- published: 14 Nov 2009
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Far-infrared astronomy is the branch of astronomy and astrophysics that deals with objects visible in far-infrared radiation (extending from 30 µm towards submillimeter wavelengths around 450 µm).
In the far-infrared, stars are not especially bright, but we can see emission from very cold matter (140 Kelvins or less) that is not seen at shorter wavelengths.
Huge, cold clouds of gas and dust in our own galaxy, as well as in nearby galaxies, glow in far-infrared light. This is due to thermal radiation of interstellar dust contained in molecular clouds. In some of these clouds, new stars are just beginning to form. Far-infrared observations can detect these protostars long before they "turn on" visibly by sensing the heat they radiate as they contract.
The center of our galaxy also shines brightly in the far-infrared: These emissions are from dust in circumstellar shells around numerous old red giant stars. These stars heat up the dust and cause it to glow brightly in the infrared. The Bolocam Galactic Plane Survey mapped the galaxy for the first time in the far-infrared.
Far infrared (FIR) is a region in the infrared spectrum of electromagnetic radiation. Far infrared is often defined as any radiation with a wavelength of 15 micrometers (µm) to 1 mm (corresponding to a range of about 20 THz to 300 GHz), which places far infrared radiation within the CIE IR-B and IR-C bands. Different sources use different boundaries for the far infrared spectrum; for example, astronomers sometimes define far infrared as wavelengths between 25 µm and 350 µm.
Visible light includes radiation with wavelengths between 400 nm and 700 nm, meaning that far infrared photons have less energy than visible light photons.
Objects with temperatures between about 5 K and 340 K will emit radiation in the far infrared range (see Wien's displacement law and Black-body radiation). This property is sometimes used to observe interstellar gases where new stars are often formed.
For example, the center of the Milky Way Galaxy is very bright in far infrared images because the dense concentration of stars there heats the surrounding dust and causes it to emit radiation in this part of the spectrum. Disregarding the center of our own galaxy, the brightest far infrared object in the sky is the galaxy M82, which radiates as much far infrared light from its central region as all of the stars in the Milky Way combined. This is due to the dust at the center of M82 being heated by an unknown source.
Crash Course (also known as Driving Academy) is a 1988 made for television teen film directed by Oz Scott.
Crash Course centers on a group of high schoolers in a driver’s education class; many for the second or third time. The recently divorced teacher, super-passive Larry Pearl, is on thin ice with the football fanatic principal, Principal Paulson, who is being pressured by the district superintendent to raise driver’s education completion rates or lose his coveted football program. With this in mind, Principal Paulson and his assistant, with a secret desire for his job, Abner Frasier, hire an outside driver’s education instructor with a very tough reputation, Edna Savage, aka E.W. Savage, who quickly takes control of the class.
The plot focuses mostly on the students and their interactions with their teachers and each other. In the beginning, Rico is the loner with just a few friends, Chadley is the bookish nerd with few friends who longs to be cool and also longs to be a part of Vanessa’s life who is the young, friendly and attractive girl who had to fake her mother’s signature on her driver’s education permission slip. Kichi is the hip-hop Asian kid who often raps what he has to say and constantly flirts with Maria, the rich foreign girl who thinks that the right-of-way on the roadways always goes to (insert awesomely fake foreign Latino accent) “my father’s limo”. Finally you have stereotypical football meathead J.J., who needs to pass his English exam to keep his eligibility and constantly asks out and gets rejected by Alice, the tomboy whose father owns “Santini & Son” Concrete Company. Alice is portrayed as being the “son” her father wanted.
The Herschel Space Observatory was a space observatory built and operated by the European Space Agency (ESA). It was active from 2009 to 2013, and was the largest infrared telescope ever launched, carrying a single 3.5-metre (11.5 ft) mirror and instruments sensitive to the far infrared and submillimetre wavebands (55–672 µm). Herschel was the fourth cornerstone mission in the ESA science programme, along with Rosetta, Planck, and Gaia. NASA is a partner in the Herschel mission, with US participants contributing to the mission; providing mission-enabling instrument technology and sponsoring the NASA Herschel Science Center (NHSC) at the Infrared Processing and Analysis Center and the Herschel Data Search at the Infrared Science Archive.
The observatory was carried into orbit in May 2009, reaching the second Lagrangian point (L2) of the Earth–Sun system, 1,500,000 kilometres (930,000 mi) from Earth, about two months later. Herschel is named after Sir William Herschel, the discoverer of the infrared spectrum and planet Uranus, and his sister and collaborator Caroline Herschel.
