We conducted four surveys, and resultant data is recorded on four separate sheets within the document, titled S1, S2, S3, and NAS. The S1-S3 data pertain to surveys of astrobiologists on the existence of basic/complex/intelligent extraterrestrial life. The NAS data pertain to a survey of non-astrobiologist scientists, on the existence of any kind of extraterrestrial life.

Extra-terrestrial liberty : an enquiry into the nature and causes of tyrannical government beyond the Earth is a book. It was written by Charles Cockell and published by Shoving Leopard in 2013.

E T özgün adı E T the Extra Terrestrial 1982 yapımı bilimkurgu filmi Yönetmenliğini Steven Spielberg ün yaptığ

The DAISIE - inventory of alien invasive species in Europe is a species checklist dataset published by the Research Institute for Nature and Forest (INBO) and the Centre for Ecology and Hydrology (CEH). It contains information on 12,104 taxa (mostly species and mostly introduced) occurring in the wild in Europe since 1500. It covers a broad taxonomic spectrum of terrestrial and aquatic free living and parasitic organisms. The collation of the alien species list is the result of the efforts of the DAISIE (http://www.europe-aliens.org/) project partners and more than 300 collaborators from Europe and neighbouring countries, involved in different fields of expertise and organisations. Here the DAISIE checklist is published as a standardized Darwin Core Archive and includes for each species: the scientific name, higher classification, and stable taxon identifier (in the taxon core), the vernacular names (in the vernacular names extension), the presence in a specific region, the year of the first introduction (first collection) and/or last assessment/observation in that region, as well as extra information (in the distribution extension), and the habitat, native range, and ecofunctional group (in the description extension). The DAISIE dataset is no longer maintained, but can be used as a historical archive for researching and managing alien plants or compiling regional and national registries of alien species. Issues with the dataset can be reported at https://github.com/trias-project/daisie-checklist

We have released this dataset under a Creative Commons Attribution license (CC-BY 4.0). We would appreciate it if you follow the GBIF citation guidelines (https://www.gbif.org/citation-guidelines) when using the data. If you have any questions regarding this dataset, don’t hesitate to contact us via the contact information provided in the metadata or via https://twitter.com/trias_project.

The publication of the checklist to GBIF was supported by the European Cooperation in Science and Technology (COST) action Alien CSI “CA17122 - Increasing understanding of alien species through citizen science” as a Short Term Scientific Mission “Publishing alien species checklist data for Europe through repeatable, open workflows”, with technical support provided by the Research Institute for Nature and Forest (INBO).

When germinated and grown on-board the ISS (International Space Station) plant do not exhibit abnormal structures but they do have altered growth habits and this project aims to investigate the molecular mechanisms that provide the foundation for the altered growth habits observed in orbit. APEX03-2 (Advanced Plant Experiment 03-2) also known as TAGES-ISA (Transgenic Arabidopsis Gene Expression System-Intracellular Signaling Architecture) specifically addresses the growth and molecular changes that occur in Arabidopsis thaliana plants during spaceflight by using molecular and genetic tools and by asking fundamental questions regarding root structure growth and cell wall remodeling may be answered. This investigation advances the fundamental understanding of the molecular biological responses to extraterrestrial environments. This understanding helps to further define the impacts of spaceflight on biological systems to better enable NASA x92s future space exploration goals.

