FLAT EARTH REFLECTIONS (Robert Bassano) - PHONE CALL WITH SOFIA TEAM MANAGER! Is this Hubble & Chandra Space Telescopes @ 45,000 FEET?
Dear Robert Bassano (FLAT EARTH REFLECTIONS aka PLANATE VERITAS),
Fact check = You FAIL
You made some major mistakes in your interview..
First off, you should have asked Nicholas Veronico for permission to tape and later rebroadcast the conversation. But you did not.
Because you don't understand what the ES (electromagnetic spectrum) is, when Nicholas Veronico told you that SOFIA can see further into the infra-red than the Hubble Space Telescope can, YOU INCORRECTLY TOOK THAT TO MEAN that SOFIA can see objects farther "distance" away than the HST. THAT'S YOUR FAIL.
What part of the ES you do see does not depend on distance. Rather, it depends upon what spectral range an instrument was designed and built to be able to see (detect).
As a primer - the ES (electromagnetic spectrum) is the entire range of electromagnetic radiation, which includes, in order of increasing frequency and decreasing wavelength, radio waves, microwaves, infrared radiation, visible light, ultraviolet radiation, x-rays, and gamma rays.
The visible spectrum is the small portion of the electromagnetic spectrum that is visible to the human eye. Electromagnetic radiation in this range of wavelengths is called visible light or simply light. A typical human eye will respond to wavelengths from about 390 to 700 nm. In terms of frequency, this corresponds to a band in the vicinity of 430-770 THz.
Convert nm to um - Conversion of Measurement Units
converting between nanometre and micrometre.
Convert (390 to 700 nm) to
390 nm = 0.39
700 nm = 0.70
http://www.convertunits.com/from/nm/to/um
ES (electromagnetic spectrum)
http://www.astro.wisc.edu/~kerry/pics/em.jpg
Here is the SOFIA site...
https://www.sofia.usra.edu/
The SOFIA Stratospheric Observatory for Infrared
Astronomy is actually a Boeing 747SP aircraft that flies only one of the following instruments at a time - one per flight...
EXES - Echelon-Cross -Echelle Spectrograph:
FIFI-LS - Field Imaging Far-Infrared Line Spectrometer:
FLITECAM - First Light Infrared Test Experiment CAMera:
FORCAST - Faint Object InfraRed CAmera for the SOFIA Telescope:
FPI+ - Focal Plane Imager:
GREAT - German Receiver for Astronomy at Terahertz Frequencies:
HAWC+ - High-resolution Airborne Wideband Camera:
HIPO - High-speed Imaging Photometer for Occultations
Video at..
(https://www.youtube.com/watch?v=nUJNlR4spuM)
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Update: September 14, 2020
SOFIA is not getting as much observation time as originally envisioned...
OIG: NASA’s Management of the Stratospheric Observatory for Infrared Astronomy Program
The Stratospheric Observatory for Infrared Astronomy (SOFIA) is an airborne observatory housing a 106-inch telescope mounted onboard a Boeing 747SP that makes observations from between 38,000 and 45,000 feet, putting it above 99 percent of water vapor that interferes with ground-based infrared observations. The aircraft is operated out of NASA’s Armstrong Flight Research Center in Palmdale, California, and is currently equipped with six interchangeable instruments that can be upgraded or replaced. SOFIA is used by astronomers to study astronomical objects and phenomena including star birth and death, formation of new solar systems, identification of complex molecules in space, nebulas and galaxies, and transient events like eclipses.
The SOFIA Program is a partnership between NASA—within the Science Mission Directorate’s (SMD) Astrophysics portfolio—and the German Aerospace Center and operates in cooperation with the Universities Space Research Association (USRA) and German SOFIA Institute. NASA began development of SOFIA in 1991 and the Program achieved full operational capability in 2014, 13 years behind schedule with development costs over $1 billion (more than 300 percent over the initial cost estimate). Because SOFIA has experienced ongoing operational and technical challenges and has not met science output expectations, NASA has questioned whether its $83 million in annual operating costs could be put to better use. Likewise, the President’s Budget Request has proposed terminating SOFIA on multiple occasions including most recently for fiscal year 2021. However, in the past Congress has continued to fund the Program...
(Please read this full article at the URL posted above)
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Update: April 24, 2022
Happy Birthday, Hubble (skyandtelescope.org)
https://skyandtelescope.org/astronomy-news/happy-birthday-hubble-3/
The Hubble Space Telescope turns 32 on April 24th, and the team behind the telescope is marking the occasion with the release of a galactic family picture.
Three spiral galaxies, an elliptical, and a lenticular feature in this Hubble Space Telescope image, all packed into a volume less than 200,000 light-years across, or twice the diameter of the Milky Way’s disk. Their light traveled 300 million light-years before it reached Hubble’s cameras.
At first glance, the five stunning galaxies of Hickson Compact Group 40 look disconnected, placed next to each other in space by chance superposition. But a closer look reveals connections between them, bridges made of gas and stars.
The galaxies make up one of the most crowded compact galaxy groups known, and it’s getting more crowded still. They’re falling inexorably toward each other — in about 1 billion years, there’ll be nothing to see here except for a giant elliptical fuzzball of stars.
Such compact groups might have been more common earlier in the universe’s timeline. Galactic interactions fueled the supermassive black holes that lurk in most galaxy centers and, indeed, most of the galaxies here show evidence of such a central black hole.
The image, taken late last year, was released recently in celebration of the Hubble Space Telescope’s 32nd year of operations. Hubble has far outlived its expected lifetime, having captured 1.5 million images of about 50,000 celestial objects along the way so far. HCG 40 is one more under its belt.
