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Making A Broad Impact Through LLS.webm

Science · Video

Making A Broad Impact Through LLS.webm

Laboratory Leadership Service (LLS) fellow Rita Stinnett (PhD, MHS) shared why LLS is a challenge worth accepting. From research to emergency response work, LLS fellows help solve major public health challenges while gaining experience in biosafety, emergency response, quality management systems, and more! This video was originally posted to Instagram ( https://www.instagram.com/p/Bw7ugVsnprv/ ) during the 2019 Epidemic Intelligence Service (EIS) conference. Learn more about the LLS program at www.cdc.gov/eis. Comments on this video are allowed in accordance with our comment policy: https://www.cdc.gov/SocialMedia/Tools/CommentPolicy.html This video can also be viewed at https://www.cdc.gov/wcms/video/low-res/lls/2019/74527452making-a-broad-impact-through-lls-rina-stinnett.mp4

Wikimedia Commons · Public domain · ♥ 0

Seizing Fulfilling Opportunities- Cecilia Kretz (LLS 2017).webm

Science · Video

Seizing Fulfilling Opportunities- Cecilia Kretz (LLS 2017).webm

Laboratory Leadership Service fellow Cecilia Kretz shares about the personal and professional growth that the LLS fellowship provides and her experience as both a laboratorian and a liaison at the New York State Department of Health. For more information about CDC’s LLS fellowship, visit www.cdc.gov/lls. Comments on this video are allowed in accordance with our comment policy: https://www.cdc.gov/SocialMedia/Tools/CommentPolicy.html This video can also be viewed at https://www.cdc.gov/lls/videos/lls-kretz.wmv

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Liberia Laboratory Progress.webm

Science · Video

Liberia Laboratory Progress.webm

Liberia Laboratory Progress Laboratories, and the Ebola testing they perform, play a crucial role in responding to Ebola both in West Africa and in the United States. When lab responders arrived in Liberia they identified a need for laboratories and quickly set up mobile labs. CDC jointly ran a lab in Liberia with the National Institutes of Health, and supports labs in Liberia with the U.S. Department of Defense. Comments on this video are allowed in accordance with our comment policy: https://www.cdc.gov/SocialMedia/Tools/CommentPolicy.html This video can also be viewed at https://www.cdc.gov/wcms/video/low-res/globalhealth/2019/33043304liberia-laboratory-progress-hiRez.mp4

Wikimedia Commons · Public domain · ♥ 0

Asteroid2016HO3-SunEarthOrbit.webm

Science · Video

Asteroid2016HO3-SunEarthOrbit.webm

News: June 15, 2016 Small Asteroid Is Earth's Constant Companion http://www.jpl.nasa.gov/news/news.php?feature=6537 Asteroid 2016 HO3 has an orbit around the sun that keeps it as a constant companion of Earth NASA/JPL IMAGE Asteroid 2016 HO3 has an orbit around the sun that keeps it as a constant companion of Earth. Credit: NASA/JPL-Caltech › Larger view A small asteroid has been discovered in an orbit around the sun that keeps it as a constant companion of Earth, and it will remain so for centuries to come. As it orbits the sun, this new asteroid, designated 2016 HO3, appears to circle around Earth as well. It is too distant to be considered a true satellite of our planet, but it is the best and most stable example to date of a near-Earth companion, or "quasi-satellite." "Since 2016 HO3 loops around our planet, but never ventures very far away as we both go around the sun, we refer to it as a quasi-satellite of Earth," said Paul Chodas, manager of NASA's Center for Near-Earth Object (NEO) Studies at the Jet Propulsion Laboratory in Pasadena, California. "One other asteroid -- 2003 YN107 -- followed a similar orbital pattern for a while over 10 years ago, but it has since departed our vicinity. This new asteroid is much more locked onto us. Our calculations indicate 2016 HO3 has been a stable quasi-satellite of Earth for almost a century, and it will continue to follow this pattern as Earth's companion for centuries to come." NASA/JPL VIDEO (01:00) Asteroid 2016 HO3 - Earth's Constant Companion In its yearly trek around the sun, asteroid 2016 HO3 spends about half of the time closer to the sun than Earth and passes ahead of our planet, and about half of the time farther away, causing it to fall behind. Its orbit is also tilted a little, causing it to bob up and then down once each year through Earth's orbital plane. In effect, this small asteroid is caught in a game of leap frog with Earth that will last for hundreds of years. The asteroid's orbit also undergoes a slow, back-and-forth twist over multiple decades. "The asteroid's loops around Earth drift a little ahead or behind from year to year, but when they drift too far forward or backward, Earth's gravity is just str