Astronomy, a natural science, is the study of celestial objects (such as stars, galaxies, planets, moons, asteroids, comets and nebulae) and processes (such as supernovae explosions, gamma ray bursts, and cosmic microwave background radiation), the physics, chemistry, and evolution of such objects and processes, and more generally all phenomena that originate outside the atmosphere of Earth. A related but distinct subject, physical cosmology, is concerned with studying the Universe as a whole.
Astronomy is one of the oldest sciences. The early civilizations in recorded history, such as the Babylonians, Greeks, Indians, Egyptians, Nubians, Iranians, Chinese, and Maya performed methodical observations of the night sky. However, the invention of the telescope was required before astronomy was able to develop into a modern science. Historically, astronomy has included disciplines as diverse as astrometry, celestial navigation, observational astronomy and the making of calendars, but professional astronomy is nowadays often considered to be synonymous with astrophysics.
http://www.facebook.com/ScienceReason ... Science@ESA Vodcast (Episode 3, Part 1): Exploring The Infrared Universe. In the Science@ESA series Rebecca Barnes will take you on a journey of discovery into the rapidly evolving field of space astronomy and planetary exploration. --- Please SUBSCRIBE to Science & Reason: • http://www.youtube.com/Best0fScience • http://www.youtube.com/ScienceTV • http://www.youtube.com/FFreeThinker --- In this third episode of the Science@ESA vodcast series we investigate the infrared Universe, explore discoveries made by ground-breaking infrared space telescopes, and take a look at Herschel - ESA's pioneering infrared space telescope. Herschel, ESA's cutting-edge space observatory, will carry the largest, most powerful infrared telescope ever flown in space....
Most telescopes in the world work at visible light wavelengths because this is where stars shine the brightest. However in those places where new objects (e.g. planets, stars, and galaxies) are being born the light is emitted at much longer wavelengths. Thus, to observe the births of new objects requires instrumentation in the far-infrared and submillimeter. Facilities at these wavelengths are either recently built or still under development. In this talk I will review the observational signatures of the formation of new objects, the instruments available, and some of the new instruments under development to do this science. One of these new instruments, the Herschel Space Observatory was launched in May of 2009 - containing a significant piece of Waterloo hardware!
Most telescopes in the world work at visible light wavelengths because this is where stars shine the brightest. However in those places where new objects (e.g. planets, stars, and galaxies) are being born the light is emitted at much longer wavelengths. Thus, to observe the births of new objects requires instrumentation in the far-infrared and submillimeter. Facilities at these wavelengths are either recently built or still under development. In this talk I will review the observational signatures of the formation of new objects, the instruments available, and some of the new instruments under development to do this science. One of these new instruments, the Herschel Space Observatory was launched in May of 2009 - containing a significant piece of Waterloo hardware!
Most telescopes in the world work at visible light wavelengths because this is where stars shine the brightest. However in those places where new objects (e.g. planets, stars, and galaxies) are being born the light is emitted at much longer wavelengths. Thus, to observe the births of new objects requires instrumentation in the far-infrared and submillimeter. Facilities at these wavelengths are either recently built or still under development. In this talk I will review the observational signatures of the formation of new objects, the instruments available, and some of the new instruments under development to do this science. One of these new instruments, the Herschel Space Observatory was launched in May of 2009 - containing a significant piece of Waterloo hardware!
In order to understand how we study the universe, we need to talk a little bit about light. Light is a form of energy. Its wavelength tells us its energy and color. Spectroscopy allows us to analyze those colors and determine an object’s temperature, density, spin, motion, and chemical composition. Crash Course Chemistry posters are available at DFTBA.com http://www.dftba.com/crashcourse -- Table of Contents Light is a Form of Energy 0:39 Wavelength Tells Us Its Energy and Color 0:59 Spectroscopy 7:28 -- PBS Digital Studios: http://youtube.com/pbsdigitalstudios Follow Phil on Twitter: https://twitter.com/badastronomer Want to find Crash Course elsewhere on the internet? Facebook - http://www.facebook.com/YouTubeCrashCourse Twitter - http://www.twitter.com/TheCrashCourse Tumblr - htt...
