Infrared spectroscopy of Jupiter and Saturn

final technical report
  • 2.90 MB
  • English

National Aeronautics and Space Administration, National Technical Information Service, distributor , [Washington, DC, Springfield, Va
Albedo., Astronomical photometry., Astronomical spectroscopy., Infrared photometry., Infrared spectra., Infrared spectroscopy., Satellite atmospheres., T
StatementRoger F. Knacke.
SeriesNASA contractor report -- NASA CR-196294.
ContributionsUnited States. National Aeronautics and Space Administration.
The Physical Object
Pagination1 v.
ID Numbers
Open LibraryOL15400524M

Cite this paper as: Hunt G.E. () Spectroscopy of Jupiter and Saturn. In: McCormac B.M. (eds) Atmospheres of Earth and the Planets. Space Science Library (A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews), vol Jupiter's Atmospheric Composition from the Cassini Thermal Infrared Spectroscopy Experiment Article (PDF Available) in Science () October with Reads How we measure 'reads''s_Atmospheric_Composition.

Infrared Spectroscopy. Infrared spectroscopy is a useful tool to confirm the penetration of adsorbed molecules, such as methanol or acetone (Serna and VanScoyoc, ), into the tunnels by the shift of absorption bands associated with H2O coordinated to Mg2+ ions. From: Developments in Clay Science, Related terms: Clay Mineral; Wavelength The infrared spectrometer and radiometer for the Mariner-Jupiter-Saturn mission is described.

Results of Nimbus and Mariner 9 IR spectroscopy of earth and Mars are used as examples to demonstrate the power and diversity of the technique.

Details Infrared spectroscopy of Jupiter and Saturn FB2

Determinations of planetary surface compositions, surface temperatures, vertical temperature profiles, surface pressures, and atmospheric constituents are Infrared spectra of Jupiter and Saturn have been recorded with the two spectrometers of the Infrared Space Observatory (ISO) in –, in the – μm :// /_Infrared_Spectroscopy_of_Solar-System_Planets.

Infrared spectroscopy of Jupiter and Saturn final technical report (SuDoc NAS ) [Roger F. Knacke] on *FREE* shipping on qualifying :// Similar infrared spectrometers, without the INFRARED SPECTROSCOPY Fig.

Wooden mock-up of the infrared spectrometer and radiometer (IRIS) under construction for the Mariner - Jupiter - Saturn mission to be launched in However, since the early days of infrared astronomical spectroscopy, in the late s and early s when some of his graduate students (myself included) were developing spectrometers for use in the 10 μm atmospheric window, he also has had an interest in spectroscopy of planetary atmospheres and, in particular, the atmosphere of Jupiter Get this from a library.

Infrared spectroscopy of Jupiter and Saturn: final technical report. [Roger F Knacke; United States. National Aeronautics and Space Administration.]   mm Mak Cass @f ASImm. Baader nm pass. ADC :// The story of the Voyager space flights past Jupiter and Saturn are recounted in detail.

The pre-Voyager thinking about the nature of these planetary systems is contrasted with the new knowledge gained by the missions. Numerous photographs illustrate the ://   mm Mak Cass @f ASImm camera.

ZWO ADC. Baader nm pass. EQ6 Pro ://   Successful; reached vicinity of Jupiter on March 5, and Saturn on Novem ; returned much new information on both planets. Reference: JPL,   Older Results.

Clays on Mars. New research indicates that on a global scale, there are little if any clays on Mars.

Description Infrared spectroscopy of Jupiter and Saturn FB2

Clays are commonly found on the Earth, but the search for them on Mars has only resulted in setting upper limits that are many times lower than on ://+papers/. Fourier Transform Infrared Spectroscopy - CHAPTER 9 FOURIER TRANSFORM INFRARED SPECTROSCOPY Neen Mars, and the moon (which defines earth's atmosphere) and major planets, which include Jupiter, Saturn, Uranus, and  › 百度文库 › 互联网.

In this activity, students will build a spectrometer using basic materials to observe the light emitted and absorbed by several sources. This will be used as a model for how NASA uses spectroscopy to determine the nature of elements found on Earth and other planets. For higher grades, this activity   NEAR-INFRARED SPECTROSCOPIC STUDIES OF THE TROPOSPHERE my IR Spectroscopy Lab cohorts, Joe Montani and Ralf Timmermann, who con­ IR observations of Saturn and Jupiter from the KAO and ground Figure KAO low-resolution uncalibrated spectrum of Open Library is an initiative of the Internet Archive, a (c)(3) non-profit, building a digital library of Internet sites and other cultural artifacts in digital projects include the Wayback Machine, and ps:// Keck near-infrared observations of Saturn's E and G rings during Earth's ring plane crossing in August Icarus,– de Pater, I., + 8 co-authors, Jupiter with Baader RG (R+IR) and Astronomik (IR) and a mm telescope.

