Infrared and Submillimeter Space Missions in the Coming Decade


Book Description

A revolution similar to that brought by CCDs to visible astronomy is still ahead in IR and submillimeter astronomy. There is certainly no wavelength range which has, over the past several years, seen such impressive advances in technology: large-scale detector arrays, new designs for cooling in space, lightweight mirror technologies. Scientific cases for observing the cold universe are outstanding. Observations in the FIR/Submm range will provide answers to such fundamental questions as: What is the spectrum of the primordial fluctuations? How do primeval galaxies look? What are the first stages of star formation? Most of the international space missions that have been triggered by these questions are presented in detail here. Technological issues raised by these missions are reviewed, as are the most recent achievements in cooling and detector technologies.







New Concepts for Far-Infrared and Submillimeter Space Astronomy


Book Description

The "Second Workshop on New Concepts for Far-Infrared and Submillimeter Space Astronomy" aimed to highlight the groundbreaking opportunities available for astronomical investigations in the far-infrared to submillimeter using advanced, space-based telescopes. The National Research Council's Decade Report, "Astronomy and Astrophysics in the New Millennium," assigned a high priority to a Single Aperture Far-Infrared (SAFIR) observatory and encouraged the subsequent development of space-based far-infrared interferometry. With community guidance from the Origins and Structure and Evolution of the Universe Subcommittees of the Space Science Advisory Committee, NASA recently incorporated SAFIR and a kilometer maximum baseline far-IR interferometer into the Space Science roadmap. The interferometer is widely known as SPECS, the Submillimeter Probe of the Evolution of Cosmic Structure. An important outcome of this workshop was the development of a "Community Plan for Far-IR/Submillimeter Space Astronomy". The name "Community Plan" was adopted because this paper gives the consensus view of the workshop participants. The Community Plan addresses practical considerations, such as the tradeoffs associated with alternative mission designs and the flowdown from scientific objectives to measurement requirements, engineering requirements, and technology needs. It recommends an implementation strategy for technology development and validation, and recommends specific science and technology pathfinder missions that would pave the way for the "roadmap missions" SAFIR and SPECS. The community plan concludes by saying: "The time is right to place SAFIR on the NASA plan as one of the successors of SIRTF and JWST, to set our sights on a longbaseline far-infrared/submillimeter interferometric imaging telescope, to further develop far-infrared/submillimeter single-aperture and interferometric mission concepts, and to invest strategically in the technology that will enable future far-infrared/submillimeter missions. Supporting studies and smaller mission opportunities should be actively pursued."




Next Generation Infrared Space Observatory


Book Description

Infrared astronomy has undergone an enormous revolution during the last decade. Despite the great technical difficulties of building detectors in a cryogenic environment, the scientific advances in infrared astronomy have been astounding. In the near future many more advances can be expected from still newer developments in telescope and detector designs. High quality detector arrays and passively cooled telescopes are very promising techniques for achieving considerably larger apertures. This volume contains the refereed papers from the workshop on 'Next Generation Infrared Observatory', dealing with all new aspects of future infrared telescopes.










The Decade of Discovery in Astronomy and Astrophysics


Book Description

Astronomers and astrophysicists are making revolutionary advances in our understanding of planets, stars, galaxies, and even the structure of the universe itself. The Decade of Discovery presents a survey of this exciting field of science and offers a prioritized agenda for space- and ground-based research into the twenty-first century. The book presents specific recommendations, programs, and expenditure levels to meet the needs of the astronomy and astrophysics communities. Accessible to the interested lay reader, the book explores: The technological investments needed for instruments that will be built in the next century. The importance of the computer revolution to all aspects of astronomical research. The potential usefulness of the moon as an observatory site. Policy issues relevant to the funding of astronomy and the execution of astronomical projects. The Decade of Discovery will prove valuable to science policymakers, research administrators, scientists, and students in the physical sciences, and interested lay readers.







Infrared Submillimeter and Radio Astronomy Research and Analysis Program


Book Description

This program entitled "Infrared Submillimeter and Radio Astronomy Research and Analysis Program" with NASA-Ames Research Center (ARC) was proposed by the Smithsonian Astrophysical Observatory (SAO) to cover three years. Due to funding constraints only the first year installment of $18,436 was funded, but this funding was spread out over two years to try to maximize the benefit to the program. During the tenure of this contact, the investigators at the SAO, Drs. Wesley A. Traub and Nathaniel P. Carleton, worked with the investigators at ARC, Drs. Jesse Bregman and Fred Wittebom, on the following three main areas: 1. Rapid scanning SAO and ARC collaborated on purchasing and constructing a Rapid Scan Platform for the delay arm of the Infrared-Optical Telescope Array (IOTA) interferometer on Mt. Hopkins, Arizona. The Rapid Scan Platform was tested and improved by the addition of stiffening plates which eliminated a very small but noticeable bending of the metal platform at the micro-meter level. 2. Star tracking Bregman and Wittebom conducted a study of the IOTA CCD-based star tracker system, by constructing a device to simulate star motion having a specified frequency and amplitude of motion, and by examining the response of the tracker to this simulated star input. 3. Fringe tracking. ARC, and in particular Dr. Robert Mah, developed a fringe-packet tracking algorithm, based on data that Bregman and Witteborn obtained on IOTA. The algorithm was tested in the laboratory at ARC, and found to work well for both strong and weak fringes. Traub, Wesley A. Ames Research Center




NASA Space Science Vision Missions


Book Description

"Using a solar sail, the Solar Polar Imager mission would observe the Sun from a polar orbit to observe magnetic fields and convective flows in the polar regions as well as coronal mass ejections and the Sun's outer atmosphere in order to better understand the solar dynamo and solar activity. Titan Explorer mission includes an orbiter with remote sensing instruments and an airship platform to investigate the atmosphere, clouds, haze, and surface of Saturn's moon Titan. Neptune Orbiter with Probes mission would use aerocapture to explore Neptune's rings and magnetosphere, which serve as an analog for the primordial solar nebula and accretion disks around other stars, and its satellite Triton, which resembles small objects at the outer boundary of our solar system today. Neptune Orbiter, Probe, and Lander mission would use nuclear electric propulsion to investigate Neptune and orbit its satellite, Triton. Interstellar Probe would leave the heliosphere to explore interstellar space, learning about its composition and dynamics and its interaction with our solar system. Observing distant stars with ultra-high resolution, the Stellar Imager mission could reveal their magnetic activity and internal structure, helping us understand solar activity and magnetohydrodynamics throughout the Universe. By bringing our understanding of other galaxies nearly up to our understanding of our own, the Modern Universe Space Telescope could illuminate how the chemical elements are created and dispersed, how normal galaxies form and evolve, and how stars and planetary systems form. Generation-X mission could detect the first black holes formed when the Universe was only a few hundred million years old. Advanced Compton Telescope is a wide-field gamma-ray spectrometer designed to uncover how supernovae and other stellar explosions create the chemical elements through an all-sky survey of nuclear line emissions. Far-Infrared/Submillimeter Interferometer in Space would use a two-element array to study the formation of the earliest-born stars and galaxies in the Universe and to probe the structure of the disks of gas and dust collapsing today to form a new generation of stars and planets. Single Aperture Far Infrared Observatory would be a single-spacecraft large space telescope for observing the early chemical history of the Universe and the structure of young planetary systems, tracking the chemistry needed for life from interstellar clouds to young solar systems. A final chapter describes an analysis of directions for future technology development inspired by this portfolio of mission concepts."--Publisher description.