Most telescopes in the world work at visible light wavelengths because this is where stars shine the brightest. However in those places where new objects (e.g. planets, stars, and galaxies) are being born the light is emitted at much longer wavelengths. Thus, to observe the births of new objects requires instrumentation in the far-infrared and submillimeter. Facilities at these wavelengths are either recently built or still under development. In this talk I will review the observational signatures of the formation of new objects, the instruments available, and some of the new instruments under development to do this science. One of these new instruments, the Herschel Space Observatory was launched in May of 2009 - containing a significant piece of Waterloo hardware!
Today Phil explains how telescopes work and offers up some astronomical shopping advice. -- How Telescopes Work 1:07 Refractors vs Reflectors 2:50 Technology and the Light Spectrum 7:45 -- PBS Digital Studios: http://youtube.com/pbsdigitalstudios Follow Phil on Twitter: https://twitter.com/badastronomer Want to find Crash Course elsewhere on the internet? Facebook - http://www.facebook.com/YouTubeCrashCourse Twitter - http://www.twitter.com/TheCrashCourse Tumblr - http://thecrashcourse.tumblr.com Support CrashCourse on Subbable: http://subbable.com/crashcourse -- PHOTOS/VIDEOS http://en.wikipedia.org/wiki/Galileo_Galilei#mediaviewer/File:Justus_Sustermans_-_Portrait_of_Galileo_Galilei,_1636.jpg http://en.wikipedia.org/wiki/Human_eye#mediaviewer/File:Human_eye_with_blood_vessels.jp...
Episode 3 of 5 Check us out on iTunes! http://testtube.com/podcast Please Subscribe! http://testu.be/1FjtHn5 The amount of the electromagnetic spectrum that humans can perceive is extremely small. So to see the rest we built telescopes that could see it all. But how do they work? + + + + + + + + Previous Episode: Galileo Didn't Invent The Telescope... Sorry.: https://www.youtube.com/watch?v=FVdmHxZE3hM&list;=PLwwOk5fvpuuJrG-gYpuz_qqcVZrIXgR2z&index;=2 + + + + + + + + Sources: The Electromagnetic Spectrum: http://imagine.gsfc.nasa.gov/science/toolbox/emspectrum1.html "The electromagnetic (EM) spectrum is the range of all types of EM radiation. Radiation is energy that travels and spreads out as it goes - the visible light that comes from a lamp in your house an...
Over the last 2 months me and my friend Artem (you met him in the last video) built our first radio telescope. It was built mostly out of off the shelf components, like a satellite dish and Ku band LNB, as well as some parts we 3d printed. When all was said and done we had a system that could not only take images of the sky in radip frequencies (in this case 10-12ghz), but could also be used to track satellites. With it, we were able to see the ring of satellites in geosynchronous orbit, over 35,000km away, This is only the first of what I suspect will be many more telescopes like this. Next time we'll be building ones that are far larger and can see things like the hydrogen lines so we can image the milky way. If you enjoyed this video and would like to support the continued production o...
Most telescopes in the world work at visible light wavelengths because this is where stars shine the brightest. However in those places where new objects (e.g. planets, stars, and galaxies) are being born the light is emitted at much longer wavelengths. Thus, to observe the births of new objects requires instrumentation in the far-infrared and submillimeter. Facilities at these wavelengths are either recently built or still under development. In this talk I will review the observational signatures of the formation of new objects, the instruments available, and some of the new instruments under development to do this science. One of these new instruments, the Herschel Space Observatory was launched in May of 2009 - containing a significant piece of Waterloo hardware!
Full podcast episodes: http://www.askaspaceman.com Support: http://www.patreon.com/pmsutter Follow: http://www.twitter.com/PaulMattSutter and http://www.facebook.com/PaulMattSutter How do we make observations beyond visible light? What exactly is a telescope? And what’s up with NASA adding colors to images? I discuss these questions and more in today’s Ask a Spaceman! Support the show: http://www.patreon.com/pmsutter All episodes: http://www.AskASpaceman.com Follow on Twitter: http://www.twitter.com/PaulMattSutter Like on Facebook: http://www.facebook.com/PaulMattSutter Watch on YouTube: http://www.youtube.com/c/PaulMattSutter Keep those questions about space, science, astronomy, astrophysics, physics, and cosmology coming to #AskASpaceman for COMPLETE KNOWLEDGE OF TIME AND SPACE! Bi...
