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Instrumentation for the New Millennium Program, Mars Microprobe Project: Design Approach and Test Results
The Mars Microprobe Project provides a unique opportunity to validate instrumentation technologies for performing relevant science experiments on the Martian Surface and at a depth of up to two meters.
Flight Operations in the New Millennium
New approaches are being studied for real-time interaction and related supporting processes with spacecraft and instruments in deep space. Spacecraft are evolving, improving in many ways, and generally becoming more robust. Opertions is changing also. Operatins will be more automated in the future. However, there is a chanllenge. Deep space missions are not all alike. The Operations phases of discovery and exploration are an extension of the research that creates the mission; they are the time of obtaining results.
The New Millennium Formation Flying Optical Interferometer
Spaceborne optical interferometry has been idenfified as a critial technology for many of NASA's 21st century sceince visions.
Forced changes in a Tibetan lake ecosystem over the past millennium
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High-redshift millennium and astrid galaxies in effective field theory at the field level
Effective field theory (EFT) modeling is expected to be a useful tool in the era of future higher-redshift galaxy surveys such as DESI-II and Spec-S5 due to its robust description of various large-scale structure tracers. However, large values of EFT bias parameters of higher-redshift galaxies could jeopardize the convergence of the perturbative expansion. Here, in this paper we measure the bias parameters and other EFT coefficients from samples of two types of star-forming galaxies in the state-of-the-art MilleniumTNG and astrid hydrodynamical simulations. Our measurements are based on the field-level EFT forward model that allows for precision EFT parameter measurements by virtue of cosmic variance cancellation. Specifically, we consider approximately representative samples of Lyman-break galaxies (LBGs) and Lyman-𝛼 emitters (LAEs) that are consistent with the observed (angular) clustering and number density of these galaxies at 𝑧 = 3. Reproducing the linear biases and number densities observed from existing LAE and LBG data, we find quadratic bias parameters that are roughly consistent with those predicted from the halo model coupled with a simple halo occupation distribution model. We also find nonperturbative velocity contributions (fingers of God) of a similar size for LBGs to the familiar case of luminous red galaxies. However, these contributions are quite small for LAEs despite their large satellite fraction values of up to ∼ 30%. Our results indicate that the effective momentum reach 𝑘 max at 𝑧 = 3 for LAEs (LBGs) will be in the range 0.3−0.6ℎ Mpc −1 (0.2−0.8ℎ Mpc −1 ), suggesting that EFT will perform well for high-redshift galaxy clustering. This work provides the first step toward obtaining realistic simulation-based priors on EFT parameters for LAEs and LBGs.
From the November Revolution toward the Millennium: Discoveries, Insights, Tools
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Rapid growth of a carbonate island over the last millennium
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Extracting a History of Global Fire Emissions for the Past Millennium From Ice Core Records of Acetylene, Ethane, and Methane
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Sixteenth Space Simulation Conference Confirming Spaceworthiness Into the Next Millennium
The conference provided participants with a forum to acquire and exchange information on the state of the art in space simulation, test technology, thermal simulation and protection, contamination, and techniques of test measurements.
Toward the next millennium: A vision for spaceship Earth
The transcript of NASA Administrator Daniel S. Goldin's address to the World Space Congress is presented. The address discusses the current international flavor of space exploration, especially in the context of cooperative ventures with the former Soviet Union, and establishes the need for a return to the Moon. Goldin's speech emphasizes that returning to the moon is only the beginning of a program of exploration that will lead to human investigation of Mars, the rest of the solar system, and beyond. By following this program to its logical conclusion, human beings will eventually establish themselves as a multi-planetary species.
Radar Reconnaissance of Near-Earth-Objects at the Dawn of the Next Millennium
Radar, the most powerful ground-based technique for post discovery investigation of NEO's (near-Earth objects), can contribute a great deal to their exploration as well as to identification and mitigation of hazardous objects. My intentions in this article are to review the current state of NEO radar reconnaissance, examine the imminent prospects for this work as upgraded instrumentation becomes available, and propose construction of a next-generation radar telescope that, unlike any existing radar instrument, would be optimized for, and dedicated to, NEO radar.
