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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.

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At least 253 records · Page 14

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NASA NTRS1967

Red giants and white dwarfs.

Book on red giants and white dwarfs covering stellar evolution, planets and life, solar system origin, etc

GIANT STAR↗

NASA NTRS1999

Giant Magnetoresistive (GMR) Sensor Microelectromechanical System (MEMS) Device

The measurement of acceleration has been accomplished using several technologies in high-reliability applications such as guidance control, detonation, and shock/vibration measurement. Electromechanical, piezoelectric, piezoresistive, and capacitive acceleration sensors are available and the literature pertinent to giant magnetoresistive sensors (GMR) for the above applications are scanty.

acceleration MEMS GMR giant magnetoresistive senso↗

NASA NTRS1998

Excitation and Disruption of a Giant Molecular Cloud by the Sepurnova Remnant 3C 391

The ambient molecular gas at the distance of the remnant comprises a giant molecular cloud whose edge is closely parallel to a ridge of bright non-thermal radio continuum, which evidently delineates the blast-wave into the cloud.

giant molecular cloud supernova remnants ISM radio↗

NASA NTRS1998

RADII and Effective Temperatures for G,K and M Giants and Supergiants

Interferometrically determined angular diameters obtained at the Palomar Testbed Interferometer (PTI) for 80 giant and supergiant stars are presented in this paper.

Temperatures Palomar Testbed Interferometer (PTI) ↗

NASA NTRS1998

Giant Magnetoresistive (GMR) Sensor Microelectromechanical System (MEMS) Device for Nondestructive Evaluation (NDE) Health Monitoring Applications for International Space Station (ISS)

This paper discusses the fabrication aspects of an accelerometer device that is based on a sputter deposited, multilayer, and giant magnetoresistive field sensor.

Mission Assurance accelerometer Giant Magnetoresis↗

NASA NTRS1994

The tip of the Red Giant Branch as a Distance Indicator for Resolved Galaxies: II. Computer Simulations

Based on both empirical data for nearby galaxies, and on computer simulations, we show that measuring the position of the tip of the first-ascent red-giant branch (TRGB) provides a means of obtaining the distances to nearby galaxies with a precision and accuracy comparable to using Cepheids and/or RR Lyrae variables.

Red Giants↗

NASA NTRS2010

Galactic Bulge Giants: Probing Stellar and Galactic Evolution. 1. Catalogue of Spitzer IRAC and MIPS Sources (PREPRINT)

Aims. We aim at measuring mass-loss rates and the luminosities of a statistically large sample of Galactic bulge stars at several galactocentric radii. The sensitivity of previous infrared surveys of the bulge has been rather limited, thus fundamental questions for late stellar evolution, such as the stage at which substantial mass-loss begins on the red giant branch and its dependence on fundamental stellar properties, remain unanswered. We aim at providing evidence and answers to these questions. Methods. To this end, we observed seven 15 15 arcmin2 fields in the nuclear bulge and its vicinity with unprecedented sensitivity using the IRAC and MIPS imaging instruments on-board the Spitzer Space Telescope. In each of the fields, tens of thousands of point sources were detected. Results. In the first paper based on this data set, we present the observations, data reduction, the final catalogue of sources, and a detailed comparison to previous mid-IR surveys of the Galactic bulge, as well as to theoretical isochrones. We find in general good agreement with other surveys and the isochrones, supporting the high quality of our catalogue.

CMD(COLOR MAGNITUDE DIAGRAMS)↗

NASA NTRS2016

Lithium in Open Cluster Red Giants Hosting Substellar Companions

We have measured stellar parameters, [Fe/H], lithium abundances, rotation, and (12)C/13C in a small sample of red giants (RGs) in three open clusters that are each home to a RG star that hosts a substellar companion (SSC) (NGC 2423 3, NGC 4349 127, and BD+12 1917 in M67). Our goal is to explore whether the presence of SSCs influences the Li content. Both (12)C/13C and stellar rotation are measured as additional tracers of stellar mixing. One of the companion hosts, NGC 24233, is found to be Li-rich with A(Li)(sub NLTE) = 1.56 dex, and this abundance is significantly higher than the A(Li) of the two comparison stars in NGC 2423. All three SSC hosts have the highest A(Li) and (12)C/13C when compared to the control RGs in their respective clusters; however, except for NGC 24233, at least one control star has similarly high abundances within the uncertainties. Higher A(Li) could suggest that the formation or presence of planets plays a role in the degree of internal mixing on or before the RG branch. However, a multitude of factors affect A(Li) during the RG phase, and when the abundances of our sample are compared with the abundances of RGs in other open clusters available in the literature, we find that they all fall well within a much larger distribution of A(Li) and (12)C/13C. Thus, even the high Li in NGC 2423 3 cannot be concretely tied to the presence of the SSC.

stellar parameters↗

NASA NTRSDate not supplied

Parametric Analysis of Entry Vehicles for Giant Planet Missions

Summarize concept designs for entry vehicles for giant planet destinations identified as high priority in the latest decadal survey. Identify viable entry states, aerothermal environments, and heatshield thermal protection systems (TPS) for various vehicle dimensions. Viable TPS options and sizing focus on low-g (< 50g) entry conditions to avoid costly instrumentation requalification. TPS manufacturing capabilities are also taken into consideration while adhering to the manufacturing capabilities of the TPS options. Margined mass estimates for heatshield TPS options are provided for Uranus and Saturn test cases.

Giant Planet↗

NASA NTRS1962