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951 gaspra mass

Fri Oct 23 2020

Durch Messung der Größe und Verteilung der Krater wird Gaspras Alter auf 200 Millionen Jahre geschätzt. List of geological features on 951 Gaspra, "JPL Small-Body Database Browser: 951 Gaspra (1916 S45)", "Asteroid 951 Gaspra – Nesvorny HCM Asteroid Families V3.0", "A Galileo Multi Spectral Instrument Analysis of 951 Gaspra", "Regional spectrophotometric properties of 951 Gaspra", https://en.wikipedia.org/w/index.php?title=951_Gaspra&oldid=1014785749, Creative Commons Attribution-ShareAlike License, This page was last edited on 29 March 2021, at 02:04. [5] The results of the orbit integration are shown in Figure 2. These craters are more numerous than previously thought because much of the area seen … Gaspra's surface area has been calculated at about 525 km 2, which, for comparison, is about the size of Guam, or half the land area of Hong Kong. (Galileo also visited 243 Ida where it discovered a moon, allowing a mass estimate there.) If that were true, the volume of Gaspra would be . Neujmin named it after Gaspra, a Black Sea retreat that was visited by his contemporaries, such as Gorky and Tolstoy. This is particularly relevant to mass and density. Neujmin named it after Gaspra, a Black Sea retreat that was visited by his contemporaries, such as Gorky and Tolstoy. The pitted appearance of some grooves may suggest that the surface is covered by a regolith. Gaspra was named by its discoverer Neujmin for a resort on the Crimean peninsula. However, some craters are much deeper than this without showing any structural difference on their walls. 951 Gaspra. The flat facets and concavities give Gaspra a very angular appearance.[8]. where V is the volume, and a, b, and c are the principal radii of the triaxial ellipsoid. [10], Because Gaspra's position was only known to within about 200 km (120 mi) before the encounter, and the camera's field of view was only about 5° across, Galileo would not know where to point to capture images of the asteroid once it was closer than 70,000 km (43,000 mi). [12] It is, however, difficult to explain the origin of a putative regolith. (951) Gaspra ist ein Asteroid des Asteroiden-Hauptgürtels, der am 30. The mass of the celestial body is sufficient to exercise a strength of gravitation superior to the strengths of cohesion of the matter. Through the maze of garden plots at the other end of the space hangs a hollow, aluminum asteroid—which is modeled after 951 Gaspra, the first rocky mass humans were able to observe in detail thanks to a 1991 viewing by the Galileo spacecraft. August 2020 um 17:47 Uhr bearbeitet. Benannt wurde Gaspra nach dem Urlaubsort Gaspra auf der Krim, in dem der russische Schriftsteller Leo Tolstoi längere Zeit lebte. PDF | On Feb 16, 2016, Xiangyuan Zeng and others published Gaspra 951 | Find, read and cite all the research you need on ResearchGate A system of much more prominent grooves is seen on the Martian moon Phobos. [10] It was suggested in 2007 that the fresh, steep craters on Gaspra were formed by the Baptistina family-forming event that happened near it. Subtle albedo and color variations appear to correlate with morphological features: Brighter materials are associated with … This work uses the asteroids 433 Eros and 951 Gaspra as examples cosmic bodies with irregular gravitational fields. Gaspra was the first asteroid ever to be closely approached when it was visited by the Galileo spacecraft, which flew by on its way to Jupiter on 29 October 1991. They tend to be an irregular shaped but Ceres asteroid is known to be spherical in shape but because it doesn't clear its path round the Sun, it is only a dwarf planet. Its surface reflects approximately 20 percent of the sunlight striking it. Gaspra was discovered by Russian astronomer G. N. Neujmin in 1916. Gaspra (Stooke) Gaspra (Thomas) Gaspra (Lightcurve 1) Gaspra (Lightcurve 2) Please note that the models are in planetocentric coordinate system, with Z axis passing through north pole. (Galileo also visited 243 Ida where it discovered a moon, allowing a mass