The answers to some of the universe's greatest mysteries are being beamed through the night sky in light we can't see with human eyes ... but it won't be invisible to us forever. Explore the wonder of infrared astronomy and the promise of the upcoming Webb Space Telescope through the technological wizardry of paper cutouts. Informs you faster and guaranteed to contain 100 percent more llamas than any astronomy video ever produced before! To learn more about this video and infrared astronomy, visit http://webbtelescope.org/go/beyond To learn more about the Webb Space Telescope, visit http://webbtelescope.org/ Interested in finding out more about Webb's science? Try here: http://webbtelescope.org/webb_telescope/science_on_the_edge/ Curious about the technology that goes into the telescop...
This 5-minute, 30-second video shows the four U.S. educators who flew on the Stratospheric Observatory for Infrared Astronomy (SOFIA) on Nov. 3, 2015 as Airborne Astronomy Ambassadors (AAA). Flying on SOFIA as Airborne Astronomy Ambassadors lets teachers experience world-class astronomy first-hand, and gives them tools to inspire their students to pursue careers in Science, Technology, Engineering, & Math (STEM). SOFIA is a partnership between NASA and the German Aerospace Center (DLR). The SOFIA aircraft, a 747SP, is operated by NASA's Armstrong Flight Research Center and is based at Hangar 703 in Palmdale, CA. For more information on SOFIA visit: http://www.nasa.gov/mission_pages/SOFIA/index.html
Visit my website at http://www.junglejoel.com - this is a closer look at a huge new master image of the central parts of the Milky Way -made from thousands of smaller images, taken by ESO's VISTA telescope at Paranal, Chile. In the video we see a comparison of visible and infrared views. VISTA's infrared camera can see through much of the dust blocking the view in visible light, although the more opaque dust filaments still show up in this picture. Please rate and comment, thanks! Video Credits: ESO/VVV Consortium/Nick Risinger (skysurvey.org) Music: Delmo -- Acoustic (disasterpeace.com) Acknowledgement: Ignacio Toledo
Most telescopes in the world work at visible light wavelengths because this is where stars shine the brightest. However in those places where new objects (e.g. planets, stars, and galaxies) are being born the light is emitted at much longer wavelengths. Thus, to observe the births of new objects requires instrumentation in the far-infrared and submillimeter. Facilities at these wavelengths are either recently built or still under development. In this talk I will review the observational signatures of the formation of new objects, the instruments available, and some of the new instruments under development to do this science. One of these new instruments, the Herschel Space Observatory was launched in May of 2009 - containing a significant piece of Waterloo hardware!
Infrared astronomy Infrared astronomy is the branch of astronomy and astrophysics that studies astronomical objects visible in infrared (IR) radiation.The wavelength of infrared light ranges from 0.75 to 300 micrometers. =======Image-Copyright-Info======== License: Creative Commons Attribution 4.0 (CC BY 4.0) LicenseLink: http://creativecommons.org/licenses/by/4.0 Author-Info: ESO/B. Tafreshi Image Source: https://en.wikipedia.org/wiki/File:Wrapped_Up_for_the_Cool_Cosmos.jpg =======Image-Copyright-Info======== -Video is targeted to blind users Attribution: Article text available under CC-BY-SA image source in video https://www.youtube.com/watch?v=_aj_YEk9Wy4
The bigger the collector, more light telescope can gather. Ultraviolet telescopes, and x ray telescopes. Optical their development over the years has seen a steady increase in size for one simple, but very important, reason large telescopes can gather and focus more this absorption is particular problem nonoptical radiation because glass opaque to (that is, it blocks completely) much of infrared ultraviolet regions 11 may 2016 its life ukirt evolved from an almost 'do yourself' light bucket operated by half dozen astronomers armed with voltmeters screwdrivers stfc astronomy now on vista, visible survey telescope astronomy, which european 13 2011 spitzer space (formerly sirtf, facility) designed take pictures universe at wavelengths beyond what human eye see. But that's not the biggest chal...
As the world's largest flying observatory, NASA's Stratospheric Observatory for Infrared Astronomy, or SOFIA, is a unique space-science asset. SOFIA incorporates a 19-ton German-built telescope with an effective diameter of 2.5 meters in a highly modified Boeing 747SP aircraft that flies astronomical science missions at altitudes between 39,000 and 45,000 feet, above 99 percent of the infrared-blocking water vapor in the atmosphere. Capable of conducting observations in visible through far-infrared spectra from any part of the globe, SOFIA provides access to a spectral region not currently accessible by ground or space telescopes. A joint program of NASA and the German Aerospace Center DLR, the SOFIA observatory is based at NASA's Science and Aircraft Integration Facility in Palmdale, Ca...