Wikimedia Commons · Public domain · ♥ 0

PIA17061-MSL-RAD-RadiationStudy-20130530.jpg

Science · Photo

PIA17061-MSL-RAD-RadiationStudy-20130530.jpg

PIA17061: Calculating Radiation Dose for Biological Tissue http://photojournal.jpl.nasa.gov/catalog/PIA17061 The relationship between charged-particle radiation dose measured with silicon sensors and the dose that biological tissue would receive in the same setting is assessed as a function of how much energy the charged particles would deposit in water (which serves as a proxy for biological tissue). This graph shows the flux of energetic particles (vertical axis) as a function of the estimated energy deposited in water (horizontal axis). The term "dose equivalent," which is used to discuss health risk from radiation exposure, takes this relationship into account. A quality factor, Q, is used to convert measured dose to dose equivalent. The green line on this graph indicates the biological weighting function of how Q is related to how charged-particle radiation deposits energy in water. These factors have been used in the process of interpreting the ramifications for future human interplanetary missions from the measurements made by the Radiation Assessment Detector inside NASA's Mars Science Laboratory spacecraft during the spacecraft's travel from Earth to Mars in 2011 and 2012. Southwest Research Institute, in San Antonio, Texas, and Boulder, Colo., supplied and operates the RAD instrument in collaboration with Germany's national aerospace research center, Deutsches Zentrum für Luft- und Raumfahrt. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Science Laboratory Project and the mission's Curiosity rover for NASA's Science Mission Directorate in Washington. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology, Pasadena, manages the Mars Science Laboratory Project for NASA's Science Mission Directorate, Washington. JPL designed and built the rover. For more information about Curiosity and its mission, visit: http://www.nasa.gov/msl and http://mars.jpl.nasa.gov/msl .

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Laboratory (3).jpg

Science · Photo

Laboratory (3).jpg

Title Laboratory Description A laboratory apparatus for immunology research. These photographs are taken at Massachusetts Institute of Technology (MIT). Only the equipment is visible. Topics/Categories Science and Technology -- Laboratory Techniques/Equipment Type Color, Photo Source National Cancer Institute

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Mars Science Laboratory empty chassis.jpg

Science · Photo

Mars Science Laboratory empty chassis.jpg

Mars Science Laboratory empty chasis after a successful test of the suspension system by the Jet Propulsion Laboratory .

Wikimedia Commons · Public domain · ♥ 0

MSL Concept.jpg

Science · Photo

MSL Concept.jpg

NASA's Mars Science Laboratory , a mobile robot for investigating Mars' past or present ability to sustain microbial life, is in development for a launch opportunity in 2009 . This picture is an artist's concept portraying what the advanced rover would look like in Martian terrain, from a side aft angle. The arm extending from the front of the rover is designed both to position some of the rover's instruments onto selected rocks or soil targets and also to collect samples for analysis by other instruments. Near the base of the arm is a sample preparation and handling system designed to grind samples, such as rock cores or small pebbles, and distribute the material to analytical instruments. The mast, rising to about 2.1 meters (6.9 feet) above ground level, supports two remote-sensing instruments: the Mast Camera for stereo color viewing of surrounding terrain and material collected by the arm, and the ChemCam for analyzing the types of atoms in material that laser pulses have vaporized from rocks or soil targets up to about 9 meters (30 feet) away.