estimate there. Aufgrund seiner Oberflächenbeschaffenheit wird der Asteroid der Spektralklasse S zugeordnet. Gaspra ist ein Asteroid des Asteroiden-Hauptgürtels, der am 30. In dem kleinen Ort Gaspra ist besonders das Sanatorium „Jasnaja Poljana“ von Bedeutung. Oktober 1991 von der Raumsonde Galileo (benannt nach Galileo Galilei) bei einem Vorbeiflug-Manöver (engl. Juli 1916 vom ukrainischen Astronomen G. N. Neuimin (Григорий Николаевич Неуймин) entdeckt wurde. On October 29, 1991, the Galileo spacecraft flew by the asteroid Gaspra on its way to Jupiter. According to , the physical properties and orbital characteristics asteroids are presented in Table 1. Benannt wurde Gaspra nach dem Urlaubsort Gaspra auf der Krim, in dem der russische Schriftsteller Leo … Juli 1916 vom ukrainischen Astronomen G. N. Neuimin (Григорий Николаевич Неуймин) entdeckt wurde. Nach dem Ort ist der Asteroid (951) Gaspra benannt.. Sehenswürdigkeiten. 951 Gaspra /ˈɡæsprə/ is an S-type asteroid that orbits very close to the inner edge of the asteroid belt. Gaspra bewegt sich in einem Abstand von 1,8256 (Perihel) bis 2,5939 (Aphel) astronomischen Einheiten in 3,285 Jahren um die Sonne. These craters are more numerous than previously thought because much of the area seen … [11], Grooves about 100 m (330 ft) to 300 m (980 ft) wide, up to 2.5 km (1.6 mi) long, and tens of meters deep are seen on Gaspra's surface, which may be related to Gaspra's formation along with the rest of the Flora family in an asteroid collision. Gaspra's surface area has been calculated at about 525 km2,[5] which, for comparison, is about the size of Guam, or half the land area of Hong Kong. near flyby) mit einer Entfernung von 1600 km vermessen und fotografiert. At this closest range, the pointing was still not known accurately enough, but the camera took a 51 image mosaic so as to capture Gaspra on at least one image.[10]. Juli 1916 vom ukrainischen Astronomen G. N. Neuimin entdeckt wurde. Gaspra is an irregular body with dimensions of about 20 x 12 x 11 km (12.5 x 7.5 x 7 miles). 107, pp. Facets and limb concavities suggest a long history of large impacts producing 5 to 7 km diameter craters. (951) Gaspra ist ein Asteroid des Asteroiden-Hauptgürtels, der am 30.Juli 1916 vom ukrainischen Astronomen G. N. Neuimin (Григорий Николаевич Неуймин) entdeckt wurde. Es zeigte sich, dass Gaspra ein unregelmäßig geformter Asteroid mit Abmessungen von 19 × 12 × 11 Kilometern ist. [7], Apart from a multitude of small craters, Gaspra has half a dozen large flat areas and concavities. mass of Gaspra is unknown [Belton et al., 1992; Thomas et al., 1994]; we assumed a nominal density of 3 g cm 3.All km-sized bodies whose average densities are known have values lower than this [e.g., Rubincam, 2000], but any departure from the assumed density has only a tiny effect on Gaspra’s orbit about the Sun. Gaspra appears to be fairly olivine-rich among the S-type asteroids (the surface appears to contain olivine and pyroxene in the proportions 4:1 to 7:1[9]). De (951) Gaspra ass en Asteroid vun der Haaptasteroidenceinture, deen den 30. There are no prominent albedo or color patterns, although a subtle color variation is seen across the surface. Their presence also suggest that it is a single coherent body, rather than a rubble pile. We estimate the collisional lifetime of asteroid 951 Gaspra, the first target of an asteroid encounter by an interplanetary space probe. Craters 1 to 4 km in diameter date the last facet-forming impact, though it is not clear which facet this formed. Galileo flew by Gaspra October 29, 1991, passing within 1,600 kilometers. (951) Gaspra Asteroid Gaspra is an asteroid, a large rock that orbits the Sun mainly between the orbits of Mars and Jupiter. One of these flat areas, Dunne Regio, is a 5 km × 7 km (3.1 mi × 4.3 mi) area that is flat to within 200 m (660 ft). I present new maps, photomosaics and geological interpretations of asteroid 951 Gaspra. This was successful and allowed the spacecraft to obtain images from as close as 5,300 km (3,300 mi). Galileo images of Gaspra reveal it to be an irregularly shaped