Infrared light is all around us even though we cannot see it. Find out how this invisible radiation impacts our everyday lives. Everything Scientists Could Learn By Looking At Your Skull - https://youtu.be/PtG9uB5C7Sk Sign Up For The Seeker Newsletter Here - http://bit.ly/1UO1PxI Read More: What Are Redshift and Blueshift? http://www.space.com/25732-redshift-blueshift.html What Wavelength Goes With a Color? https://science-edu.larc.nasa.gov/EDDOCS/Wavelengths_for_Colors.html#invisible Infrared Telescopes http://www.astro.caltech.edu/~george/ay20/ir-telescopes.pdf Infrared Astronomical Satellite - https://www.jpl.nasa.gov/missions/infrared-astronomical-satellite-iras/ High-performance near-infrared imaging for breast cancer detection - https://www.ncbi.nlm.ni...
A team from NASA's Goddard Space Flight Center in Greenbelt, Maryland, is developing a new, third-generation facility science instrument for the Stratospheric Observatory for Infrared Astronomy, SOFIA. The High Resolution Mid-InfrarEd Spectrometer (HIRMES), is a spectrometer optimized to detect neutral atomic oxygen, water, as well as normal and deuterated (or "heavy") hydrogen molecules at infrared wavelengths between 25 and 122 microns (a micron is one-millionth of a meter). These wavelengths are key to determining how water vapor, ice, and oxygen combine at different times during planet formation, and will enable new observations of how these elements combine with dust to form the mass that may one day become a planet. HIRMES will provide scientists with a unique opportunity to study ...
The James Webb Space Telescope will continue to revolutionize our study of the cosmos. Slated for launch in late 2018, Webb will look deeper than either the Hubble or Spitzer Space Telescopes at infrared wavelengths. This talk will describe Webb as a whole, with a focus on the Mid-Infrared Instrument —— a partnership between JPL and a consortium of European astronomical institutes. Speaker: Michael Ressler U.S. MIRI Project Scientist, JPL
Host: Gary Melnick Speaker: David Neufeld (Johns Hopkins University) Observations at far- and mid-infrared wavelengths provide a wealth of information about the molecular inventory of interstellar gas clouds. Because of the different chemical pathways responsible for their formation and destruction, different molecules probe specific aspects of the interstellar environment. Carefully interpreted, they provide unique information about the molecular fraction, the UV radiation field, the dissipation of energy within the turbulent ISM, and the cosmic-ray density in the Galaxy. This talk will include a general overview of astrochemical probes of the interstellar medium, along with new estimates of a key parameter in astrochemical models: the cosmic-ray ionization rate. Observations at far- a...
The World of PANDORA - Life After Earth http://www.advexon.com Pandora is the idyllic blue world featured in the movie Avatar. Its location is a real place: Alpha Centauri, the nearest star to our Sun and the most likely destination for our first journey beyond the solar system. Remarkably, it's anti-matter, the science fiction fuel of choice that could take us there. Normally, it's only created in powerful jets that roar out of black holes. We can now produce small quantities in Earth-bound particle colliders. Will we journey out only to plunder other worlds? Or will we come in peace? The answer may depend on how we see Earth at that time in the distant future. The year is 2154. Our planet has been ruined by environmental catastrophe. In the movie Avatar, greedy prospectors from Earth d...
