Starscan Johnson Space Center Astronomical Society VOLUME 22, NUMBER 4 April 2006
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Arxiv:2012.09981V1 [Astro-Ph.SR] 17 Dec 2020 2 O
Contrib. Astron. Obs. Skalnat´ePleso XX, 1 { 20, (2020) DOI: to be assigned later Flare stars in nearby Galactic open clusters based on TESS data Olga Maryeva1;2, Kamil Bicz3, Caiyun Xia4, Martina Baratella5, Patrik Cechvalaˇ 6 and Krisztian Vida7 1 Astronomical Institute of the Czech Academy of Sciences 251 65 Ondˇrejov,The Czech Republic(E-mail: [email protected]) 2 Lomonosov Moscow State University, Sternberg Astronomical Institute, Universitetsky pr. 13, 119234, Moscow, Russia 3 Astronomical Institute, University of Wroc law, Kopernika 11, 51-622 Wroc law, Poland 4 Department of Theoretical Physics and Astrophysics, Faculty of Science, Masaryk University, Kotl´aˇrsk´a2, 611 37 Brno, Czech Republic 5 Dipartimento di Fisica e Astronomia Galileo Galilei, Vicolo Osservatorio 3, 35122, Padova, Italy, (E-mail: [email protected]) 6 Department of Astronomy, Physics of the Earth and Meteorology, Faculty of Mathematics, Physics and Informatics, Comenius University in Bratislava, Mlynsk´adolina F-2, 842 48 Bratislava, Slovakia 7 Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, H-1121 Budapest, Konkoly Thege Mikl´os´ut15-17, Hungary Received: September ??, 2020; Accepted: ????????? ??, 2020 Abstract. The study is devoted to search for flare stars among confirmed members of Galactic open clusters using high-cadence photometry from TESS mission. We analyzed 957 high-cadence light curves of members from 136 open clusters. As a result, 56 flare stars were found, among them 8 hot B-A type ob- jects. Of all flares, 63 % were detected in sample of cool stars (Teff < 5000 K), and 29 % { in stars of spectral type G, while 23 % in K-type stars and ap- proximately 34% of all detected flares are in M-type stars. -
Aerospace Safety Advisory Panel
Aerospace Safety Advisory Panel Annual Report for 2009 NASA AEROSPACE SAFETY ADVISORY PANEL National Aeronautics and Space Administration Washington, DC 20546 VADM Joseph W. Dyer, USN (Ret.), Chair January 15, 2010 The Honorable Charles F. Bolden, Jr. Administrator National Aeronautics and Space Administration Washington, DC 20546 Dear General Bolden: Pursuant to Section 106(b) of the National Aeronautics and Space Administration Authorization Act of 2005 (P.L. 109-155), the Aerospace Safety Advisory Panel (ASAP) is pleased to submit the ASAP Annual Report for 2009 to the U.S. Congress and to the Administrator of the National Aeronautics and Space Administration (NASA). ASAP members believe that NASA and the Administration face significant challenges for the Nation’s space program. Following the precedent set in 2008, the ASAP again pro - vides this letter report in lieu of the lengthier annual report submitted in previous years. This letter report is based on the Panel’s 2009 quarterly meetings (and public session minutes), fact-finding meetings, and formal recommendations, as well as ASAP members’ past experiences. In Section II of this report, the Panel provides a summary of key safety-related issues that the Agency confronts at this time. The most important relate to the future of the Nation’s human space flight program, and the ASAP hopes to encourage key stakeholders to immediately consider the critical decisions relating to this mission. Significant issues include human rating requirements for potential commercial and international entities, extension of Shuttle beyond the current manifest, workforce transition from the Shuttle to the follow-on program, the need for candid public communications about the risks of human space flight, and the more aggressive use of robots to reduce the risk of human exploration. -
Mars Exploration Office Jet Propulsion Laboratory California Institute of Technology Pasadena, California