object (19 by 12 by 11 kilometers) that appears to have been created by a catastrophic collisional disruption of a precursor parent body. Benannt wurde Gaspra nach dem Urlaubsort Gaspra auf der Krim, in dem der russische Schriftsteller Leo Tolstoi längere Zeit lebte. EVOLUTION OF THE SURFACE OF 951 GASPRA: Namiki, N. and Binzel, R. P. ... At the end of each time step, h is computed by calculating the mass loss from the weak layer and mass added through penetration of the strong layer. ), Galileo flew by Gaspra on 29 October 1991, passing within 1,600 km (990 mi) at a relative speed of about 8 km/s (18,000 mph). We combine Earth-based telescopic photometry over phase angles 2° ≤ α ≤ 25° with … I thought it might be a good idea to open up a talk about the issue of whether to call asteroid pages like this "951 Gaspra" or just "Gaspra." [10], The extensiveness of regolith on Gaspra and its presence overall is a matter of debate, and not fully understood. Secondly, it has been estimated that the matter ejected by all the craters would be only enough to cover Gaspra with 10 m of regolith. Gaspra dürfte somit ein Bruchstück eines größeren Ursprungskörpers sein, der vor 200 Millionen Jahren bei einer Kollision auseinandergerissen wurde. Gaspra orbits the Sun at an average distance of about 2.21 astronomical units. Gaspra wurde am 29. Below 500 km in diameter, asteroids as Gaspra (15 km) or Ida (56 km), present much more irregular forms. A probable reason is that the collision that produced the Flora family and Gaspra was relatively recent on an astronomical timescale, so that Gaspra has not yet had the opportunity to acquire many large craters since. 14 likes. Sinfonie.Auch Leo Tolstoi lebte dort von 1901 bis 1902. Gaspra was discovered by Russian astronomer G. N. Neujmin in 1916. 18-22, 1994. (951) Gaspra ist ein Asteroid des Asteroiden-Hauptgürtels, der am 30. Der Komponist Dmitri Dmitrijewitsch Schostakowitsch hielt sich hier 1937 auf und komponierte dabei seine 5. This is a mosaic of two images captured on October 29, 1991 from a distance of about 5350 kilometers. Gaspra's surface lacks unambiguous craters of a size comparable to its radius, like those seen for example on 253 Mathilde. [1], Gaspra's rotational axis has been determined[13] to point in the direction of RA 0h40m, declination 27±2°. Asteroid 951 Gaspra Galileo's highest-resolution global view of asteroid Gaspra. (951) Gaspra ist ein Asteroid des Asteroiden-Hauptgürtels, der am 30.Juli 1916 vom ukrainischen Astronomen G. N. Neuimin (Григорий Николаевич Неуймин) entdeckt wurde. Also, correlations are seen between the subtle color variations and local topography, and it has been suggested that this is caused by the slow migration of regolith to lower areas. The Figure shows the expected crater densities for a constant projectile flux corresponding to Population II and f of 10 %. Galileo images of Gaspra make it possible for the first time to determine a main-belt asteroid's photometric properties accurately by providing surface-resolved coverage over a wide range of incidence and emission angles and by extending the phase angle coverage to phases not observable from Earth. NASA / JPL / Emily Lakdawalla. Belton, J. Veverka, and P. C. Thomas, "The Direction of the North Pole and the Control Network of Asteroid 951 Gaspra," Icarus, Vol. Visually, the somewhat subdued and mantled appearance suggests a substantial regolith. Craters 1 to 4 km in diameter date the last facet-forming impact, though it is not clear which facet this formed. Gaspra was discovered by Russian astronomer G. N. Neujmin in 1916. Gaspra ist ein Mitglied der Flora-Familie. Firstly, Gaspra's escape velocity is very small, so small that it is difficult to understand how it could keep a significant portion of fragments ejected by impacts from escaping. It is uncertain whether these are the result of impacts or whether they are instead facets formed when Gaspra broke off its parent asteroid. The choices of these asteroids are explained by the shape of the asteroid, its mass and its orbit. 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