If you don't have a star tracker, here's what I've so far found the best way to take deep space astrophotography photos. You'll do better with a good tracker, but I got some good results without one. http://forrest-tanaka.com/ Exposure information: Focal length: 280mm Aperture: f/4.0 ISO: 6400 Shutter: 1.6s
The Herschel satellite observed a large fraction of the Far Infrared sky. This video displays our Galaxy, the Milky Way, as seen in the 70 micron (blue) and 160 micron (red) PACS bands. Numbers at the top indicate the camera position in galactic coordinates. The data was processed using the JScanam data reduction pipeline and it's available for download at a dedicated ESA webpage: http://archives.esac.esa.int/hsa/legacy/HPDP/PACS/PACS-P/JScanam/ Music: Almost in F - Tranquillity by Kevin MacLeod http://incompetech.com/music/royalty-free/index.html?isrc=USUAN1100394
In her public lecture at Perimeter on March 1, 2017, Dr. Amber Straughn of NASA provided a behind-the-scenes look at the James Webb Space Telescope. Watch more Perimeter public lectures: https://insidetheperimeter.ca/discover/public-lectures/
Want to start capturing Infrared, Full Spectrum, or Ultraviolet Photos? But you also want to be able to use the same camera for "normal" visible spectrum pics? Easy. You'll need a Sony DSC-F717 and a special rare earth Neodymium magnet. This hack also works for the F707 and the F828. The special rare earth magnet enables you to temporarily convert the Sony from a normal camera into a full spectrum powerhouse, in seconds! The best magnet to use is a Neodymium rare earth magnet: 3/8" x 1" grade N52 cylinder shape. Any other size would be a trial and error approach. However be cautious to use a magnet that is too powerful because it could damage the internals of the camera. On eBay the seller 1960galaxy sells the exact perfect size magnet for under $10 shipped. This method allows you to ...
EU2017: Future Science -- Rebroadcast—only $29: https://www.electricuniverse.live In Part 1 of this presentation, physicist Wal Thornhill began his discussion on the electrical nature of stars with an examination of pulsars – electromagnetic, pulsing signals in space which astronomers attribute to so-called neutron stars. In this episode, Thornhill offers an in-depth juxtaposition of the standard theory of stars versus that of the Electric Universe model. Note: This series had previously been announced as a three-parter, but was adjusted to two-parts for continuity reasons. Electric Stars in Focus: https://www.youtube.com/watch?v=aemwD0SW0Y0&t;=618s If you see a CC with this video, it means that subtitles are available. To find out which ones, click on the Gear Icon in the lower right...
Can we find stellar civilizations by looking for their waste heat? New research suggests that it is possible, and practical. Earth-like civilizations generate heat from the energy that they utilize. The thermal radiation from this heat can be a thermodynamic marker for civilizations. Here we model such planetary radiation on Earth-like planets and propose a strategy for detecting such an alien unintentional thermodynamic electromagnetic biomarker. Astronomical infrared (IR) civilization biomarkers may be detected within an interestingly large cosmic volume using a 70 m-class or larger telescope. In particular, the Colossus telescope with achievable coronagraphic and adaptive optics performance may reveal Earth-like civilizations from visible and IR photometry timeseries’ taken during ...
November 21, 2013 From Nano to Cosmo: Nanoscale Superconductivity Used to Detect Faint Far-Infrared Astronomical Signals Guest Speaker: Prof. Teun Klapwijk, The Kavli Institute of Nanoscience at Delft University of Technology, Netherlands Abstract: Superconductivity is a phenomenon, which is very well suited for interactions with far-infrared radiation. This part of the electromagnetic spectrum is very important to gather information about processes in the ‘cool universe’. It is largely masked by the absorption in the earth’s atmosphere. Superconducting devices have been developed capable of measuring the detailed chemistry of the interstellar gas using the Herschel Space telescope and more recently with the Atacama Large Millimeter Array. In considering future astronomical goals it has...
WISE, the Wide-field Infrared Survey Explorer, surveyed the entire sky in 4 mid-infrared bands at 3.4, 4.6, 12 and 22 microns with vastly greater sensitivity than previous all-sky surveys at these wavelengths. WISE surveyed everything more than 1 AU from the Sun including asteroids, comets, nearby brown dwarfs and star forming regions both in the Milky Way and in distant galaxies. The 12 and 22 micron channels were very powerful for detecting Ultra-Luminous Infrared Galaxies, and WISE has detected some of the most luminous galaxies in the Universe. The WISE short wavelength channels are very powerful for detecting old cold brown dwarfs, and WISE has detected objects as cool as 250 K, and the 3rd and 4th closest stellar systems to the Sun. WISE reported 3.75 million asteroid observations to...
