Dry Ice Is Not Poisonous, but It Is Extremely Cold and Can Cause Cryogenic Burns to Unprotected Skin
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Dry Ice Blasting
Dry Ice Blasting The Dry Ice Blasting method can reduce the overall time spent on sanding, scraping or scrub- bing with solvents, acids and other cleaning agents. With no secondary waste generation there is no need for disposal of hazardous waste. This saves time and money while increasing worker safety. Online Cleaning of Fin Dry Ice Blasting can safely and effectively clean contaminants that plug and foul fin fan heat Fan Heat Exchangers exchangers. Dry Ice Blasting can be performed while the system is online so no costly downtime is required. Cleaning will increase airflow which will lower approach temperatures and increase efficiency. The dry nature of the process will mitigate the potential for harming motors, bearings or instrumentation. Other Applications May The demand to keep the equipment running often leads to deferred cleaning and maintenance, Also Benefit reduced efficiency and in some cases, outages caused by flashover. Dry ice blast cleaning can provide a non-conductive cleaning process that may allow equipment to be cleaned in-place without cool down or disassembly. This includes generators, turbines, stators, rotors, compressors and boilers. Industrial cleaning applications exist in markets as diverse as food & beverage equipment clean-up, pharmaceutical production, aerospace surfaces & components, and foundry core- making machinery. A Leading Supplier of Working with Linde Services offers you product reliability from an industry leader in carbon Carbon Dioxide dioxide applications. This includes: → A focus on safety -
Companion Q&A Fact Sheet: What Mars Reveals About Life in Our
What Mars Reveals about Life in Our Universe Companion Q&A Fact Sheet Educators from the Smithsonian’s Air and Space and Natural History Museums assembled this collection of commonly asked questions about Mars to complement the Smithsonian Science How webinar broadcast on March 3, 2021, “What Mars Reveals about Life in our Universe.” Continue to explore Mars and your own curiosities with these facts and additional resources: • NASA: Mars Overview • NASA: Mars Robotic Missions • National Air and Space Museum on the Smithsonian Learning Lab: “Wondering About Astronomy Together” Guide • National Museum of Natural History: A collection of resources for teaching about Antarctic Meteorites and Mars 1 • Smithsonian Science How: “What Mars Reveals about Life in our Universe” with experts Cari Corrigan, L. Miché Aaron, and Mariah Baker (aired March 3, 2021) Mars Overview How long is Mars’ day? Mars takes 24 hours and 38 minutes to spin around once, so its day is very similar to Earth’s. How long is Mars’ year? Mars takes 687 days, almost two Earth years, to complete one orbit around the Sun. How far is Mars from Earth? The distance between Earth and Mars changes as both planets move around the Sun in their orbits. At its closest, Mars is just 34 million miles from the Earth; that’s about one third of Earth’s distance from the Sun. On the day of this program, March 3, 2021, Mars was about 135 million miles away, or four times its closest distance. How far is Mars from the Sun? Mars orbits an average of 141 million miles from the Sun, which is about one-and-a-half times as far as the Earth is from the Sun. -
NASA Spacecraft Observes Further Evidence of Dry Ice Gullies on Mars 11 July 2014, by Guy Webster
NASA spacecraft observes further evidence of dry ice gullies on Mars 11 July 2014, by Guy Webster "As recently as five years ago, I thought the gullies on Mars indicated activity of liquid water," said lead author Colin Dundas of the U.S. Geological Survey's Astrogeology Science Center in Flagstaff, Arizona. "We were able to get many more observations, and as we started to see more activity and pin down the timing of gully formation and change, we saw that the activity occurs in winter." Dundas and collaborators used the High Resolution Imaging Science Experiment (HiRISE) camera on MRO to examine gullies at 356 sites on Mars, beginning in 2006. Thirty-eight of the sites showed active gully formation, such as new channel segments and increased deposits at the downhill end of some gullies. Using dated before-and-after images, researchers determined the timing of this activity coincided with This pair of images covers one of the hundreds of sites seasonal carbon-dioxide frost and temperatures on Mars where researchers have repeatedly used the that would not have allowed for liquid water. High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter to study changes in gullies on slopes. Credit: NASA/JPL- Frozen carbon dioxide, commonly called dry ice, Caltech/Univ. of Arizona does not exist naturally on Earth, but is plentiful on Mars. It has been linked to active processes on Mars such as carbon dioxide gas geysers and lines on sand dunes plowed by blocks of dry ice. One Repeated high-resolution observations made by mechanism by which carbon-dioxide frost might NASA's Mars Reconnaissance Orbiter (MRO) drive gully flows is by gas that is sublimating from indicate the gullies on Mars' surface are primarily the frost providing lubrication for dry material to formed by the seasonal freezing of carbon dioxide, flow. -
Physical Changes
How Matter Changes By Cindy Grigg Changes in matter happen around you every day. Some changes make matter look different. Other changes make one kind of matter become another kind of matter. When you scrunch a sheet of paper up into a ball, it is still paper. It only changed shape. You can cut a large, rectangular piece of paper into many small triangles. It changed shape and size, but it is still paper. These kinds of changes are called physical changes. Physical changes are changes in the way matter looks. Changes in size and shape, like the changes in the cut pieces of paper, are physical changes. Physical changes are changes in the size, shape, state, or appearance of matter. Another kind of physical change happens when matter changes from one state to another state. When water freezes and makes ice, it is still water. It has only changed its state of matter from a liquid to a solid. It has changed its appearance and shape, but it is still water. You can change the ice back into water by letting it melt. Matter looks different when it changes states, but it stays the same kind of matter. Solids like ice can change into liquids. Heat speeds up the moving particles in ice. The particles move apart. Heat melts ice and changes it to liquid water. Metals can be changed from a solid to a liquid state also. Metals must be heated to a high temperature to melt. Melting is changing from a solid state to a liquid state. -
It's Just a Phase!
