Search results for "MARS"

showing 10 items of 384 documents

Allometries of maximum growth rate versus body mass at maximum growth indicate that non-avian dinosaurs had growth rates typical of fast growing ecto…

2014

We tested if growth rates of recent taxa are unequivocally separated between endotherms and ectotherms, and compared these to dinosaurian growth rates. We therefore performed linear regression analyses on the log-transformed maximum growth rate against log-transformed body mass at maximum growth for extant altricial birds, precocial birds, eutherians, marsupials, reptiles, fishes and dinosaurs. Regression models of precocial birds (and fishes) strongly differed from Case's study (1978), which is often used to compare dinosaurian growth rates to those of extant vertebrates. For all taxonomic groups, the slope of 0.75 expected from the Metabolic Theory of Ecology was statistically supported. …

Anatomy and PhysiologyMetabolic theory of ecologyVertebrate Paleontologylcsh:MedicineBiostatisticsBody Mass IndexDinosaursBirdsbiology.animalAnimalsGrowth rateStatistical Methodslcsh:ScienceBiologyEvolutionary BiologyMultidisciplinarybiologyEcologyEcologyFossilsApplied Mathematicslcsh:RStatisticsFishesVertebrateReptilesPaleontologyThermoregulationBiological EvolutionAltricialTaxonMarsupialiaEctothermEarth Scienceslcsh:QPrecocialPaleobiologyPhysiological ProcessesEnergy MetabolismMathematicsResearch ArticleDevelopmental BiologyPloS one
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Zvaigžņotā Debess: 2009, Rudens (205)

2009

Contents: I.Daube. Jānis Ikaunieks ; A.Balklavs. Mountains on the Venus ; TASS and “Pravda” materials. Soviet Automatic Stations “Venera-5” and “Venera-6” Reach Venus ; A.Alksnis. Gathering of Astronomers at the University ; A.Alksnis, M.Ābele, I.Eglītis, B.Rjabovs, K.Salmiņš, I.Pundure. Directions of Scientific Research of the UL Institute of Astronomy Assessed ; D.Docenko. Meteorite Fallen in Sudan Recovered ; A.Alksnis. How Asteroids Will Disturb Observation with Extremely Large Telescopes ; M.Gills. Daily in Network with Astronomy ; I.Pundure. Arturs Balklavs and Astronomy of Latvia (continued) ; M.Sudārs. IXV – Step towards Reusable Space Vehicles ; V.Kalniņš. Hyperdrive and Heim’s Qua…

Asteroīdi un novērošana ar lielajiem teleskopiemAlfrēds Štrauss – dzīvesstāsta meklējumiAndromedas galaktika M31Vienošanās starp Latvijas valdību un Eiropas Kosmosa aģentūruMeteorīts Almahatta SittaArturs Balklavs “Latvijas astronomija pēc Trešās atmodas”IXV – Eiropas daudzkārt izmantojams kosmosa kuģisLatvijas atklātā matemātikas olimpiādeRainis – kosmosa dzejnieksJānis IkaunieksAstronomu salidojums UniversitātēSiltumnīcas uz MarsaAstronomiskās parādības - 2009Latvijas astronomija - vēstureStarptautiskais Astronomijas gads 2009 – plakātsAstronomijas institūts - zinātniskā pētniecībaJaunākie žurnāli “Zvaigžņotās Debess” bibliotēkāEduards Riekstiņš – 90LU fizikas docents Ludvigs Jansons – 100Hiperdzinējs – Heima kvantu teorijaAgreement between the Government of the Republic of Latvia and the European Space AgencyAstronomija - tīmeklīRīgas Politehnikuma Astronomijas kabinets – 130Latvijas atklātā skolēnu astronomijas olimpiāde
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Zvaigžņotā Debess: 2009/10, Ziema (206)

2009

Contents: TASS and Soviet Press materials. Flight of the Group of Three Soviet Spaceships ; Soviet and Foreign Press materials. Second Expedition on the Moon ; Č.Šklennik. Excursion to an Ancient Laboratory ; M.Gills. Opening Address ; Conference “Astronomy in Latvia” Programme ; From Presentation Abstracts ; I.Pundure. First Enterprise of this Kind ; N.Cimahoviča. Astronomical Contribution to Culture ; A.Alksnis. First Findings of Space Mission CoRoT ; I.Pundure. Ten Years of Chandra Hot Universe Exploration ; M.Gills. The Beginning of Autumn with Astronomy ; Buying Stars and Star Names (translation from IAU) ; I.Pundure. Arturs Balklavs and Astronomy of Latvia (1990-1997) ; J.Jaunbergs. A…