TECHNOLOGIES FOR MARSEXPLORATION AND SAMPLE RETURN Carl F. Ruoff, Technology Manager Mars Exploration Office Jet Propulsion Laboratory California Institute of Technology Pasadena, California ABSTRACT history, to understand how the planet evolved physically, and to locate potentially useful resources. A comprehensive program of robotic Mars exploration is The common thread among these is water: How much being undertaken inorder to address important scientific existed, when, where, and in what form? In addition to questions, to investigate whether or not life exists or ever remote sensing, answering these questions will require existed on Mars, and to pave the way for eventual human surface and subsurface sampling, in-situ analysis, and presence. The program, which is likely to include returning samples to Earth for analysis in terrestrial establishing robotic outposts, will require many technical laboratories. advances. This paper briefly describes key missions in the Mars exploration program, including robotic outposts, and As currently envisioned, the exploration strategy begins discusses near- and far-term technologies needed for theirwith a series of robotic missions which gradually implementation. evolve into the sustained presence of robotic outposts. The early missions will perform science investigations, INTRODUCTION acquire and returnsamples, and will provide engineering The first decades of the new Millennium will see a data on system and technology performance in the vigorous program of robotic Mars exploration, Martian environment. They will also establish undertaken both for compelling scientific reasons as communication and navigation capabilities and will well as to pave the way, over the long term, for human make it possible to select promising sites for additional missions and potential human habitation. -
Instruction Manual Meade Instruments Corporation
Instruction Manual 7" LX200 Maksutov-Cassegrain Telescope 8", 10", and 12" LX200 Schmidt-Cassegrain Telescopes Meade Instruments Corporation NOTE: Instructions for the use of optional accessories are not included in this manual. For details in this regard, see the Meade General Catalog. (2) (1) (1) (2) Ray (2) 1/2° Ray (1) 8.218" (2) 8.016" (1) 8.0" Secondary 8.0" Mirror Focal Plane Secondary Primary Baffle Tube Baffle Field Stops Correcting Primary Mirror Plate The Meade Schmidt-Cassegrain Optical System (Diagram not to scale) In the Schmidt-Cassegrain design of the Meade 8", 10", and 12" models, light enters from the right, passes through a thin lens with 2-sided aspheric correction (“correcting plate”), proceeds to a spherical primary mirror, and then to a convex aspheric secondary mirror. The convex secondary mirror multiplies the effective focal length of the primary mirror and results in a focus at the focal plane, with light passing through a central perforation in the primary mirror. The 8", 10", and 12" models include oversize 8.25", 10.375" and 12.375" primary mirrors, respectively, yielding fully illuminated fields- of-view significantly wider than is possible with standard-size primary mirrors. Note that light ray (2) in the figure would be lost entirely, except for the oversize primary. It is this phenomenon which results in Meade 8", 10", and 12" Schmidt-Cassegrains having off-axis field illuminations 10% greater, aperture-for-aperture, than other Schmidt-Cassegrains utilizing standard-size primary mirrors. The optical design of the 4" Model 2045D is almost identical but does not include an oversize primary, since the effect in this case is small. -
A Healthy Outlook NASA’S FY16 Budget Funds JPL’S Ongoing Work, Future Initiatives
FEBRUARY Jet Propulsion 2015 Laboratory VOLUME 45 NUMBER 2 A healthy outlook NASA’s FY16 budget funds JPL’s ongoing work, future initiatives By Mark Whalen The White House’s budget request for fiscal year 2016 includes “Last year was an exciting year and I think this year is going to full funding for all of JPL’s ongoing missions as well as continuing be even more exciting,” JPL Director Charles Elachi told employ- support for development of a mission to Jupiter’s moon Europa ees in an all-hands meeting. next decade. Continued on page 2 BUDGET Continued from page 1 2 The request includes about $5.2 billion Space Research Organization; Orbiting sion,” Elachi said. “In order to deploy as- for science overall, of which $1.95 billion Carbon Observatory 3; the Surface Wa- sets on Mars for humans, you need a lot Universe is requested for Earth science and $1.36 ter Ocean Topography mission; and a of tonnage. Electric propulsion is the most billion for planetary science. NASA’s total Gravity Recovery and Climate Experiment efficient way to transport heavy mass.” FY 2016 budget requests $18.5 billion. follow-on mission. The proposed asteroid mission’s two “NASA did pretty well in this very tight All ongoing Mars activities and op- major objectives, he added, are illustrat- budget environment,” said Elachi, noting erations at JPL are fully funded, as is ing high-power electric propulsion and an increase of $450 million relative to FY the continuing development of the Mars providing a platform to assess astronauts 14. -
