scholarly journals Solar system bodies ‘Observations in the Past’ with the plate archive of the Main Astronomical Observatory of the Ukrainian National Academy of Sciences

2006 ◽  
Vol 2 (14) ◽  
pp. 615-615
Author(s):  
Tetyana P. Sergeeva ◽  
Aleksandre V. Sergeev

The improvement of the dynamical models of solar system bodies’ motions will be very useful for the future space astrometry mission Gaia for a fast identification of objects, to discriminate between the well-known objects and the new ones. ‘Observations in the Past’ with plate archives allow realising it.

2021 ◽  
Vol 217 (4) ◽  
Author(s):  
Diego Janches ◽  
Alexey A. Berezhnoy ◽  
Apostolos A. Christou ◽  
Gabriele Cremonese ◽  
Takayuki Hirai ◽  
...  

AbstractThis manuscript represents a review on progress made over the past decade concerning our understanding of meteoroid bombardment on airless solar system bodies as one of the sources of the formation of their exospheres. Specifically, observations at Mercury by MESSENGER and at the Moon by LADEE, together with progress made in dynamical models of the meteoroid environment in the inner solar system, offer new tools to explore in detail the physical phenomena involved in this complex relationship. This progress is timely given the expected results during the next decade that will be provided by new missions such as DESTINY+, BepiColombo, the Artemis program or the Lunar Gateway.


2020 ◽  
Vol 497 (1) ◽  
pp. L46-L49 ◽  
Author(s):  
A Morbidelli ◽  
K Batygin ◽  
R Brasser ◽  
S N Raymond

ABSTRACT In two recent papers published in MNRAS, Namouni and Morais claimed evidence for the interstellar origin of some small Solar system bodies, including: (i) objects in retrograde co-orbital motion with the giant planets and (ii) the highly inclined Centaurs. Here, we discuss the flaws of those papers that invalidate the authors’ conclusions. Numerical simulations backwards in time are not representative of the past evolution of real bodies. Instead, these simulations are only useful as a means to quantify the short dynamical lifetime of the considered bodies and the fast decay of their population. In light of this fast decay, if the observed bodies were the survivors of populations of objects captured from interstellar space in the early Solar system, these populations should have been implausibly large (e.g. about 10 times the current main asteroid belt population for the retrograde co-orbital of Jupiter). More likely, the observed objects are just transient members of a population that is maintained in quasi-steady state by a continuous flux of objects from some parent reservoir in the distant Solar system. We identify in the Halley-type comets and the Oort cloud the most likely sources of retrograde co-orbitals and highly inclined Centaurs.


2015 ◽  
Vol 5 (4) ◽  
pp. 76 ◽  
Author(s):  
Yu-Shou Su

<p>Taiwan has performed well economically during the past four decades. However, economic development can be profoundly hampered by natural disasters. Sustainable economic development requires environmental resilience. With 23 million people occupying only 13,974 square miles of land, Taiwan is both densely populated and highly exposed to natural disasters: 73.1% of the total population lives in vulnerable areas, and Taiwan is ranked as the country most exposed to multiple hazards (The World Bank, 2005). Storms and floods damage Taiwan frequently, with an average of six typhoons hitting Taiwan annually for the past four decades. Taiwan had the highest occurrence and highest death toll on the natural disaster density indicator (NDDI) in comparison with China, Japan, U.S.A, U.K., France, and the Netherlands from 1985 to 2014. Also, Taiwan’s economic losses during the past thirty years are estimated at $650, 000 per km². This is approximately 5 times that of the Netherlands’ $134,362 and the U.K.’s $135,292, 8 times that of the U.S.A.’s $78,186 losses, and 9 times that of France’s $70,599. Research finds that every dollar invested into disaster preparedness would save $4 to $7 dollars in post-disaster damages (Multihazard Mitigation Council, 2005; The National Academy of Sciences, 2012). Hence, promoting urban resilience policies for disaster risk reduction should become a priority in Taiwan and other Asian nations in the future. Most important is the need of a strong political commitment and leadership to initiate and implement spatial policies toward resilience.</p>