Astronomija kultūrāNesējraķetes Ares I izstrādeArturs Balklavs “Latvijas astronomija pēc Trešās atmodas”Krustvārdu mīklaLU fizikas docents Ludvigs JansonsCoRoT misijas pirmie rezultātiKosmiskā ēra pastmarkāsKonference “Astronomija Latvijā”Astronomiskās parādības - 2009Latvijas astronomija - vēstureLatvijas atklātā fizikas olimpiādeStarptautiskais Astronomijas gads 2009 - pasākumiTeodoram Grothusam – 225Latvijas matemātikas olimpiāde – uzdevumu atrisinājumiAstronomijas seminārs „Ērgļa tau”LZA Fizikas un tehnisko zinātņu nodaļas sēdes „Starptautiskais Astronomijas gads” lēmuma projektsRentgenstaru observatorijas Chandra desmitgadeLatvijas Pasta Eiropas sērijaMarsa meteorītiAstronomiskās parādības - 2010Zvaigžņu un to nosaukumu pirkšanaRosetta’s trešā pietuvošanās ZemeiAstronomija Zinātņu akadēmijas sēdēs 2009.gadāPilnais Saules aptumsums - novērojumi - 2009. gada 22. jūlijs Ķīna
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Report of the COSPAR Mars special regions colloquium

2010

International audience; In this paper we present the findings of a COSPAR Mars Special Regions Colloquium held in Rome in 2007. We review and discuss the definition of Mars Special Regions, the physical parameters used to define Mars Special Regions, and physical features on Mars that can be interpreted as Mars Special Regions. We conclude that any region experiencing temperatures > -25 degrees C for a few hours a year and a water activity > 0.5 can potentially allow the replication of terrestrial microorganisms. Physical features on Mars that can be interpreted as meeting these conditions constitute a Mars Special Region. Based on current knowledge of the martian environment and the conser…

Atmospheric Science010504 meteorology & atmospheric sciencesPlanetary protectionLiquid waterAerospace EngineeringTerrainBACTERIAL-ACTIVITY01 natural sciencesSPACECRAFT SURFACESAstrobiologyWater-vaporSouth-pole snow0103 physical sciencesBacterial activitySpace research010303 astronomy & astrophysicsBacterial activity0105 earth and related environmental sciencesMartianCommittee on Space ResearchCOSPAR mars special regions colloquiumNear-surfaceAstronomy and AstrophysicsMars Exploration Program15. Life on landGround ice[PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph]GeophysicsLiquid water13. Climate actionSpace and Planetary ScienceGeneral Earth and Planetary SciencesHigh obliquitySea-iceUpper martian surfaceSpace-craft surfacesGeology
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FIDO science payload simulating the Athena Payload

2002

[1] The Jet Propulsion Laboratory's Field Integrated Development and Operations rover (FIDO) emulates and tests operational rover capabilities for advanced Mars rover missions, such as those originally planned for the Mars Surveyor 2001 Rover and currently planned for the Athena Payload on the Mars Exploration Rovers scheduled for launch in 2003. This paper describes FIDO's science instrument payload, which is fully integrated with rover hardware and software. Remote science teams visualize instrument suite data and generate FIDO commands using the Web Interface for Telescience. FIDO's instrument suite has been used in terrestrial laboratory and field tests to simulate Mars operations, to t…

Atmospheric ScienceComputer scienceSoil ScienceAquatic ScienceOceanographyExploration of Marslaw.inventionSoftwareGeochemistry and PetrologylawEarth and Planetary Sciences (miscellaneous)Earth-Surface ProcessesWater Science and TechnologyRemote sensingEcologySpectrometerbusiness.industryPaleontologyForestryMars Exploration ProgramRobot end effectorMars roverGeophysicsStereo imagingSpace and Planetary ScienceRadiancebusinessJournal of Geophysical Research: Planets
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Opportunity Mars Rover mission: Overview and selected results from Purgatory ripple to traverses to Endeavour crater

2011

Opportunity has been traversing the Meridiani plains since 25 January 2004 (sol 1), acquiring numerous observations of the atmosphere, soils, and rocks. This paper provides an overview of key discoveries between sols 511 and 2300, complementing earlier papers covering results from the initial phases of the mission. Key new results include (1) atmospheric argon measurements that demonstrate the importance of atmospheric transport to and from the winter carbon dioxide polar ice caps; (2) observations showing that aeolian ripples covering the plains were generated by easterly winds during an epoch with enhanced Hadley cell circulation; (3) the discovery and characterization of cobbles and boul…