Wikimedia Commons · Public domain · ♥ 0

Imaging the Orion Nebula at Mud Lake.webm

Space · Video

Imaging the Orion Nebula at Mud Lake.webm

An 8" Ritchey–Chrétien telescope images panels of an Orion Nebula mosaic at Mud Lake Wildlife Area in Columbia County, Wisconsin, USA. The session is briefly interrupted by clouds.

Wikimedia Commons · CC BY 4.0 · ♥ 0

Conversatorio Astrónomas y científicas. Iluminando el universo contra la invisibiilización..webm

Space · Video

Conversatorio Astrónomas y científicas. Iluminando el universo contra la invisibiilización..webm

En el marco de los Conversatorios que Cuarto Propio en Wikipedia organiza desde 2015 con el fin debatir y reflexionar en torno a cuestiones de interés feminista, en esta ocasión contamos con Marina Rodríguez Baras, Doctora en Astrofísica, investigadora del Observatorio Astronómico Nacional e integrante de la Comisión Mujeres y Astronomía de la Sociedad Española de Astronomía (SEA). Ella nos hablará de astrónomas y científicas, dándonos a conocer a muchas de ellas y el contexto en el que desarrollan su trabajo. Mas información: - Estudio de la brecha salarial de género en las universidades públicas españolas (ANECA, CRUE): https://www.aneca.es/-/el-ministerio-de-universidades-aneca-y-crue-igualdad-presentaron-el-13-de-junio-el-informe-brecha-salarial-de-g%C3%A9nero-en-las-universidades-p%C3%BAblicas-espa%C3%B1olas./ - Estadísticas comparables a nivel europeo sobre la igualdad de género en la investigación y la innovación (Comisión Europea): https://research-and-innovation.ec.europa.eu/knowledge-publications-tools-and-data/interactive-reports_en - Participación de las científicas como fuentes expertas en los medios: motivaciones y obstáculos (Ministerio de Ciencia, Innovación y Universidades): https://www.fecyt.es/publicaciones/participacion-de-las-cientificas-como-fuentes-expertas-en-los-medios-motivaciones-y/ - Radiografía de la brecha de género en la formación STEAM. Un estudio en detalle de la trayectoria educativa de niñas y mujeres en España (Ministerio de Educación, Formación Profesional y Deportes): https://www.libreria.educacion.gob.es/libro/radiografia-de-la-brecha-de-genero-en-la-formacion-steam-un-estudio-en-detalle-de-la-trayectoria-educativa-de-ninas-y-mujeres-en-espana_173513/

Wikimedia Commons · CC BY 3.0 · ♥ 0

Imaging with an RC at York Prairie.webm

Space · Video

Imaging with an RC at York Prairie.webm

An 8" Ritchey–Chrétien telescope on a strain wave mount and equipped with a monochrome camera and filter wheel tracks the Pleiades and the Orion Nebula under dark skies in York Prairie, WI, USA. At the start of the time lapse, the rig is imaging the last three panels of a 12-panel mosaic of the Pleiades. The mount then slews to home position, awaiting further instructions, and then slews to the Orion Nebula. The camera position is adjusted so that Orion moves into the frame, and the rig images two panels of the Orion Nebula before the time lapse ends. Although the mount was set to dither at set intervals, each visible mount motion corresponds to a switch between panels.

Wikimedia Commons · CC BY 4.0 · ♥ 0

Using Infrared to Survey Our Galaxy’s Far Side (SVS14521 Galactic Plane Infrared good).webm

Space · Video

Using Infrared to Survey Our Galaxy’s Far Side (SVS14521 Galactic Plane Infrared good).webm

Observatories with smaller views of space have provided exquisite images of other galaxies, revealing complex structures. But studying our own galaxy’s anatomy is surprisingly difficult. The plane of the Milky Way covers such a large area on the sky that studying it in detail can take a very long time. Astronomers also must peer through thick dust that obscures distant starlight. Infrared light can pass through that dust and is a key tool for learning about the far side of our galaxy.Credit: NASA's Goddard Space Flight CenterMusic: "Time Shift Equalibrium" from Universal Production MusicWatch this video on the NASA Goddard YouTube channel.Complete transcript available.

