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Phil Plait
Philip Cary Plait (born September 30, 1964), also known as The Bad Astronomer, is an American astronomer, skeptic, and popular science blogger. Plait has worked as part of the Hubble Space Telescope team, images and spectra of astronomical objects, as well as engaging in public outreach advocacy for NASA missions. He has written three books, '' Bad Astronomy'', '' Death from the Skies'', and '' Under Alien Skies''. He has also appeared in several science documentaries, including '' How the Universe Works'' on the Discovery Channel. From August 2008 through 2009, he served as president of the James Randi Educational Foundation. Additionally, he wrote and hosted episodes of '' Crash Course'' Astronomy, which aired its last episode in 2016. Early life Plait grew up in the Washington, D.C. area. He has said he became interested in astronomy when his father brought home a telescope when Plait was 5 years old or so. According to Plait, he "aimed it at Saturn that night. One look, an ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
The Amazing Meeting
The Amazing Meeting (TAM), stylized as The Amaz!ng Meeting, was an annual conference that focused on science, scientific skepticism, skepticism, and critical thinking; it was held for twelve years. The conference started in 2003 and was sponsored by the James Randi Educational Foundation (JREF). Perennial speakers included Penn & Teller, Phil Plait, Michael Shermer and James Randi, James "The Amazing" Randi. Speakers at the four-day conference were selected from a variety of disciplines including scientific educators, magicians, and community activists. Outside the plenary sessions the conference included workshops, additional panel discussions, music and magic performances and live taping of podcasts including ''The Skeptics' Guide to the Universe''. The final Amazing Meeting was held in July 2015. History and organization TAM was first held in 2003, attracting around 150 attendees. When the Committee for Skeptical Inquiry, CSICOP conferences entered a seven-year hiatus in 2005, T ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Crash Course (YouTube)
''Crash Course'' (sometimes stylized as ''CrashCourse'') is an educational YouTube channel started by John Green and Hank Green (collectively the Green brothers), who became known on YouTube through their '' Vlogbrothers'' channel. ''Crash Course'' was one of the hundred initial channels funded by YouTube's $100 million original channel initiative. The channel launched a preview on December 2, 2011, and , it has accumulated over 16 million subscribers and 1.8 billion video views. The channel launched with John and Hank presenting their respective '' World History'' and ''Biology'' series; the early history of the channel continued the trend of John and Hank presenting humanities and science courses, respectively. In November 2014, Hank announced a partnership with PBS Digital Studios, which would allow the channel to produce more courses. As a result, multiple additional hosts joined the show to increase the number of concurrent series. To date, there are 44 main ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Astronomy And Astrophysics
''Astronomy & Astrophysics (A&A)'' is a monthly peer-reviewed scientific journal covering theoretical, observational, and instrumental astronomy and astrophysics. It is operated by an editorial team under the supervision of a board of directors representing 27 sponsoring countries plus a representative of the European Southern Observatory. The journal is published by EDP Sciences and the current editors-in-chief are Thierry Forveille and João Alves. History Origins ''Astronomy & Astrophysics'' was created as an answer to the publishing situation found in Europe in the 1960s. At that time, multiple journals were being published in several countries around the continent. These journals usually had a limited number of subscribers, and articles were written in languages other than English. They were less widely read than American and British journals and the research they reported had therefore less impact in the community. Starting in 1963, conversations between astronomers from ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Herbig Ae/Be Star
A Herbig Ae/Be star (HAeBe) is a pre-main-sequence star – a young () star of spectral types A or B. These stars are still embedded in gas-dust envelopes and are sometimes accompanied by circumstellar disks. Hydrogen and calcium emission lines are observed in their spectra. They are 2-8 Solar mass () objects, still existing in the star formation (gravitational contraction) stage and approaching the main sequence (i.e. they are not burning hydrogen in their center). Description In the Hertzsprung–Russell diagram, Herbig Ae/Be stars are located to the right of the main sequence. They are named after the American astronomer George Herbig, who first distinguished them from other stars in 1960. The original Herbig criteria were: * Spectral type earlier than F0 (in order to exclude T Tauri stars), * Balmer emission lines in the stellar spectrum (in order to be similar to T Tauri stars), * Projected location within the boundaries of a dark interstellar cloud (in order to select ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
HD 163296
HD 163296 is a young Herbig Ae/Be star, Herbig Ae star surrounded by a protoplanetary disk. The disk is a popular target to study disk composition, and several works suggested the presence of Protoplanet, protoplanets inside the gaps of the disk. The star HD 163296 was first identified in the Henry Draper Catalogue. The star was first identified to have peculiar hydrogen emission lines in 1925, based on observations with the Mount Wilson Observatory by Paul W. Merrill, Milton L. Humason and Cora G. Burwell. The star was classified as having a spectral type of A2e. In 1984, it was first considered that HD 163296 is a Herbig Ae star due to the H-alpha and NaD lines having a P Cygni profile. The status as a Herbig Ae star was questioned at the time. It was, however concluded that it is surrounded by a dust shell from near-infrared excess. Later in 1989, it was found that magnesium and calcium lines have short-term variability from observations with the International Ultravi ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
AB Aurigae