MRS Bulletin ◽  
1987 ◽  
Vol 12 (4) ◽  
pp. 20-23 ◽  
Author(s):  
G.L. Liedl

Materials have always been interwoven throughout the very fabric of man's history. The present reawakening to the value and importance of materials, however, has become a dominant factor in manufacturing, national security, international competition and trade, consumer products (quality and reliability), and even education. Other renewals of interest have occurred over the centuries, probably beginning with the formation of the first pot from clay. These renewals were associated with discoveries such as copper, iron, and the transistor. However, in the past 40 years the base for renewed interest has broadened.A true coupling of science and engineering into the field of materials was probably initiated in the 1940s and 1950s. Emphasis at that time was on metals and the “new” semiconductors, with an interest that incubated and grew to where their central position in national economies and man's daily life was recognized. In 1970 the National Academy of Sciences appointed a committee to conduct a comprehensive analysis and assessment of the field of “materials science and engineering.” The COSMAT report which resulted from that study had a dramatic impact on the field and has been a frame of reference for the past 17 years. These years have seen a virtual explosion of ideas, processes, and materials in the field.


2005 ◽  
Vol 1 (T26A) ◽  
pp. 153-160
Author(s):  
Giovanni B. Valsecchi ◽  
Julio A. Fernández ◽  
J.-E. Arlot ◽  
E.L.G. Bowell ◽  
Y. Chernetenko ◽  
...  

The past triennium has continued to see a huge influx of astrometric positions of small solar system bodies provided by near-Earth object (NEO) surveys. As a result, the size of the orbital databases of all populations of small solar system bodies continues to increase dramatically, and this in turn allows finer and finer analyses of the types of motion in various regions of the orbital elements space.


Author(s):  
M. A. (Tony) Barry ◽  
Dave Gault ◽  
Hristo Pavlov ◽  
William Hanna ◽  
Alistair McEwan ◽  
...  

AbstractStellar occultations by asteroids and outer solar system bodies can offer ground based observers with modest telescopes and camera equipment the opportunity to probe the shape, size, atmosphere, and attendant moons or rings of these distant objects. The essential requirements of the camera and recording equipment are: good quantum efficiency and low noise; minimal dead time between images; good horological faithfulness of the image timestamps; robustness of the recording to unexpected failure; and low cost. We describe an occultation observing and recording system which attempts to fulfil these requirements and compare the system with other reported camera and recorder systems. Five systems have been built, deployed, and tested over the past three years, and we report on three representative occultation observations: one being a 9 ± 1.5 s occultation of the trans-Neptunian object 28978 Ixion (mv =15.2) at 3 seconds per frame; one being a 1.51 ± 0.017 s occultation of Deimos, the 12 km diameter satellite of Mars, at 30 frames per second; and one being a 11.04 ± 0.4 s occultation, recorded at 7.5 frames per second, of the main belt asteroid 361 Havnia, representing a low magnitude drop (Δmv = ~0.4) occultation.


2021 ◽  
Vol 34 ◽  
pp. 114-118
Author(s):  
S.V. Shatokhina ◽  
L.V. Kazantseva

For more than 50 years, the continuous photographic observations of asteroids have been carried outwith telescopes of the Astronomical Observatory of the Taras Shevchenko National University of Kyiv and the Main Astronomical Observatory of the National Academy of Sciences of Ukraine. About 3,000 photographic plates were obtained, some of which were exposed in 1908. We collected the data on more than 5,500 positions and magnitudes of asteroids on these astroplates taking into account all results of the processing of observations available in various publications and in the Minor Planet Center database. All positional data were compared with JPL ephemeris and analyzed. From different series of asteroid observations the values of positional accuracy were obtained, depending on the methods of measuring and processing the plates and reference catalogs of stars. In order to systematically improve the obtained asteroid positions, we evaluated the possibilities of reprocessing some of the earliest asteroid observations applying the modern star high accuracy catalogs. Using the Tycho-2, Gaia DR2, and Gaia EDR3 as the reference catalogs, the 590 astroplates exposed on the MAO NASU Double Long-Focus Astrograph (DLA) in 1952-1986 were reprocessed based on old plate measurements. All newly determined and previous original asteroid positions were compared with the JPL ephemeris. The comparison results show an improvement in the systematic and random components of the accuracy of coordinates for new positions of asteroids. When comparing the new positions of the asteroids  determined in the Tycho-2 and Gaia catalog systems, no significant changes in accuracy were found.


2019 ◽  
Vol 41 (3) ◽  
pp. 85-89
Author(s):  
E.V. Sklyarenko ◽  
R.V. Serhiienko

We present the results of technical – and – economical analysis showing that the most efficient fuel from biomass for thermal power engineering is bio carbon, which is produced with the help of industrial facility developed and manufactured at the Institute of Engineering Thermophysics of Ukrainian National Academy of Sciences.


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