Not exact matches
They glimpsed the image
with the Visible and
Infrared Survey Telescope for
Astronomy, or VISTA telescope, the European Southern Observatory reported today.
Among the beneficiaries would be scientists involved
with the Stratospheric Observatory for
Infrared Astronomy (SOFIA), a joint mission between NASA and Germany's space agency.
With a new lease on life, the Stratospheric Observatory for Infrared Astronomy (SOFIA) also continues to be funded, with $ 85 million for operati
With a new lease on life, the Stratospheric Observatory for
Infrared Astronomy (SOFIA) also continues to be funded,
with $ 85 million for operati
with $ 85 million for operations.
Modern
astronomy has moved light years ahead
with the opening up to observation of new parts of the electromagnetic spectrum, from
infrared (the Spitzer Space Telescope, launched in 2003) to gamma (the Integral Space Observatory, launched in 2002).
One surprise is the administration request for the Stratospheric Observatory for
Infrared Astronomy (SOFIA), a joint mission
with the German space agency that consists of a converted 747 jet
with a telescope riding in the rear.
With Falcon Heavy's additional lift, researchers planning the Large UV Optical Infrared Surveyor telescope, a proposed mission for the 2020s with a mirror at least 9 meters across, could focus less on reducing weight and more on delivering a great scientific instrument, says Matt Mountain, president of the Association of Universities for Research in Astronomy in Washington, D.C. «If we don't have to fight for mass, the testing is greatly simplified and you can launch more ambitious systems.&ra
With Falcon Heavy's additional lift, researchers planning the Large UV Optical
Infrared Surveyor telescope, a proposed mission for the 2020s
with a mirror at least 9 meters across, could focus less on reducing weight and more on delivering a great scientific instrument, says Matt Mountain, president of the Association of Universities for Research in Astronomy in Washington, D.C. «If we don't have to fight for mass, the testing is greatly simplified and you can launch more ambitious systems.&ra
with a mirror at least 9 meters across, could focus less on reducing weight and more on delivering a great scientific instrument, says Matt Mountain, president of the Association of Universities for Research in
Astronomy in Washington, D.C. «If we don't have to fight for mass, the testing is greatly simplified and you can launch more ambitious systems.»
From left, Terry Herter, principal investigator of FORCAST, and SOFIA staff scientist James De Buizer discuss an
infrared image
with Airborne
Astronomy Ambassadors Theresa Paulsen and Marita Beard.
It's called optical SETI, and its instruments are focused on a different band of the light spectrum than radio
astronomy, looking instead at the same waves our eyes take in, along
with infrared frequencies, which are just a smidge longer.
The Airborne
Astronomy Ambassadors project is aimed to measurably enhance student STEM engagement and achievement in selected school districts via professional development for teachers consisting of: (1) STEM Professional Development in astrophysics and planetary science delivered via webinars & in - person workshops; (2) a week - long STEM immersion experience at NASA's science research aircraft facility in Palmdale, California, including participation in research flights on the Stratospheric Observatory for
Infrared Astronomy (SOFIA); (3) follow - through involving continuing webinars fostering reflection and connections
with astrophysics & planetary science subject matter experts.
This work used the Immersion Grating
INfrared Spectrometer (IGRINS), developed under a collaboration between the University of Texas at Austin and the Korea
Astronomy and Space Science Institute (KASI)
with the financial support of the US National Science Foundation (NSF grant AST - 1229522) to the University of Texas at Austin, and the Korean GMT Project of KASI.
We present a detailed description of our data... ▽ More Here we report on the first successful exoplanet transit observation
with the Stratospheric Observatory for
Infrared Astronomy (SOFIA).
Abstract: Here we report on the first successful exoplanet transit observation
with the Stratospheric Observatory for
Infrared Astronomy (SOFIA).
This illustration represents the fainter disk inferred from 2016 data was collected
with the Stratospheric Observatory for
Infrared Astronomy (SOFIA).