In Search of a Cure IIT 2010
Features F ALL 2005 IIT MAGAZINE Associate Vice President of Communications and Marketing Catherine Braendel Director of Marketing Marlis Manley Broadhead Managing Editor Chelsea Kalberloh Jackson Contributing Editors Catherine Bruck Beth Duncan Jon Kavanaugh Anne Johnson Theresa Minarik Melanie Nimrodi Abigail Nall Linda Packer Beth Wittbrodt Art Editor Theresa Minarik Design 18 Panebianco, Inc. IIT Magazine is published three times Cover: The Crowded Sky a year by the Office of Communications Cell phones, laptops, radios, and and Marketing. © 2005 airplanes—even microwaves—are Send Letters To all competing for increasingly con- IIT Magazine gested air space. Researchers at Office of Communications and Marketing IIT’s Wireless Interference Labora- 3300 South Federal Street Main Building, Suite 503 tory are studying how to prevent Chicago, IL 60616-3793 a frequency overload. 22 Or Email [email protected] Big Things in Small Packages Send Alumni News To What could the ultra-small neutrino [email protected]. tell us about the universe? Professor 12 Chris White is shooting them from Founded in 1890, Illinois Institute of Technology is a private Chicago to Minnesota in hopes of In Search of a Cure Ph.D.-granting university that awards finding out. IIT is steadily building its reputation degrees in engineering, the sciences, math- ematics, architecture, law, design, psycholo- in cancer research. Bolstered by sev- gy, and business. IIT takes an interprofes- eral high-profile grants, researchers 24 sional approach to research and teaching. at IITRI and faculty and students in By reaching across geographic boundaries, engineering and the life sciences are A Man for Mars academic disciplines, and the professions, investigating new ways to detect, Now more than ever, the world is IIT prepares students for leadership roles in an increasingly complex global workplace treat, and prevent this disease. -
Spaceport News America's Gateway to the Universe
MissionUpdate Vol. 36, No. 17 August 29, 1997 Shuttle-Mir Spaceport News America's gateway to the universe. Leading the world in preparing and launching missions to Earth and beyond. John F. Kennedy Space Center Internal EVA conducted: Mir 24 cosmonauts Anatoly Solovyev and Pavel Vinogradov and U.S. astronaut Michael Foale continue the process of verifying restoration of electrical power to the Russian Busy week at Space Station Mir after an intravehicular activity Aug. 22. Troubleshooting of the oxygen- generating system also was under America’s way, and an extravehicular activity was tentatively set for the first week of September to conduct an spaceport inspection of leak sites on the damaged Spektr module. STS-86 ONE Shuttle rolled out to the launch pad Aug. 18 and another returned to KSC the following day. The Space Shuttle Atlantis (above) is now at Pad 39A, undergoing final preparations for launch Sept. 25 on the seventh Shuttle-Mir docking mission, STS-86. The Terminal Countdown Demonstration Test is scheduled for Sept. 9- Atlantis (20th flight OV-104) 10. At about 7:08 a.m., Aug. 19, Discovery (right) 87th Shuttle flight touched down on Runway 33 of KSC's Shuttle Landing Pad 39A Facility, bringing Mission STS-85 to a successful 7th Mir Docking conclusion. Researchers were delighted with the Launch: Sept. 25, 10:34 p.m. performance of the primary scientific instruments flown Crew: Wetherbee; Bloomfield; on the 86th Shuttle flight, the Cryogenic Infrared Parazynski; Titov; Chretien Spectrometers and Telescopes for the Atmosphere (France); Lawrence; Wolf. (CRISTA)-SPAS and the Middle Atmosphere High Commander Wetherbee flew on Resolution Spectrograph Investigation (MAHRSI), both of STS-63, the Shuttle flight that which performed flawlessly. -
The Double Helix Nebula: a Magnetic Torsional Wave Propagating out of the Galactic Centre