The abundances of Platinum Group Elements (PGEs: Ruthenium, Rhodium, Palladium, Osmium, Iridium, and Platinum) are high in meteorites and extremely low in terrestrial rocks and water and accumulations of mainly platinum and iridium in ancient polar archives have been argued to trace terrestrial (continental/volcanic dust) and extra-terrestrial sources. The PGE concentration data, however, lack specificity. For example, the extent to which terrestrial dust compared to cosmic dust has contributed to the PGE inventory of polar ice cannot be readily evaluated from the PGE concentration data alone. Since the osmium isotopic compositions (R(187Os/188Os) ratio) of terrestrial (= 1.40 ± 0.30) and extraterrestrial/volcanic sources (= 0.13) are distinctly different from each other, osmium isotopic composition has the potential to elucidate relative contributions from these sources in ancient polar ice. However, the determination of osmium isotopes in polar ice core archives is challenging due to extremely low concentrations (∼10E-15 g g−1), and due to the availability of small sample sizes (tens of grams). The main objective of this study is to develop a highly sensitive procedure that allows accurate and precise determination of osmium concentration and isotope composition using ~50 g of melted Greenland ice or snow. By substantially improving previously established clean lab chemistry and high sensitivity mass spectrometry we analyzed snow collected from Summit, Greenland during 2009, 2014, and 2017. We find that the average osmium concentration of the snow is 0.459 ± 0.018 (95% C.I.) fg g−1 corresponding to an osmium flux of 0.0579 ± 0.0023 (95% C.I.) fmol cm−2 yr−1. The average R(187Os/188Os) ratio of the Summit snow is 0.264 ± 0.026 (95% C.I.). Assuming that the volcanic source is negligible, the average ratio indicates that about 0.0518 ± 0.0040 (95% C.I.) fmol cm−2 yr−1 of osmium is of cosmic derivation, corresponding to an accretion rate of extra-terrestrial osmium to the Earth of 264 ± 21 mol yr−1. This assessment is similar to the present-day accretion rate of extra-terrestrial osmium to the Earth determined by previous studies. Because of its sensitivity our procedure can be extended to study changes in the accretion of extra-terrestrial osmium over the last several hundred thousand years using samples of ice core. The data contains osmium concentration and isotope composition of (1) reagents and procedural blanks of two Osmium purification methods (Table 1), (2) Antarctic sea snow, sea water, and NEEM firn for method comparison (Table 2), and finally (3) modern snow from Summit, Greenland for sample application (Table 3).

Atari - ET The Extra-Terrestrial Atari 2600 - ET

Source: Objaverse 1.0 / Sketchfab

The aim of this proposal is to investigate the application of highly-curved HAPG analyzer crystals in WD-XRF spectroscopy for the simultaneous analysis of lanthanides in unique extraterrestrial materials and explore its 3D voxel scanning capabilities at low excitation energies. For this a novel analysis technique is proposed to obtain non-destructive, selective volume information of rare earth elements (REEs) in µm-sized analogues of coarse grain asteroid samples in preparation for the initial analysis of materials from asteroid sample return missions. The combination of cylindrical HAPG optics with ultra-high curvature having a mm-sized working distance is expected to provide higher throughput and collimation as compared to high energy resolution fluorescence detection (HERFD) spectroscopy.

This data compilation contains uranium isotopes (234U/235U/238U) and concentration data on a suite of terrestrial and extra-terrestrial samples for understanding the uranium isotope cycling on Earth. Sample list includes meteorites (ordinary chondrites, eucrites), mantle-derived basalts (Ocean Island Basalts, Mid-Ocean Ridge Basalts), arc volcanics, altered oceanic crust (ODP 801), volcanici-clastic sediments, seawater, fossil corals and organic-rich sediments (From the Black Sea and Cariaco Basin).

Distribution by countries (EEZ): All the terrestrial alien species in Europe. Number of species 13439. Done by EASIN Official on 18-02-2014.

Marine invasive species are currently recognized as one of the major direct causes of biodiversity loss and changes in ecosystem provisioning and supporting services. This dataset documents the recent progress in addressing their growing threat to ocean biodiversity and ecosystems.

When germinated and grown on-board the ISS (International Space Station) plant do not exhibit abnormal structures but they do have altered growth habits and this project aims to investigate the molecular mechanisms that provide the foundation for the altered growth habits observed in orbit. APEX03-2 (Advanced Plant Experiment 03-2) also known as TAGES-ISA (Transgenic Arabidopsis Gene Expression System-Intracellular Signaling Architecture) specifically addresses the growth and molecular changes that occur in Arabidopsis thaliana plants during spaceflight by using molecular and genetic tools and by asking fundamental questions regarding root structure growth and cell wall remodeling may be answered. This investigation advances the fundamental understanding of the molecular biological responses to extraterrestrial environments. This understanding helps to further define the impacts of spaceflight on biological systems to better enable NASA x92s future space exploration goals.

No description is available. Visit https://dataone.org/datasets/2c0389eea7d4afe225ec81e502edc89d for complete metadata about this dataset.