Bay Area Scientists in School Presentation Plan Lesson Name It’s just a phase!______________ Presenter(s) Kevin Metcalf, David Ojala, Melanie Drake, Carly Anderson, Hilda Buss, Lin Louie, Chris Jakobson California Standards Connection(s): 3rd Grade – Physical Science 3-PS-Matter has three states which can change when energy is added or removed. Next Generation Science Standards: 2nd Grade – Physical Science 2-PS1-1. Plan and conduct an investigation to describe and classify different kinds of materials by their observable properties. 2-PS1-4. Construct an argument with evidence that some changes caused by heating or cooling can be reversed and some cannot. Science & Engineering Practices Disciplinary Core Ideas Crosscutting Concepts Planning and carrying out PS1.A: Structure and Properties Patterns investigations to answer of Matter ・Patterns in the natural and questions or test solutions to ・Different kinds of matter exist human designed world can be problems in K–2 builds on prior and many of them can be observed. (2-PS1-1) experiences and progresses to either solid or liquid, simple investigations, based on depending on temperature. Cause and Effect fair tests, which provide data to Matter can be described and ・Events have causes that support explanations or design classified by its observable generate observable patterns. solutions. properties. (2-PS1-1) (2-PS1-4) ・Plan and conduct an ・Different properties are suited ・Simple tests can be designed to investigation collaboratively to to different purposes. (2-PS1- gather evidence to support or produce data to serve as the 2), (2-PS1-3) refute student ideas about basis for evidence to answer a ・A great variety of objects can causes. -
Cosmic Microwave Background
1 29. Cosmic Microwave Background 29. Cosmic Microwave Background Revised August 2019 by D. Scott (U. of British Columbia) and G.F. Smoot (HKUST; Paris U.; UC Berkeley; LBNL). 29.1 Introduction The energy content in electromagnetic radiation from beyond our Galaxy is dominated by the cosmic microwave background (CMB), discovered in 1965 [1]. The spectrum of the CMB is well described by a blackbody function with T = 2.7255 K. This spectral form is a main supporting pillar of the hot Big Bang model for the Universe. The lack of any observed deviations from a 7 blackbody spectrum constrains physical processes over cosmic history at redshifts z ∼< 10 (see earlier versions of this review). Currently the key CMB observable is the angular variation in temperature (or intensity) corre- lations, and to a growing extent polarization [2–4]. Since the first detection of these anisotropies by the Cosmic Background Explorer (COBE) satellite [5], there has been intense activity to map the sky at increasing levels of sensitivity and angular resolution by ground-based and balloon-borne measurements. These were joined in 2003 by the first results from NASA’s Wilkinson Microwave Anisotropy Probe (WMAP)[6], which were improved upon by analyses of data added every 2 years, culminating in the 9-year results [7]. In 2013 we had the first results [8] from the third generation CMB satellite, ESA’s Planck mission [9,10], which were enhanced by results from the 2015 Planck data release [11, 12], and then the final 2018 Planck data release [13, 14]. Additionally, CMB an- isotropies have been extended to smaller angular scales by ground-based experiments, particularly the Atacama Cosmology Telescope (ACT) [15] and the South Pole Telescope (SPT) [16]. -
ACIDS and BASES Unique Properties of Dry Ice
ACIDS AND BASES Unique Properties of Dry Ice OVERVIEW: Students observe properties of dry ice. For example, whether dry ice can change the color of a basic solution that contains an indicator OBJECTIVE: To review basic principles of matter and how this relates to every day objects. Develop concepts and nature of acids and bases and relate this to common household items. GRADE LEVEL: 6-7 OHIO STANDARDS: PS7 Grade 7 Physical Science: The properties of matter are determined by the arrangement of atoms. TIME: 30-45 minutes VOCABULARY: acid, base, organic, inorganic, indicator, pH, hydrogen ion, molecule, CO2, dry ice MATERIALS: (per group of 5-6 students) *Block of dry ice *8 Beakers—600 ml tall with wide mouth *1 Graduated cylinder-10ml *1 stirring rod IMPORTANT: *Gloves.—cotton and latex Read all instructions before *Safety glasses proceeding *Indicator Solutions *pH paper *Balloons *1 pint Ammonia * 1 pint Vinegar DEVELOPED BY: Bob Maloney, Analytical Chemist, BP Chemicals INDICATOR SOLUTIONS: 100-250 ml of one or more of the following: *Grape juice concentrate *Cherry Juice *Beet Juice *Red Cabbage Juice VARIATION: 10-15 ml of one of the following: Thymolphthalein solution: (To prepare 100 ml of stock solution, dissolve 0.04g of thymolphthalein in 50 ml of 95% ethyl alcohol (ethanol) and dilute the resulting solution to 100ml with water. Alternatively, “Disappearing Ink” which is sold in toy stores can be used). Phenolphthalein solution (To prepare 10ml stock solution, dissolve 0.05g phenolphthalein in 50 ml of 95% ethyl alcohol and dilute the resulting solution to 100ml with water. Alternatively, crush two or three EX-Lax tablets and cover with rubbing alcohol and mix. -