The Double Helix Nebula: a magnetic torsional wave propagating out of the Galactic centre Mark Morris1, Keven Uchida2, and Tuan Do1 1Department of Physics and Astronomy, University of California, Los Angeles, Los Angeles, CA 90095-1547, USA 2Center for Radiophysics and Space Research, Cornell University, Space Sciences Building, Ithaca, NY 14853-6801 Radioastronomical studies have indicated that the magnetic field in the central few hundred parsecs of our Milky Way Galaxy has a dipolar geometry and a strength substantially larger than elsewhere in the Galaxy, with estimates ranging up to a milligauss1-6. A strong, large-scale magnetic field can affect the Galactic orbits of molecular clouds by exerting a drag on them, it can inhibit star formation, and it can guide a wind of cosmic rays away from the central region, so a characterization of the magnetic field at the Galactic center is important for understanding much of the activity there. Here, we report Spitzer Space Telescope observations of an unprecedented infrared nebula having the morphology of an intertwined double helix. This feature is located about 100 pc from the Galaxy’s dynamical centre toward positive Galactic latitude, and its axis is oriented perpendicular to the Galactic plane. The observed segment is about 25 pc in length, and contains about 1.25 full turns of each of the two continuous, helically wound strands. We interpret this feature as a torsional Alfvén wave propagating vertically away from the Galactic disk, driven by rotation of the magnetized circumnuclear gas disk. As such, it offers a new morphological probe of the Galactic center magnetic field. -
Atlas Menor Was Objects to Slowly Change Over Time
C h a r t Atlas Charts s O b by j Objects e c t Constellation s Objects by Number 64 Objects by Type 71 Objects by Name 76 Messier Objects 78 Caldwell Objects 81 Orion & Stars by Name 84 Lepus, circa , Brightest Stars 86 1720 , Closest Stars 87 Mythology 88 Bimonthly Sky Charts 92 Meteor Showers 105 Sun, Moon and Planets 106 Observing Considerations 113 Expanded Glossary 115 Th e 88 Constellations, plus 126 Chart Reference BACK PAGE Introduction he night sky was charted by western civilization a few thou - N 1,370 deep sky objects and 360 double stars (two stars—one sands years ago to bring order to the random splatter of stars, often orbits the other) plotted with observing information for T and in the hopes, as a piece of the puzzle, to help “understand” every object. the forces of nature. The stars and their constellations were imbued with N Inclusion of many “famous” celestial objects, even though the beliefs of those times, which have become mythology. they are beyond the reach of a 6 to 8-inch diameter telescope. The oldest known celestial atlas is in the book, Almagest , by N Expanded glossary to define and/or explain terms and Claudius Ptolemy, a Greco-Egyptian with Roman citizenship who lived concepts. in Alexandria from 90 to 160 AD. The Almagest is the earliest surviving astronomical treatise—a 600-page tome. The star charts are in tabular N Black stars on a white background, a preferred format for star form, by constellation, and the locations of the stars are described by charts. -
The Idea of Sacred Time Is As Old As Human History As Well As Being Attributed to a Time Before Human History Began
The Sacred Time of 2012 By Willard G. Van De Bogart June 21, 2008 The wonderful host of rays has risen: the eye of Mitra, Varuna, and Agni: the Sun, the soul of all that moves or Immovable, has filled the heaven, the Earth and the firmament. Rig-Veda: 1, 115, 1 The idea of sacred time is as old as human history itself as well as being attributed to a time before human history began. It is a time known as the creation time. The time 2012 is thought of as the end time, the time when the world comes to an end and unimaginable catastrophes end the human race resulting in the infamous doomsday scenario and the fulfillment of the two millennia of Christian eschatology. Due to the loss of understanding of the celestial significance of the time 2012, and its relationship to human cognition, the unprecedented opportunity to be spiritually transformed is the other scenario which this paper on the sacred time of 2012 will address. 1 Sacred time is unlike the time associated with daily activities but is rather a time affiliated with a reverence for heaven and earth, honored and held in the highest esteem, and definitely not to be sullied by actions counter to the messages conveyed by actions or events considered to be a part of that sacred time when the universe was born; the creation time. Assailing or desacralizing the concept of something which is sacred is perhaps one of the greatest cultural efforts attempted by a deconstructionist point of view, or even by those who just wish to undermine or dismantle the ideological framework which allows the idea of something to become sacred. -