Atmospheric ScienceEcologyEarth sciencePaleontologySoil ScienceMars exploration roverForestryAquatic ScienceOceanographyAstrobiologyMars roverGeophysicsImpact craterSpace and Planetary ScienceGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)PurgatoryGeologyEarth-Surface ProcessesWater Science and Technology
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Spirit Mars Rover Mission: Overview and selected results from the northern Home Plate Winter Haven to the side of Scamander crater

2010

Spirit Mars Rover Mission : Overview and selected results from the northern Home Plate Winter Haven to the side of Scamander crater

Atmospheric ScienceEcologyEarth sciencePaleontologySoil ScienceMars exploration roverForestryMars Exploration ProgramAquatic ScienceOceanographyExploration of MarsHavenAstrobiologyMars roverGeophysicsImpact craterSpace and Planetary ScienceGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)GeologyEarth-Surface ProcessesWater Science and TechnologyJournal of Geophysical Research
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Meteorites on Mars observed with the Mars Exploration Rovers

2008

[1] Reduced weathering rates due to the lack of liquid water and significantly greater typical surface ages should result in a higher density of meteorites on the surface of Mars compared to Earth. Several meteorites were identified among the rocks investigated during Opportunity's traverse across the sandy Meridiani plains. Heat Shield Rock is a IAB iron meteorite and has been officially recognized as “Meridiani Planum.” Barberton is olivine-rich and contains metallic Fe in the form of kamacite, suggesting a meteoritic origin. It is chemically most consistent with a mesosiderite silicate clast. Santa Catarina is a brecciated rock with a chemical and mineralogical composition similar to Bar…

Atmospheric ScienceEcologyPaleontologySoil ScienceForestryMars Exploration ProgramAquatic ScienceOceanographyIron meteoriteStrewn fieldAstrobiologyKamaciteMesosideriteGeophysicsImpact craterMeteoriteSpace and Planetary ScienceGeochemistry and PetrologyChondriteEarth and Planetary Sciences (miscellaneous)GeologyEarth-Surface ProcessesWater Science and TechnologyJournal of Geophysical Research
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Evidence for montmorillonite or its compositional equivalent in Columbia Hills, Mars

2007

During its exploration of the Columbia Hills, the Mars Exploration Rover ‘‘Spirit’’ encountered several similar samples that are distinctly different from Martian meteorites and known Gusev crater soils, rocks, and sediments. Occurring in a variety of contexts and locations, these ‘‘Independence class’’ samples are rough-textured, iron-poor (equivalent FeO 4 wt%), have high Al/Si ratios, and often contain unexpectedly high concentrations of one or more minor or trace elements (including Cr, Ni, Cu, Sr, and Y). Apart from accessory minerals, the major component common to these samples has a compositional profile of major and minor elements whic…

Atmospheric ScienceGeochemistryMarsSoil ScienceMineralogymontmorilloniteAquatic ScienceOceanographychemistry.chemical_compoundImpact craterGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)chemical compositionEarth-Surface ProcessesWater Science and TechnologyGusevMineralEcologyPaleontologyForestryColumbia HillsclayMars Exploration ProgramMars explorationSilicateGeophysicsMontmorilloniteMeteoritechemistrySpace and Planetary ScienceroverGusev CraterSoil horizonClay mineralsGeologyJournal of Geophysical Research
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Geochemical and mineralogical indicators for aqueous processes in the Columbia Hills of Gusev crater, Mars

2006

[1] Water played a major role in the formation and alteration of rocks and soils in the Columbia Hills. The extent of alteration ranges from moderate to extensive. Five distinct rock compositional classes were identified; the order for degree of alteration is Watchtower ≅ Clovis > Wishstone ≅ Peace > Backstay. The rover's wheels uncovered one unusual soil (Paso Robles) that is the most S-rich material encountered. Clovis class rocks have compositions similar to Gusev plains soil but with higher Mg, Cl, and Br and lower Ca and Zn; Watchtower and Wishstone classes have high Al, Ti, and P and low Cr and Ni; Peace has high Mg and S and low Al, Na, and K; Backstay basalts have high Na and K comp…

Atmospheric ScienceGeochemistrySoil ScienceMineralogyPyroxeneAquatic Scienceengineering.materialOceanographyFeldsparGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Composition of MarsAllophaneEarth-Surface ProcessesWater Science and TechnologyBasaltgeographygeography.geographical_feature_categoryOlivineEcologyPaleontologyForestryVolcanic rockGeophysicsSpace and Planetary Sciencevisual_artengineeringvisual_art.visual_art_mediumIlmeniteGeologyJournal of Geophysical Research: Planets
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