Cryocoolers and Heat Exchangers Special Feature
SPECIAL FEATURE – CRYOCOOLERS AND HEAT EXCHANGERS SPECIAL FEATURE evolve from here? Whilst Brouwers “There is more need for path cleanliness. In focus... said that the company’s plans were cryogenic cold at a certain Awe confirmed that CAS has also confidential, he did say that it sees noticed a drastic upturn in demand possibilities in the market in terms of place, at a certain moment, for heat exchanger technology in the Cryocoolers and heat exchangers systems with a higher output compared at a certain time...” LNG sector, highlighting, “Natural with the output that its technology gas processors are morphing from By Rhea Healy can provide at the moment. “That markets, as well as customer bases in the successfully generating and capturing might be a combination of increasing LNG sector. these materials to rolling them out to the hether it’s heating media up the output of our existing technology Jeffery Awe, Marketing Director at marketplace on a massive scale. As the or cooling it down, time is of and systems, but it will also be in CAS, confirmed that the LNG sector is LNG and compressed natural gas (CNG) the essence in the industrial combination with the development of currently the most ‘vibrant’ in terms of industries continue to expand, we’d like gas industry. Companies and new systems. Ultimately, our main goal demand for the company’s technology, to parallel that growth trajectory in our Wengineers need gases and liquid gases to is to be recognised by our customers as along with its traditional industrial gas CAST-X line. -
NASA Observations Point to 'Dry Ice' Snowfall on Mars 12 September 2012
NASA observations point to 'dry ice' snowfall on Mars 12 September 2012 "These are the first definitive detections of carbon- dioxide snow clouds," said the report's lead author, Paul Hayne of NASA's Jet Propulsion Laboratory in Pasadena, Calif. "We firmly establish the clouds are composed of carbon dioxide—flakes of Martian air—and they are thick enough to result in snowfall accumulation at the surface." The snowfalls occurred from clouds around the Red Planet's south pole in winter. The presence of carbon-dioxide ice in Mars' seasonal and residual southern polar caps has been known for decades. Also, NASA's Phoenix Lander mission in 2008 observed falling water-ice snow on northern Mars. Hayne and six co-authors analyzed data gained by looking at clouds straight overhead and sideways Carbon-Dioxide Snowfall on Mars. Observations by with the Mars Climate Sounder, one of six NASA's Mars Reconnaissance Orbiter have detected instruments on the Mars Reconnaissance Orbiter. carbon-dioxide snow clouds on Mars and evidence of carbon-dioxide snow falling to the surface. Deposits of This instrument records brightness in nine small particles of carbon-dioxide ice are formed by wavebands of visible and infrared light as a way to snowfall from carbon-dioxide clouds. This map shows examine particles and gases in the Martian the distribution of small-grain carbon-dioxide ice deposits atmosphere. The analysis was conducted while formed by snowfall over the south polar cap of Mars. It is Hayne was a post-doctoral fellow at the California based on infrared measurements by the Mars Climate Institute of Technology in Pasadena. -
The Temperature of the Cosmic Microwave Background at 10 Ghz D