Contrast is higher in IR but the resolution sligthly better in R+IR. For Saturn. Saturn is a more complexe target.

The penetrating effect of IR plays a role as it does for Jupiter, but   The Cassini spacecraft captured this image of Saturn's aurora using infrared waves. The aurora is shown in blue, and the underlying clouds are shown in red.

These aurorae are unique because they can cover the entire pole, whereas aurorae around Earth and Jupiter are typically confined by magnetic fields to rings surrounding the magnetic :// This focus of this project was the investigation of the planets Uranus and Neptune and Saturn's moon Titan using adaptive optics imaging and spectroscopy at the meter W.M.

Keck Telescopes. These bodies share a common type of atmosphere, one that is rich in methane and has a hydrocarbon haze layer produced by methane :// A: Each atom and molecule has its own light fingerprint that, like yours, is unlike yours, this fingerprint is made of light.

Elements and compounds emit identifying sets of “colors   Jupiter as seen by the space probe is the most detailed global color portrait of Jupiter ever assembled. An atmospheric probe was released from the spacecraft in July, The probe entered the planet's atmosphere in December 7 It parachuted through km of the atmosphere, collecting data for minutes, before being crushed by the extreme pressure to which it was :// Pierre Drossart has devoted his research activity to planetology, in the field of the atmosphere of giant and terrestrial planets through infrared spectroscopy.

From ground-based infrared spectroscopy on CFHT/FTS instrument, he has obtained many results on the spectroscopy of Jupiter, including the first spectroscopic detection of H3+ on ://   Exoplanetology, or exoplanetary science, is an integrated field of astronomical science dedicated to the search for and study of exoplanets (extrasolar planets).

It employs an interdisciplinary approach which includes astrobiology, astrophysics, astronomy, astrochemistry, astrogeology, geochemistry, and planetary science Absorption spectroscopy refers to spectroscopic techniques that measure the absorption of radiation, as a function of frequency or wavelength, due to its interaction with a sample absorbs energy, i.e., photons, from the radiating field.

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The intensity of the absorption varies as a function of frequency, and this variation is the absorption   Jupiter on Päikesest kauguselt viies planeet ja Päikesesüsteemi kõige suurem planeet. Hiidplaneet Jupiter ületab kõigi teiste planeetide kogumassi umbes kaks ja pool korda.

Päikese massist on Jupiteri mass ligikaudu korda väiksem. Astronoomid teavad Jupiteri juba antiikajast.[1] Roomlased panid sellele nime oma jumala Jupiteri   A special contribution of William Coblenz (–) to infrared radiometry and spectroscopy is marked by huge bib.

liography containing hundreds of scientific publications, talks, and abstracts to his credit [20,21]. Infrared Microspectroscopic Measurements Shukichi Ochiai and Hirofumi Seki; Infrared Microspectroscopic Imaging Shigeru Shimada; Near-Infrared Spectroscopy Masao Takayanagi; Far-Infrared Spectroscopy and Terahertz Time-Domain Spectroscopy Seizi Nishizawa; Time-Resolved Infrared Absorption Measurements ?q="Infrared+spectroscopy."&search_field.

Jowisz – piąta w kolejności od Słońca i największa planeta Układu Jowisza jest nieco mniejsza niż jedna tysięczna masy Słońca, a zarazem dwa i pół razy większa niż łączna masa pozostałych planet w Układzie z Saturnem, Uranem i Neptunem tworzą grupę gazowych olbrzymów, nazywaną czasem również planetami ://Saturn, in astronomy, 6th planet from the sun.

Astronomical and Physical Characteristics of Saturn. Saturn's orbit lies between those of Jupiter and Uranus; its mean distance from the sun is c million mi ( billion km), almost twice that of Jupiter, and its period of revolution is about 29 ://Specializing in the 3-D nature of planetary atmospheres as gleaned from spacecraft-borne visual-to-near-infrared spectral imagers, he has been a NASA-selected scientist on the Cassini-Huygens and Galileo orbiter missions to Jupiter and Saturn and was the leader of the NASA science team on ESA's Venus Express orbiter ://