The determination of the extraterrestrial constant of a Dobson spectrophotometer is a book. It was written by Richard Alexander Hamilton and published by Woodside House Hinksey Hill Oxford OX1 5BP in 1967.

This dataset contains images of the sky taken with the HRCAM (High Resolution CAMera) instrument. HRCAM is a digital SLR camera (Canon EOS 50D; 15 megapixels) equipped with a fish-eye lens (Sigma 4.5-mm f/2.8) for all-sky coverage on a 1.6 crop sensor.

HRCAM was primarily designed by Daniel Luong-Van. Nick Tothill helped with construction. Michael Ashley helped with design, construction, software, and operation.

The directories here are:

/documentation PDFs of papers and a PhD thesis describing the instrument and results /raw Canon RAW image files - these are the original images /jpg JPG images extracted from some of the raw files /thumbs Thumbnail images extracted from some of the raw files

Several versions of HRCAM have been built. You can tell which one is used from the serial numbers of the Canon EOS 50D camera, as stored in the RAW image files. Camera serial number 0330104673 was sent to Dome A, 2110703496 to Ridge A, and 2210700089 to Dome Fuji.

The image filenames in the various directories contain the UNIX epoch in seconds at which the exposure started. To convert the UNIX epoch to a date/time, you can use the Linux date command, as per the following example:

data -u -d @1282890600

Images from Dome A:

The original HRCAM was first installed in PLATO at Dome A during January 2010. The camera was refurbished and reinstalled in PLATO-A for 2015.

There are 12703 images, with cadences of 240 and 660 seconds (with different exposure times), taken from Dome A. The images are in raw/h1*.raw, and start with h1282890600.raw at Fri 27 Aug 2010 06:30:00 UTC, and end with h1295604000.raw at Fri 21 Jan 2011 10:00:00 UTC. In addition, there are 709 images, with cadences of 900 seconds in jpg/h12*.jpg, starting with h1282915324.jpg at Fri 27 Aug 2010 13:22:04 UTC, and ending with h1284925919.jpg at Sun 19 Sep 2010 19:51:59 UTC. In addition, there are 10339 images, with cadences from 120 to 1800 seconds, taken from Dome A. The images are in raw/h1-*.raw and jpg/h1-*.jpg, with thumbnails in thumbs/*jpg, and start with h1-1421930703.jpg at Thu 22 Jan 2015 12:45:03 UTC, and end with h1-1434252625.jpg at Sun 14 Jun 2015 03:30:25 UTC.

Images from Dome Fuji:

HRCAM2 was taken to Dome Fuji and installed in PLATO-F by the Japanese 52nd JARE expedition during the 2010/2011 season. In the images, green Engine Module is at the top of the image, two small iridium aerials are at left and bottom, the Iridium Openport antenna is in the insulated white box at lower left, the meteorological tower is also visible. The "egg of vision" is on the right, just above the Iridium aerial. The image reaches to the horizon in all directions.

There are 21336 images, with cadences of 240 and 660 seconds (with different exposure times), taken from Dome Fuji. The images are in raw/h1*.raw, and start with h1296361840.raw at Sun 30 Jan 2011 04:30:40 UTC, and end with h1310294940.raw at Sun 10 Jul 2011 10:49:00 UTC. In addition, there are 8487 images, with cadences of 900 seconds in jpg/h1*.jpg, starting with h1299704642.jpg at Wed 09 Mar 2011 21:04:02 UTC, and ending with h1310295070.jpg at Sun 10 Jul 2011 10:51:10 UTC.

Images from Ridge A:

HRCAM3 was taken to Ridge A and installed in PLATO-R during the 2011/2012 season by a team led by Craig Kuleas of the University of Arizona. In the images, the solar panels are at the top of the image, the Ubob cameras are at 40 degrees CW, the HEAT telescope is at 60 degrees, the SCAR flag is at 110 degrees, and the meteorological tower at 200 degrees. North is at approximately 20 degrees. The image reaches very close to the horizon in all directions.

There are 12730 images, with cadences of 300 seconds, taken from Ridge A. The images are in raw/h3-*.raw, and start with h3-1331181001.raw at Thu 08 Mar 2012 04:30:01 UTC, and end with h3-1335099900.raw at Sun 22 Apr 2012 13:05:00 UTC.