Mars Rover Opportunity Working at 'Matijevic Hill' Site 30 September 2012
Mars rover Opportunity working at 'Matijevic Hill' site 30 September 2012 reminiscent of, but different from, the iron-rich spheres nicknamed "blueberries" at the rover's landing site nearly 22 driving miles ago (35 kilometers). The small spheres at Matijevic Hill have different composition and internal structure. Opportunity's science team is evaluating a range of possibilities for how they formed. The spheres are up to about an eighth of an inch (3 millimeters) in diameter. The "blueberries" found earlier are concretions formed by the action of mineral-laden water inside rocks, but that is only one of the ways nature can make small, rounded particles. One working hypothesis, out of several, is that the new-found spherules are also concretions but with a different Rock fins up to about 1 foot (30 centimeters) tall composition. Others include that they may be dominate this scene from the panoramic camera accretionary lapilli formed in volcanic ash eruptions, (Pancam) on NASA's Mars Exploration Rover Opportunity. The component images were taken during impact spherules formed in impact events, or the 3,058th Martian day, or sol, of Opportunity's work on devitrification spherules resulting from formation of Mars (Aug. 23, 2012). The view spans an area of terrain crystals from formerly melted material. There are about 30 feet (9 meters) wide. Orbital investigation of the other possibilities, too. area has identified a possibility of clay minerals in this area of the Cape York segment of the western rim of "Right now we have multiple working hypotheses, Endeavour Crater. The view combines exposures taken and each hypothesis makes certain predictions through Pancam filters centered on wavelengths of 753 about things like what the spherules are made of nanometers (near infrared), 535 nanometers (green) and and how they are distributed," said Opportunity's 432 nanometers (violet). -
Modeling Blue Stragglers in Young Clusters∗
Research in Astron. Astrophys. 2011 Vol . 11 No. 11, 1336–1350 Research in http://www.raa-journal.org http://www.iop.org/journals/raa Astronomy and Astrophysics Modeling blue stragglers in young clusters∗ Pin Lu1,2,Li-CaiDeng1 and Xiao-Bin Zhang1 1 Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China; [email protected] 2 Graduate University of Chinese Academy of Sciences, Beijing 100049, China Received 2011 June 11; accepted 2011 July 19 Abstract A grid of binary evolution models are calculated for the study of a blue straggler (BS) population in intermediate age (log Age = 7.85 − 8.95) star clusters. The BS formation via mass transfer and merging is studied systematically using our models. Both Case A and B close binary evolutionary tracks are calculated for a large range of parameters. The results show that BSs formed via Case B are generally bluer and even more luminous than those produced by Case A. Furthermore, the larger range in orbital separations of Case B models provides a probability of producing more BSs than in Case A. Based on the grid of models, several Monte-Carlo simulations of BS populations in the clusters in the age range are carried out. The results show that BSs formed via different channels populate different areas in the color magnitude diagram (CMD). The locations of BSs in CMD for a number of clusters are compared to our simulations as well. In order to investigate the influence of mass transfer efficiency in the models and simulations, a set of models is also calculated by implementing a constant mass transfer efficiency, β =0.5, during Roche lobe overflow (Case A binary evolution excluded).