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Fermi Mission Detects Surprising Gamma-Ray Feature Beyond Our Galaxy (SVS14476 - Dipole Overlay 1080).webm

Space · Video

Fermi Mission Detects Surprising Gamma-Ray Feature Beyond Our Galaxy (SVS14476 - Dipole Overlay 1080).webm

Top: An all-sky map of extragalactic gamma rays in which the central plane of our galaxy, shown in dark blue where data has been removed, runs across the middle. The red dot and circles indicate the approximate direction from which more gamma rays than average seem to be arriving. Bottom: A similar all-sky map showing the distribution of ultrahigh-energy cosmic rays detected by the Pierre Auger Observatory in Argentina. Red indicates directions from which greater than average numbers of particles arrive, blue indicates directions with fewer than average. This video superposes the Fermi map onto the cosmic ray map, illustrating the similarity of the dipole directions. Credit: Kashlinsky et al. 2024 and the Pierre Auger Collaboration

Wikimedia Commons · Public domain · ♥ 0

I Tested Every Camera MOD for Astrophotography.webm

Space · Video

I Tested Every Camera MOD for Astrophotography.webm

Want more Ha? You will want to modify your DSLR, but which mod is the one for you? Watch this video, then check out AstroGear when ready to pull the trigger on your next mod: https://www.astrogear.net/?ref=nebulaphotos This video only compares Canon cameras, but next week I will be covering: Canon vs. Nikon!

Wikimedia Commons · CC BY 3.0 · ♥ 0

What Is Redshift- - Astronomic.webm

Space · Video

What Is Redshift- - Astronomic.webm

Support ASTRONOMIC: https://www.patreon.com/Astronomic PayPal Donations: astronomicmedia@gmail.com Subscribe to ASTRONOMIC: https://www.youtube.com/astronomic1 Twitter: https://www.twitter.com/astronomic1 Instagram: https://www.instragram.com/astronomic1 Facebook: https://www.facebook.com/astronomicbook Exclusive Content: https://www.curious.com/astronomic Hello Everyone! Welcome to OUR Universe! If you've enjoyed the video... click the LIKE button! If you want to support the channel... click the SUBSCRIBE button! TITLE: What Is Redshift? LINKS: 1. Redshift (Wiki) https://en.m.wikipedia.org/wiki/Redshift 2. Calculating Redshift (Hyperphysics) http://hyperphysics.phy-astr.gsu.edu/hbase/Astro/redshf.html 3. The Expanding Universe (BBC Bitesize) http://www.bbc.co.uk/education/guides/zphppv4/revision/2 OTHER VIDEOS: 1. How BIG Is The Milky Way? https://www.youtube.com/watch?v=5XTx1Qer9tk 2. How Many Planets Are In The Milky Way? https://www.youtube.com/watch?v=d9x9RRc0RoU 3. Can Black Holes Stop Time?! https://www.youtube.com/watch?v=ZFnUAFCffXE Thanks for Watching! Twitter: https://www.twitter.com/astronomic1 Instagram: https://www.instragram.com/astronomic1 Facebook: https://www.facebook.com/astronomicbook Exclusive Content: https://www.curious.com/astronomic Support ASTRONOMIC:

Wikimedia Commons · CC BY 3.0 · ♥ 0

Cancri 55 e- Climate Patterns on a Lava World.webm

Space · Video

Cancri 55 e- Climate Patterns on a Lava World.webm

This illustration video shows one possible scenario for the hot, rocky exoplanet called 55 Cancri e, which is nearly two times as wide as Earth. Image credit: NASA/JPL-Caltech