Processing the RAW images:

exiftool is a convenient piece of free software for processing Canon RAW images. dcraw can be used to extract images.

On a Linux computer you can use commands such as these:

To list all the metadata in a RAW file:

exiftool -all h1282890600.raw

To extract the PreviewImage and ThumbnailImage from a RAW file:

exiftool -b -PreviewImage h1282890600.raw - h1282890600.jpg exiftool -b -ThumbnailImage h1282890600.raw - h1282890600-thumb.jpg

To copy metadata to a JPG file:

exiftool -tagsFromFile h1282890600.raw -exif:all -overwrite_original h1282890600.jpg

Techical Information: Sediment depth is given in mcd. Dry bulk density values are determined from high-resolution shipboard GRA bulk density values using the relationship between bulk density, BD, and dry density, DD observed for all of Hole 1266A in shipboard moisture and density data.

The Manual of the Alien Plants of Belgium is a species checklist dataset published by the Botanic Garden Meise. It contains information on all (over 2.500) non-native vascular plants occurring in the wild in Belgium since 1800. The checklist is almost entirely based on a thorough herbarium revision of the main public Belgian herbaria (Verloove 2006), actively maintained, and updated regularly at Verloove (2018, http://alienplantsbelgium.be). Here it is published as a standardized Darwin Core Archive and includes for each species: the scientific name, kingdom, family, stable taxon identifier, and IPNI (2018) scientific name ID where available (in the taxon core), the presence in Flanders, Wallonia and the Brussels Capital Region, as well as the year of the first introduction (first collection) and last assessment/observation in Belgium (given as a year range in the event date in the distribution extension), coarse habitat information (in the species profile extension), and the pathway(s) of introduction, native range(s) and invasion stage in Belgium (in the description extension). The dataset can be used for researching and managing alien plants or compiling regional and national registries of alien species. Issues with the dataset can be reported at https://github.com/trias-project/alien-plants-belgium

We have released this dataset to the public domain under a Creative Commons Zero waiver. We would appreciate it if you follow the GBIF citation guidelines (https://www.gbif.org/citation-guidelines) when using the data. If you have any questions regarding this dataset, don’t hesitate to contact us via the contact information provided in the metadata or via https://twitter.com/trias_project.

This dataset was published as open data for the TrIAS project (Tracking Invasive Alien Species http://trias-project.be, Vanderhoeven et al. 2017), with technical support provided by the Research Institute for Nature and Forest (INBO). It is selected as one of the authoritative sources for the compilation of a unified and reproducible checklist of alien species in Belgium.

The Canadian Environmental Sustainability Indicators (CESI) program provides data and information to track Canada's performance on key environmental sustainability issues. The Invasive alien species in Canada main indicator is the number of invasive alien species found to be newly established in Canada, reported by year and regulatory status. This provides a preliminary indication of the potential harmful consequences of new arrivals. A secondary indicator, the proportion of regulated species that have not established in Canada, is reported as a partial measure of regulatory success. Regulation of potentially invasive species is intended to prevent their introduction and establishment in Canada. Species are added to the list of regulated species based on an analysis of risk. Both indicators report on species establishment since January 2012. With the implementation of the Federal Sustainable Development Strategy 2010–2013, this type of information began to be collected consistently across multiple programs, allowing information to be combined for the first time into a single indicator despite the varying approaches used to control different groups of invasive alien species. Information is provided to Canadians in a number of formats including: static and interactive maps, charts and graphs, HTML and CSV data tables and downloadable reports. See the supplementary documentation for data sources and details on how those data were collected and how the indicator was calculated. Supplemental Information Canadian Environmental Sustainability Indicators - Home page: https://www.canada.ca/environmental-indicators

This zip file contains the ArcGIS Pro files used to analyze the distribution, orientation, and morphologies of peridodic bedrock ridges and transverse aeolian ridges for the manuscript "The Aeolian Environment of the Landing Site for the ExoMars Rosalind Franklin Rover in Oxia Planum, Mars".These .lyrx files are not backwards compatible with Arc 10.6. The files contained in this zip file are: 1. The HiRISE images used2. The 1-sigma ellipses3. The study area grid4. The ripple and PBRs analyzed