The Astrophysical Journal, 612:86–95, 2004 September 1 # 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE TEMPERATURE OF THE COSMIC MICROWAVE BACKGROUND AT 10 GHZ D. J. Fixsen,1 A. Kogut,2 S. Levin,3 M. Limon,1 P. Lubin,4 P. Mirel,1 M. Seiffert,3 and E. Wollack2 Received 2004 February 23; accepted 2004 April 14 ABSTRACT We report the results of an effort to measure the low-frequency portion of the spectrum of the cosmic microwave background (CMB) radiation, using a balloon-borne instrument called the Absolute Radiometer for Cosmology, Astrophysics, and Diffuse Emission (ARCADE). These measurements are to search for deviations from a thermal spectrum that are expected to exist in the CMB as a result of various processes in the early universe. The radiometric temperature was measured at 10 and 30 GHz using a cryogenic open-aperture instrument with no emissive windows. An external blackbody calibrator provides an in situ reference. Systematic errors were greatly reduced by using differential radiometers and cooling all critical components to physical temperatures approxi- mating the antenna temperature of the sky. A linear model is used to compare the radiometer output to a set of thermometers on the instrument. The unmodeled residualsarelessthan50mKpeaktopeakwithaweightedrms of 6 mK. Small corrections are made for the residual emission from the flight train, atmosphere, and foreground Galactic emission. The measured radiometric temperature of the CMB is 2:721 Æ 0:010 K at 10 GHz and 2:694 Æ 0:032 K at 30 GHz. Subject headinggs: cosmic microwave background — cosmology: observations 1. -
Cryogen & Dry-Ice Safety Fact Sheet
Cryogen & Dry-Ice Safety Fact Sheet Definitions Cryogen: A liquefied gas with a boiling point typically below 77 K (-196°C). The most commonly cryogens used at the Penn are liquid nitrogen and liquid helium. Dewar: an insulated container used to store and transport liquefied gases. It is insulated by a vacuum between its two walls and is equipped with pressure relief device(s). Dry Ice: Frozen carbon dioxide. Dry ice sublimates from a solid to a gas at room temperature. Pressure-relief devices: Devices on cryogenic systems in place to relieve pressure build up. These devices may be: (1) valves which open to relieve pressure, (2) bursting discs that break to relieve pressure and must be replaced or (3) loose-fitting lids on Dewar flasks. (1) (2) (3) Hazards Associated with Cryogens & Dry Ice 1. Burns: Skin contact with a cryogen, dry ice or non-insulated equipment parts can cause cold burn and frostbite. Eye contact with a cryogen or dry ice can cause permanent damage. Always wear the proper PPE when working with or around cryogens and dry-ice. 2. Asphyxiation: NMR magnet quenching (the loss of superconductivity followed by the rapid release of gaseous cryogens) can result in an oxygen deficient atmosphere. The volumetric expansion rate from the liquid to gaseous phase ranges between 690 to 750 times. The use of dry ice in cold rooms can cause increased breathing, headache, dizziness, nausea and visual disturbances due to elevated carbon dioxide concentrations in the air. Dry ice can also cause asphyxiation in confined spaces. Remember: You can not detect oxygen deficiency or over exposure to Carbon Dioxide. -
Extreme Cold Is a Dangerous Situation That Can Bring on Bring Can That Situation Dangerous a Is Cold Extreme
Centers for Disease Control and Prevention and Control Disease for Centers U.S. Department of Health And Human Services Human And Health of Department U.S. U.S. Department of Health And Human Services Centers for Disease Control and Prevention http://www.bt.cdc.gov/disasters/winter/ 1-888-232-6789; [email protected] 1-888-232-6789; 4700 Buford Hwy, Atlanta, GA 30341-3717 GA Atlanta, Hwy, Buford 4700 National Center for Environmental Health, MS F52 MS Health, Environmental for Center National Centers for Disease Control and Prevention and Control Disease for Centers or more information on cold weather conditions and health, please contact: please health, and conditions weather cold on information more or F For more information on hot weather conditions and health, please contact: Centers for Disease Control and Prevention National Center for Environmental Health, MS F52 4700 Buford Hwy, Atlanta, GA 30341-3717 1-888-232-6789; [email protected] http://www.bt.cdc.gov/disasters/extremeheat/ 1 and what to do if a cold-weather health emergency arises. arises. emergency health cold-weather a if do to what and should know how to prevent cold-related health problems health cold-related prevent to how know should that is poorly insulated or without heat. without or insulated poorly is that can be affected. To keep yourself and your family safe, you safe, family your and yourself keep To affected. be can without shelter or who are stranded, or who live in a home a in live who or stranded, are who or shelter without Infants and the elderly are particularly at risk, but anyone but risk, at particularly are elderly the and Infants health emergencies in susceptible people, such as those as such people, susceptible in emergencies health can cause other serious or life-threatening health problems.