Issues in NASA Program and Project Management. Special Report: 1997 Conference. Project Management Now and in the New Millennium
Topics Considered Include: NASA's Shared Experiences Program; Core Issues for the Future of the Agency; National Space Policy Strategic Management; ISO 9000 and NASA; New Acquisition Initiatives; Full Cost Initiative; PM Career Development; PM Project Database; NASA Fast Track Studies; Fast Track Projects; Earned Value Concept; Value-Added Metrics; Saturn Corporation Lessons Learned; Project Manager Credibility.
Navigation for the new millennium: Autonomous navigation for Deep Space 1
The autonomous optical navigation system technology for the Deep Space 1 (DS1) mission is reported on. The DS1 navigation system will be the first to use autonomous navigation in deep space. The systems tasks are to: perform interplanetary cruise orbit determination using images of distant asteroids; control and maintain the orbit of the spacecraft with an ion propulsion system and conventional thrusters, and perform late knowledge updates of target position during close flybys in order to facilitate high quality data return from asteroid MaAuliffe and comet West-Kohoutek-Ikemura. To accomplish these tasks, the following functions are required: picture planning; image processing; dynamical modeling and integration; planetary ephemeris and star catalog handling; orbit determination; data filtering and estimation; maneuver estimation, and spacecraft ephemeris updating. These systems and functions are described and preliminary performance data are presented.
Check-Up of Planet Earth at the Turn of the Millennium: Anticipated New Phase in Earth Sciences
Langley's remarkable solar and lunar spectra collected from Mt. Whitney inspired Arrhenius to develop the first quantitative climate model in 1896. In 1999, NASA's Earth Observing AM Satellite (EOS-AM) will repeat Langley's experiment, but for the entire planet, thus pioneering calibrated spectral observations from space. Conceived in response to real environmental problems, EOS-AM, in conjunction with other international satellite efforts, will fill a major gap in current efforts by providing quantitative global data sets with a resolution of few kilometers on the physical, chemical and biological elements of the earth system. Thus, like Langley's data, EOS-AM can revolutionize climate research by inspiring a new generation of climate system models and enable us to assess the human impact on the environment.
X-33, Leading the Way to VentureStar(trademark)) in the Next Millennium
The X-33, NASA's flagship for reusable space plane technology demonstration, is on course to begin the flights of the X-33 that will permit industry and government decisions that can lead to VentureStar(trademark) by the end of 2000. Lockheed Martin, NASA's partner in this effort, took the bold step in January 1999 to announce formation of VentureStar(trademark) LLC. This move provides the focus for firm business planning needed to enable the decision by the time X-33 flies in mid 2000. The X-33 program began by accepting the mandate that included two unprecedented and highly challenging goals: 1) demonstrate single stage to orbit technologies in flight and ground by the end of 2000 and 2) demonstrate a new government and industry management relationship working together with industry in the lead. Since the IAF 49th Congress in Melbourne, the major hardware elements of X-33 have been through their assembly and test. The flight liquid oxygen tank was the first major element to complete final assembly. The liquid hydrogen tanks are currently in final assembly and testing. The first flight tank has been delivered to vehicle assembly, the second tank and the flight engines are expected this month. The aerospike engine is an engine concept that has never been flown, but has been extensively ground tested. It will be flown for the first time on the X-33. Major X-33 flight hardware has been tested, delivered, and assembly of the vehicle is nearly complete. Construction of the prototype spaceport was completed in November 1998. The flight test program commencing in the summer of 2000. The decision to proceed with a Single Stage To Orbit as a commercial venture is expected in the fall of 2000.
Check-Up of Planet Earth at the Turn of the Millennium Anticipated New Phase in Earth Sciences
Langley's remarkable solar and lunar spectra collected from mt. Whitney inspired Arrhenius to develop the first quantitative climate model in 1896. In 1999, NASA's Earth Observing AM Satellite named recently "Terra" (by Ms. Sasha Jones, a 17 year old student in St. Louis, MO) will repeat Langley's experiment, but for the entire planet, thus pioneering calibrated spectral observations from space. Conceived in response to real environmental problems, EOS-AM, in conjunction with other international satellite efforts, will fill a major gap in current efforts by providing quantitative global data sets with a resolution of few kilometers on the physical, chemical and biological elements of the earth system. Thus, like Langley's data, EOS-AM can revolutionize climate research by inspiring a new generation of climate system models and enable us to assess the human impact on the environment. In this talk I shall a give a historical perspective for the need for this expensive mission, give examples of the science that we anticipate to achieve using Terra measurements and describe this exciting mission.