AB Aurigae is a young Herbig Ae/Be star, Herbig Ae star in the Auriga (constellation), Auriga constellation. It is located at a distance of approximately 509 light years from the Sun based on stellar parallax. This pre-main-sequence star has a stellar classification of A0Ve, matching an A-type main-sequence star with emission lines in the stellar spectrum, spectrum. It has 2.4 times the mass of the Sun and is radiating 38 times the Sun's luminosity from its photosphere at an effective temperature of 9,772 K. The radio emission from the system suggests the presence of a thermal jet originating from the star with a velocity of . This is causing an estimated mass loss of . Mary Doris Applegate Beach discovered that AB Aurigae is a variable star by examining 150 photographic plates taken between 1914 and 1921. Her discovery was announced in 1921. This star is known for hosting a dust disk that harbour a massive protoplanet or proto-brown dwarf. The star is part of ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Reports On Progress In Physics
''Reports on Progress in Physics'' is a peer reviewed journal published by IOP Publishing. The editor-in-chief as of 2022 is Subir Sachdev (Harvard University Harvard University is a Private university, private Ivy League research university in Cambridge, Massachusetts, United States. Founded in 1636 and named for its first benefactor, the History of the Puritans in North America, Puritan clergyma ...). Abstracting and indexing ''Reports on Progress in Physics'' is abstracted and indexed in the following databases: IOP. 2010 References External links * {{Institute of Physics, state=collapsed IOP Publishing academic journals[...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
The Astrophysical Journal
''The Astrophysical Journal'' (''ApJ'') is a peer-reviewed scientific journal of astrophysics and astronomy, established in 1895 by American astronomers George Ellery Hale and James Edward Keeler. The journal discontinued its print edition and became an electronic-only journal in 2015. Since 1953, ''The Astrophysical Journal Supplement Series'' (''ApJS'') has been published in conjunction with ''The Astrophysical Journal'', with generally longer articles to supplement the material in the journal. It publishes six volumes per year, with two 280-page issues per volume. ''The Astrophysical Journal Letters'' (''ApJL''), established in 1967 by Subrahmanyan Chandrasekhar as Part 2 of ''The Astrophysical Journal'', is now a separate journal focusing on the rapid publication of high-impact astronomical research. The three journals were published by the University of Chicago Press for the American Astronomical Society until, in January 2009, publication was transferred to IOP Publis ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Space Telescope Imaging Spectrograph
The Space Telescope Imaging Spectrograph (STIS) is a spectrograph, also with a camera mode, installed on the Hubble Space Telescope. Aerospace engineer Bruce Woodgate of the Goddard Space Flight Center was the principal investigator and creator of the STIS. It operated continuously from 1997 until a power supply failure in August 2004. After repairs, it began operating again in 2009. The spectrograph has made many important observations, including the first spectrum of the Celestial body atmosphere, atmosphere of an extrasolar planet, HD 209458b. The STIS was installed on Hubble in 1997 during its second servicing mission (STS-82) by Mark C. Lee, Mark Lee and Steven Smith (astronaut), Steven Smith, replacing the High Resolution Spectrograph and the Faint Object Spectrograph. It was designed to operate for five years. On August 3, 2004, an electronic failure rendered STIS inoperable, ending its use 2 years beyond its predicted lifespan. In order to bring it back to operational ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Goddard Space Flight Center
The Goddard Space Flight Center (GSFC) is a major NASA space research laboratory located approximately northeast of Washington, D.C., in Greenbelt, Maryland, United States. Established on May 1, 1959, as NASA's first space flight center, GSFC employs about 10,000 civil servants and contractors. Named for American rocket propulsion pioneer Robert H. Goddard, it is one of ten major NASA field centers. GSFC is partially within the former Goddard, Maryland, Goddard census-designated place; it has a Greenbelt, Maryland, Greenbelt mailing address.CENSUS 2000 BLOCK MAP: GODDARD CDP (PDF). U.S. Census Bureau. Retrieved September 1, 2018. 1990 Census map of Prince George's County [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Hubble Space Telescope
The Hubble Space Telescope (HST or Hubble) is a space telescope that was launched into low Earth orbit in 1990 and remains in operation. It was not the Orbiting Solar Observatory, first space telescope, but it is one of the largest and most versatile, renowned as a vital research tool and as a public relations boon for astronomy. The Hubble Space Telescope is named after astronomer Edwin Hubble and is one of NASA's Great Observatories program, Great Observatories. The Space Telescope Science Institute (STScI) selects Hubble's targets and processes the resulting data, while the Goddard Space Flight Center (GSFC) controls the spacecraft. Hubble features a mirror, and its five main instruments observe in the ultraviolet, visible spectrum, visible, and near-infrared regions of the electromagnetic spectrum. Hubble's orbit outside the distortion of atmosphere of Earth, Earth's atmosphere allows it to capture extremely high-resolution images with substantially lower background lig ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Cosmic Background Explorer
The Cosmic Background Explorer (COBE ), also referred to as Explorer 66, was a NASA satellite dedicated to cosmology, which operated from 1989 to 1993. Its goals were to investigate the cosmic microwave background radiation (CMB or CMBR) of the universe and provide measurements that would help shape the understanding of the cosmos. COBE's measurements provided two key pieces of evidence that supported the Big Bang theory of the universe: that the CMB has a near-perfect black-body spectrum, and that it has very faint anisotropies. Two of COBE's principal investigators, George F. Smoot III and John C. Mather, received the Nobel Prize in Physics in 2006 for their work on the project. According to the Nobel Prize committee, "the COBE project can also be regarded as the starting point for cosmology as a precision science". COBE was the second cosmic microwave background satellite, following RELIKT-1, and was followed by two more advanced spacecraft: the Wilkinson Microwave Ani ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
