km. In the trans-Neptunian region, there are more than 100 objects that satisfy this definition, based on published results and diameter estimates. The dynamical structure of the trans-Neptunian region records the migration history of the giant planets in the early days of the solar system. The semi-major axes, eccentricities, and orbital inclinations of TNOs across various dynamical classes provide constraints on different aspects of planetary migration. For many TNOs, the orbital parameters are all that is known about them, due to their large distances, small sizes, and low albedos. The TNO dwarf planets are a different story. These objects are large enough to be studied in more detail from ground- and space-based observatories. Imaging observations can be used to detect satellites and measure surface colors, while spectroscopy can be used to constrain surface composition. In this way, TNO dwarf planets not only help provide context for the dynamical evolution of the outer solar system, but also reveal the composition of the primordial solar nebula as well as the physical and chemical processes at work at very cold temperatures. The largest TNO dwarf planets, those officially recognized by the IAU, plus others such as Sedna, Quaoar, and Gonggong, are large enough to support volatile ices on their surfaces in the present day. These ices are able to exist as solids and gases on some TNOs, due to their sizes and surface temperatures (similar to water ice on Earth) and include N2 (nitrogen), CH4 (methane), and CO (carbon monoxide). A global atmosphere composed of these three species has been detected around Pluto, the largest TNO dwarf planet, with the possibility of local atmospheres or global atmospheres at perihelion for Eris and Makemake. The presence of nonvolatile species, such as H2O (water), NH3 (ammonia), and organics provide valuable information on objects that may be too small to retain volatile ices over the age of the solar system. In particular, large quantities of H2O mixed with NH3 points to ancient cryovolcanism caused by internal differentiation of ice from rock. Organic material, formed through radiation processing of surface ices such as CH4, records the radiation histories of these objects as well as providing clues to their primordial surface compositions. The dynamical, physical, and chemical diversity of the >100 TNO dwarf planets are key to understanding the formation of the solar system and subsequent evolution to its current state. Most of our knowledge comes from a small handful of objects, but we are continually expanding our horizons as additional objects are studied in more detail.

Introduction and Preliminary Investigation of Buoyancy Assisted Robots That Are Cheap, Safe, and Will Never Fall Down

2021 ◽  
Author(s):  
Matthew David Williams ◽  
Dennis Hong
Keyword(s):  
Genetic Algorithm ◽  
Preliminary Analysis ◽  
Preliminary Investigation ◽  
Research Work ◽  
Legged Robots ◽  
Dynamical Analysis ◽  
Future Research ◽  
The Novel ◽  
Drag Forces ◽  
New Family

Abstract We introduce and define a new family of mobile robots called BAR (Buoyancy Assisted Robots) that are cheap, safe, and will never fall down. BARs utilize buoyancy from lighter-than-air gases as a way to support the weight of the robot for locomotion. A new BAR robot named BLAIR (Buoyant Legged Actuated Inverted Robot) whose buoyancy is greater than its weight is also presented in this paper. BLAIRs can walk “upside-down” on the ceiling, providing unique advantages that no other robot platforms can. Unlike other legged robots, the mechanics of how BARs walk is fundamentally different. We also perform a preliminary investigation for BARs. This includes comparing safety, cost, and energy consumption with other commercially available robots. Additionally, the preliminary investigation also includes analyzing previous works relating to BARs. A dynamical analysis is performed on the novel robot BLAIR. This is presented to show the impacts of buoyant and drag forces on BLAIRs. Preliminary analysis with the prevalence of drag is presented with simulations using a genetic algorithm and simulations. Results show that BARs with different mechanisms prefer different styles of walking gaits such as prancing or skipping. This work lays the foundation for future research work on the gaits for BARs.

scholarly journals Factoring Origin of Life Hypotheses into the Search for Life in the Solar System and Beyond

Life ◽  
2020 ◽  
Vol 10 (5) ◽  
pp. 52 ◽  
Author(s):  
Alex Longo ◽  
Bruce Damer
Keyword(s):  
Solar System ◽  
Hydrothermal Vents ◽  
Hot Springs ◽  
Planetary Science ◽  
Icy Moons ◽  
Alternative Hypotheses ◽  
Biochemical Mechanisms ◽  
Early Mars ◽  
Life On Earth ◽  
Detection Strategies

Two widely-cited alternative hypotheses propose geological localities and biochemical mechanisms for life’s origins. The first states that chemical energy available in submarine hydrothermal vents supported the formation of organic compounds and initiated primitive metabolic pathways which became incorporated in the earliest cells; the second proposes that protocells self-assembled from exogenous and geothermally-delivered monomers in freshwater hot springs. These alternative hypotheses are relevant to the fossil record of early life on Earth, and can be factored into the search for life elsewhere in the Solar System. This review summarizes the evidence supporting and challenging these hypotheses, and considers their implications for the search for life on various habitable worlds. It will discuss the relative probability that life could have emerged in environments on early Mars, on the icy moons of Jupiter and Saturn, and also the degree to which prebiotic chemistry could have advanced on Titan. These environments will be compared to ancient and modern terrestrial analogs to assess their habitability and biopreservation potential. Origins of life approaches can guide the biosignature detection strategies of the next generation of planetary science missions, which could in turn advance one or both of the leading alternative abiogenesis hypotheses.

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