(Please read the article posted at the URL above)
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Visit the main NASA Hubble site here ...
https://hubblesite.org/
https://hubblesite.org/resource-gallery/images
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Posted on June 18, 2022
ROBERT BASONO BUSTED. NOW WITH THE RETIREMENT OF SOPHIA HE CAN NO LONGER CLAIM THE HUBBLE SPACE TELESCOPE DOES NOT EXIST.
Some flat Earthers have and still continue to insist, that The Hubble Space Telescope does not exist - that all those pictures attributed to Hubble are really from SOPHIA (Stratospheric Observatory for Infrared Astronomy).Well, now they can't get any more traction out of that lie, as SOPHIA is being retired and the Hubble photos keep on coming. https://www.nasa.gov/mission_pages/SOFIA/overview/index.html
USRA Closeout Statement on Sopia (spaceref.com)
http://spaceref.com/news/viewpr.html?pid=60494
Press Release From: Universities Space Research Association
Posted: Wednesday, June 15, 2022
NASA and DLR (German Space Agency) recently announced the cessation of operations of SOFIA – the Stratospheric Observatory for Infrared Astronomy--whose science mission operations are managed by Universities Space Research Association (USRA). SOFIA conducts a broad range of astrophysical and planetary science investigations using unique, state-of-the-art and far infrared capabilities to address key NASA astrophysics’ objectives.
USRA has been proud to work with NASA on SOFIA whose legacy has been remarkable.
SOFIA’s contributions to interdisciplinary science include significant achievements such as
- Finding water on the Moon
- First measurements of atomic oxygen in the Earth’s mesosphere and lower thermosphere
- Determining how magnetic fields control star formation and how magnetic fields grow and develop in galaxies. Understanding the origin, amplification and morphology of the magnetic field is crucial to forming a complete picture of Galaxy development
- Discovering that Stellar winds, not supernovae disperse molecular clouds, trigger the birth of new stars and can dominate feedback
- Discerning the dynamics of interstellar gas and feedback from stars to gas through high spectral resolution
- Detecting the helium hydride molecule, the first molecule in the Universe
- Studying the composition and evolution of the Interstellar Medium (ISM) by surveying the ISM with cameras, spectrometers, and polarimeters that operate in the near-, mid-, and far-infrared wavelengths, each suited to studying a particular phenomenon
- Studies in the infrared that highlight stellar collision
- Observing a comet with “ocean-like” water, providing hints about the origins of Earth’s oceans
- Finding out how magnetic fields can help feed active black holes
- On the other hand, finding out how magnetic fields are working to keep the Milky Way’s black hole quiet
- Helping to create a panoramic view of the Milky Way’s center – spanning a distance of 600 light-years – in infrared
- Studying how a type of organic molecule could develop in space, helping to better understand how life could have developed on Earth
- Catching a glimpse of what happens after two planets collide
- Finding the amount and location of water vapor around a protostar
- Confirming that a nearby planetary system around the star Epsilon Eridani is remarkably similar to our own solar system
- Finding that dust can not only survive, but may be formed in the wake of a supernova explosion, one of the most powerful events in the universe, whose blast destroys almost everything in its path
- Observing how stellar pulsations affect the chemistry of the universe
As far as capabilities are concerned, SOFIA offers diverse competencies like high resolution spectroscopy and Far-IR polarimetry. Studies of SOFIA’s science capabilities provide compelling synergies with other observatories in NASA’s portfolio. For example, studies of the bright nearby Universe are key to illuminating the underlying physics in the more distant objects that will be targeted by the James Webb Telescope. Balloon Missions such as GUSTO and BlastPol provide direct scientific synergy with SOFIA by performing even wider-area surveys or pathfinder science of select regions. The capabilities of these facilities complement SOFIA capabilities and offer open access to a much larger observer base.
SOFIA’s instrument suite provides continuum, spectroscopic and polarization imaging in the full mid-IR and far-IR wavelength range inaccessible from the ground. The spectral resolving power of SOFIA provides measurements not possible with any other observatory. Unlike space-based IR facilities, SOFIA’s instrument detectors don’t saturate with light even on the bright targets, many of which serve as local templates for understanding the distant universe.
SOFIA’s instruments are constantly upgraded depending on the science needs. Principal Investigator teams selected through a competitive proposal process develop the instruments. Current instruments include FORCAST and HAWC+, FIFI-LS, EXES, and GREAT. All instruments remain in high demand. FORCAST and GREAT are the most mature in the instrument suite and their observations have produced the most scientific publications.
SOFIA has doubled its annual science publications over the past three years. In first eight years after starting operations, SOFIA produced over 300 scientific papers which is significantly higher than science return from far-infrared balloon programs and at a comparable hours-per-paper as the Herschel Space Observatory, the last far-infrared space observatory.
SOFIA continues to move forward with higher productivity and greater impact till the end of its term.
USRA looks forward to partner with NASA to ensure the safe fly out of SOFIA and ensure that its science legacy is captured appropriately for the astronomical community.
For more information on SOFIA’s recent accomplishments: https://www.sofia.usra.edu/sites/default/files/2022-03/SOFIA_Status_Future_Prospects_17Mar22.pdf
SOFIA Science: Remarkable Results": https://www.sofia.usra.edu/sites/default/files/2021-11/SOFIA-Science-2021.pdf
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(Please read the article posted at the URL above)
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Published on – October 21, 2016
Discussion at - https://www.youtube.com/channel/UC7ipUKERU0tzYFxALJBli4A/discussion
Video at - https://www.youtube.com/watch?v=nUJNlR4spuM
Our home page all articles - http://flatearthlunacy.com
kind regards, JonahTheScientist
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