* Because of their involvement
with the NRC's U.S. Ground - Based Optical and
Infrared (OIR)
Astronomy System study, Debra Elmegreen (Chair of the OIR study committee and Chair of the AAS Committee on
Astronomy and Public Policy), Lynne Hillenbrand (member of the OIR study committee and of the AAS Committee on
Astronomy and Public Policy), and Joel Parriott (consultant to the OIR study committee and AAS Director of Public Policy) all recused themselves from the issuance of this statement.
Notwithstanding the constrained funding environment today, we encourage AST to use the report to advocate for additional resources and to partner
with non-federal U.S. observatories to vigorously pursue this compelling ground - based optical /
infrared astronomy program.
This view combines the sharp imaging of the Hubble Space Telescope's Near
Infrared Camera and Multi-Object Spectrometer (NICMOS)
with color imagery from a previous Spitzer Space Telescope survey done
with its
Infrared Astronomy Camera (IRAC).
How to find ET
with infrared light, Kuhn, J.R., Berdyugina, S.V., Halliday, D., Harlingten, C.,
Astronomy, June issue, pp. 30 - 35 (2013) PDF Download
With this exceptional leap in performance, new domains in
infrared astronomy will become accessible, allowing us, for example, to unravel definitively galaxy evolution and metal production over cosmic time, to study dust formation and evolution from very early epochs onwards, and to trace the formation history of planetary systems.
Wiki: Near -
infrared, Short - wavelength infrared, Mid-wavelength infrared, Long - wavelength infrared, and finally Far infrared http://en.wikipedia.org/wiki/Infrared But not every classifies them the same way, continuing with wiki: Near Infrared NIR 0.78 — 3 µm Mid Infrared MIR 3 — 50 µm Far Infrared FIR 50 — 1000 µm And: Astronomy divisio
infrared, Short - wavelength
infrared, Mid-wavelength infrared, Long - wavelength infrared, and finally Far infrared http://en.wikipedia.org/wiki/Infrared But not every classifies them the same way, continuing with wiki: Near Infrared NIR 0.78 — 3 µm Mid Infrared MIR 3 — 50 µm Far Infrared FIR 50 — 1000 µm And: Astronomy divisio
infrared, Mid-wavelength
infrared, Long - wavelength infrared, and finally Far infrared http://en.wikipedia.org/wiki/Infrared But not every classifies them the same way, continuing with wiki: Near Infrared NIR 0.78 — 3 µm Mid Infrared MIR 3 — 50 µm Far Infrared FIR 50 — 1000 µm And: Astronomy divisio
infrared, Long - wavelength
infrared, and finally Far infrared http://en.wikipedia.org/wiki/Infrared But not every classifies them the same way, continuing with wiki: Near Infrared NIR 0.78 — 3 µm Mid Infrared MIR 3 — 50 µm Far Infrared FIR 50 — 1000 µm And: Astronomy divisio
infrared, and finally Far
infrared http://en.wikipedia.org/wiki/Infrared But not every classifies them the same way, continuing with wiki: Near Infrared NIR 0.78 — 3 µm Mid Infrared MIR 3 — 50 µm Far Infrared FIR 50 — 1000 µm And: Astronomy divisio
infrared http://en.wikipedia.org/wiki/
Infrared But not every classifies them the same way, continuing with wiki: Near Infrared NIR 0.78 — 3 µm Mid Infrared MIR 3 — 50 µm Far Infrared FIR 50 — 1000 µm And: Astronomy divisio
Infrared But not every classifies them the same way, continuing
with wiki: Near
Infrared NIR 0.78 — 3 µm Mid Infrared MIR 3 — 50 µm Far Infrared FIR 50 — 1000 µm And: Astronomy divisio
Infrared NIR 0.78 — 3 µm Mid
Infrared MIR 3 — 50 µm Far Infrared FIR 50 — 1000 µm And: Astronomy divisio
Infrared MIR 3 — 50 µm Far
Infrared FIR 50 — 1000 µm And: Astronomy divisio
Infrared FIR 50 — 1000 µm And:
Astronomy division scheme