Wikimedia Commons · CC BY 3.0 · ♥ 0

SOFIA - the largest airborne observatory in the world.webm

Space · Video

SOFIA - the largest airborne observatory in the world.webm

The Stratospheric Observatory for Infrared Astronomy (SOFIA) is a joint German-US space science project. Carrying a 2.5-metre telescope inside a modified Boeing 747SP, the airborne observatory performs astronomical observations in the infrared and submillimetre wavelengths, high above the disturbance of Earth's atmosphere. The scientific objective is to understand the development of galaxies and the formation and evolution of stars and planetary systems from interstellar clouds of gas and dust. dlr.de/en/sofia DEUTSCH: Das Stratosphären-Observatorium für Infrarot-Astronomie (SOFIA) ist ein gemeinsames deutsch-amerikanisches Vorhaben zur Erforschung des Weltalls. Mit dem in eine modifizierte Boeing 747SP integrierten 2,7 Meter-Teleskop werden astronomische Beobachtungen im Infrarot- und Submillimeter-Wellenlängenbereich weitgehend oberhalb der störenden irdischen Lufthülle durchgeführt. Schwerpunkt der wissenschaftlichen Zielsetzung ist die Erforschung der Entwicklung von Milchstraßensystemen sowie die Entstehung und Entwicklung von Sternen und Sonnensystemen aus interstellaren Molekül- und Staubwolken. Blog: dlr.de/blogs/home/sofia/Dokumentation-Die-fliegende-Sternwarte-SOFIA-948.aspx Sonderseite SOFIA dlr.de/sofia

Wikimedia Commons · CC BY 3.0 · ♥ 0

Starry sky with North Star circled.webm

Space · Video

Starry sky with North Star circled.webm

Time-lapse of the night sky and stars revolving around the celestial North Pole. Filmed in Petit-Croix, northeastern France. The original video lasts about 1.4 seconds, so here it has been repeated eight times to give a total length of about 11 seconds and make it easier to see the effect. In addition, the North Star has been circled in red to highlight how the other stars seem to revolve around it.

Wikimedia Commons · CC BY 3.0 · ♥ 0

Comets Kick up Dust in Helix Nebula (PIA09178).jpg

Space · Photo

Comets Kick up Dust in Helix Nebula (PIA09178).jpg

This infrared image from NASA's Spitzer Space Telescope shows the Helix Nebula , a cosmic starlet often photographed by amateur astronomers for its vivid colors and eerie resemblance to a giant eye. The nebula, located about 700 light-years away in the constellation Aquarius, belongs to a class of objects called planetary nebulae. Discovered in the 18th century, these colorful beauties were named for their resemblance to gas-giant planets like Jupiter. Planetary nebulae are the remains of stars that once looked a lot like our sun. When sun-like stars die, they puff out their outer gaseous layers. These layers are heated by the hot core of the dead star, called a white dwarf, and shine with infrared and visible colors. Our own sun will blossom into a planetary nebula when it dies in about five billion years. In Spitzer's infrared view of the Helix nebula, the eye looks more like that of a green monster's. Infrared light from the outer gaseous layers is represented in blues and greens. The white dwarf is visible as a tiny white dot in the center of the picture. The red color in the middle of the eye denotes the final layers of gas blown out when the star died. The brighter red circle in the very center is the glow of a dusty disk circling the white dwarf (the disk itself is too small to be resolved). This dust, discovered by Spitzer's infrared heat-seeking vision, was most likely kicked up by comets that survived the death of their star. Before the star died, its comets and possibly planets would have orbited the star in an orderly fashion. But when the star blew off its outer layers, the icy bodies and outer planets would have been tossed about and into each other, resulting in an ongoing cosmic dust storm. Any inner planets in the system would have burned up or been swallowed as their dying star expanded. So far, the Helix nebula is one of only a few dead-star systems in which evidence for comet survivors has been found. This image is made up of data from Spitzer's infrared array camera and multiband imaging photometer. Blue shows infrared light of 3.6 to 4.5 microns; green shows infrared light of 5.8 to 8 microns; and red shows infrared light of 24 microns.

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