This episode is an in-depth look at stars, from the common kinds and basic terminology to exotic stars, some which are entirely hypothetical. We'll look at Stars bigger than solar systems or tinier than a pinhead, and some stars that no longer exist or cannot exist till long after all other stars have died. Visit our Website: http://www.isaacarthur.net Join the Facebook Group: https://www.facebook.com/groups/1583992725237264/ Support the Channel on Patreon: https://www.patreon.com/IsaacArthur Visit the sub-reddit: https://www.reddit.com/r/IsaacArthur/ Listen or Download the audio of this episode from Soundcloud: https://soundcloud.com/isaac-arthur-148927746/the-stellar-compendium Cover Art by Jakub Grygier: https://www.artstation.com/artist/jakub_grygier
You can help support SpaceTime too, by becoming a patron...and we have rewards for you. Do your bit to keep Stuart fed and housed... details at our Patreon page... https://www.patreon.com/spacetimewithstuartgary Stream episodes on demand from www.bitesz.com (mobile friendly) *Lunar water more common than thought There could be a lot more water on the Moon than previously thought. New Satellite readings indicate that numerous volcanic deposits spread across the lunar surface contain unusually high amounts of water compared with surrounding terrains. The findings mean there could be as much water in the lunar mantle was what there is in mantle basalts on Earth. *Dark Matter more likely to be cold rather than fuzzy Scientists trying understand dark matter now believe it’s far more likely ...
Astronomers at the University of California at Irvine (UCI) and the Space Telescope Science Institute have made the most accurate statistical estimate of the number of faint, small galaxies that existed only 500 million years after the big bang. This was culled from an analysis of the deepest Hubble Space Telescope sky survey, CANDELS (Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey). Previously, studies using Caltech's CIBER (the Cosmic Infrared Background Experiment) rocket-borne instrument and NASA's Spitzer Space Telescope images confirmed the presence of "intra-halo light" from stars distributed outside of galaxies. The Hubble data found a new component in the infrared background in addition to intra-halo light — the collective glow of entire galaxies that formed firs...
Karl M. Menten, Max-Planck
Text at http://howfarawayisit.com/documents/ Planetary nebula, such as NGC 2371, and supernova remnants, such as SN 0509, form when stars die. In this segment of our "How far away is it" video book, we'll cover the nebula associated with stars being born. We begin by showing the three kinds of nebula: Reflective like the Witch Head Nebula, emission like the Rosetta Nebula NGC 2237 along with a discretion of H II Regions, and dark nebula like the Horsehead Nebula shown in visible and infrared light. We then begin a tour of some of the most spectacular star birth nebula across the Milky Way including: Rho Ophiuchi; the Blue Horsehead Nebula; R Coronae Australis, with its Herbig--Haro objects; the Iris Nebula, NGC 7023; the Great Orinon Molecular Cloud behind Minitaka, Alnilam, and Alnitak...
The Grubb Parsons Lecture 2012 was delivered by Professor Matt Griffin.
Distant Quasars & Pandora's Cluster - Episode 7 of Astronomy: Secrets of the Universe Revealed Segment 1: Most Distant Quasar Found [5:11] This ESOcast is about the discovery of the most distant quasar found to date. This brilliant beacon is powered by a black hole with a mass two billion times that of the Sun. It is by far the brightest object yet discovered in the early Universe. Credit: ESO. Visual design and editing: Martin Kornmesser and Luis Calçada. Editing: Herbert Zodet. Web and technical support: Lars Holm Nielsen and Raquel Yumi Shida. Written by: Sarah Roberts and Richard Hook. Narration: Dr. J. Music: Movetwo and John Dyson (from the album Darklight). Footage and photos: ESO, A. M. Swinbank and S. Zieleniewski, Stéphane Guisard http://www.eso.org/~sguisard and José Francis...
The Galactic Center Group at UCLA has used the W. M. Keck Observatory for the past two decades to observe the center of the Milky Way at the highest angular resolution possible. This work established the existence of a supermassive black hole at the heart of our Galaxy. In this talk, Dr. Leo Meyer, Research Scientist for the UCLA Galactic Center Group, will focus on the black hole itself and the gas that it swallows. The feeding of the black hole is a turbulent process resulting in highly variable emission of infrared light. Observations of this variability provide a great way to learn about the black hole and its immediate environment.
Observations at far- and mid-infrared wavelengths provide a wealth of information about the molecular inventory of interstellar gas clouds. Because of the different chemical pathways responsible for their formation and destruction, different molecules probe specific aspects of the interstellar environment. Carefully interpreted, they provide unique information about the molecular fraction, the UV radiation field, the dissipation of energy within the turbulent ISM, and the cosmic-ray density in the Galaxy. This talk will include a general overview of astrochemical probes of the interstellar medium, along with new estimates of a key parameter in astrochemical models: the cosmic-ray ionization rate.