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Related papers: The Golden Meteorite Fall: Fireball Trajectory, Or…

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Noble metals and gases are very sensitive to the late accretion to the Earth of asteroids and comets. We present mass balance arguments based on these elements that indicate that 0.7E22-2.7E22 kg of extraterrestrial bodies struck the Earth…

Astrophysics · Physics 2015-06-24 N. Dauphas , B. Marty

On September 21 at 18950.56 SOD (05:15:50.56) UT the FREGATE gamma-ray instrument on the High Energy Transient Explorer (HETE) detected a bright gamma-ray burst (GRB). The burst was also seen by the X-detector on the WXM X-ray instrument…

We constrain the formation history of the Milky Way bulge using a two-infall Galactic Chemical Evolution (GCE) framework implemented in the OMEGA++ code. We recover a best-fit scenario in which the bulge forms through an early, rapid…

Astrophysics of Galaxies · Physics 2025-12-10 Niall Miller , Meridith Joyce , Christian I. Johnson , Jamie Tayar , Thomas Trueman , R Michael Rich

Near-Earth asteroid (3200) Phaethon is notable for its association to a strong annual meteor shower, the Geminids, indicative of one or more episodes of mass ejection in the past. The mechanism of Phaethon's past activity is not yet…

Earth and Planetary Astrophysics · Physics 2018-09-05 Quanzhi Ye , Paul A. Wiegert , Man-To Hui

Most C-complex asteroids have albedo values less than 0.1, but there are some high-albedo (bright) C-complex asteroids with albedo values exceeding 0.1. To reveal the nature and origin of bright C-complex asteroids, we conducted…

Earth and Planetary Astrophysics · Physics 2021-01-20 Sunao Hasegawa , Toshihiro Kasuga , Fumihiko Usui , Daisuke Kuroda

Recently a new meteoritic mineral, Zolenskyite (Fe0.99Mn0.04Ca0.01Cr1.99S3.98), was discovered from the Indarch meteorite. Zolenskyite was structurally indexed as the monoclinic C2/m CrNb2Se4 - Cr3S4 type structure of synthetic FeCr2S4,…

Earth and Planetary Astrophysics · Physics 2025-10-20 Boutros Pierre Embaid

Strong strengthening of material under high confining pressure and jet nature of outflow from impact craters permit to show meteoroid impacts of >=10E6 Mt TNT equivalent are capable of ejecting rocks up to ~1 km in size from the Earth into…

Astrophysics · Physics 2007-05-23 E. M. Drobyshevski

The unique CV-type meteorite Khatyrka is the only natural sample in which "quasicrystals" and associated crystalline Cu,Al-alloys, including khatyrkite and cupalite, have been found. They are suspected to have formed in the early Solar…

We report an interesting reentrant metallic resistivity pattern beyond a characteristic temperature T* which is higher than other such characteristic transition temperatures like T(c)(Curie point), T(N) (Neel point), T(CO) (charge order…

Strongly Correlated Electrons · Physics 2007-05-23 Dipten Bhattacharya , H. S. Maiti

We report the serendipitous findings of 13 faint meteors and 44 artificial space objects by Subaru SuprimeCam imaging observations during 11-16 August 2004. The meteors, at about 100km altitude, and artificial satellites/debris in orbit, at…

Astrophysics · Physics 2015-05-13 M. Iye , M. Tanaka , M. Yanagisawa , N. Ebizuka , K. Ohnishi , C. Hirose , N. Asami , Y. Komiyama , H. Furusawa

Main-belt asteroid (6478) Gault was observed to show cometary features in early 2019. To investigate the cause, we conducted {\it BVR} observations at Xingming Observatory, China, from 2019 January to April. The two tails were formed around…

Earth and Planetary Astrophysics · Physics 2019-07-24 Man-To Hui , Yoonyoung Kim , Xing Gao

On October 8th, 2011 the Earth crossed the dust trails left by comet 21P/Giacobini-Zinner during its XIX and XX century perihelion approaches with the comet being close to perihelion. The geometric circumstances of that encounter were thus…

Past studies suggest that long-duration gamma-ray bursts (GRBs) have a standard energy of E_gamma ~ 10^51 erg in ultra-relativistic ejecta when corrected for asymmetry ("jets"). However, recently a group of sub-energetic bursts, including…

A circumsolar dust ring has been recently discovered close to the orbit of Mercury. There are currently no hypotheses for the origin of this ring in the literature, so we explore four different origin scenarios here: the dust originated…

Earth and Planetary Astrophysics · Physics 2023-01-25 Petr Pokorny , Ariel N. Deutsch , Marc J. Kuchner

C/2002 CE$_{10}$ is an object in a retrograde elliptical orbit with Tisserand parameter $-0.853$ indicating a likely origin in the Oort Cloud. It appears to be a rather inactive comet since no coma and only a very weak tail was detected…

Earth and Planetary Astrophysics · Physics 2018-02-28 Tomohiko Sekiguchi , Seidai Miyasaka , Budi Dermawan , Thomas Mueller , Naruhisa Takato , Junichi Watanabe , Hermann Boehnhardt

On 2013 February 15 a small asteroid rammed against the atmosphere above the region of Chelyabinsk in Russia, producing the most powerful superbolide since the Tunguska event in 1908. Lacking proper astrometric observations, the pre-impact…

Earth and Planetary Astrophysics · Physics 2015-10-08 C. de la Fuente Marcos , R. de la Fuente Marcos , S. J. Aarseth

We present radiometric effective radii and visual geometric albedos for six asteroids in comet-like orbits. Our sample has three of the four known retrograde asteroids (1999 LE31, 2000 DG8, and 2000 HE46) and three objects ((18916) 2000…

Astrophysics · Physics 2009-11-06 Y. R. Fernandez , D. C. Jewitt , S. S. Sheppard

Aims. We will test the statistical significance of meteorite-dropping fireballs and NEA clustering using the DN similarity function based on four geocentric quantities (U, theta, phi, and lambda). Methods. We calculated the cumulative…

Earth and Planetary Astrophysics · Physics 2025-10-08 P. M. Shober

The asteroid (3200) Phaethon is known to be the parent body of the Geminids, although meteor showers are commonly associated with the activity of periodic comets. What is most peculiar to the asteroid is its comet-like activity in the…

The identification of basaltic asteroids in the asteroid Main Belt and the description of their surface mineralogy is necessary to understand the diversity in the collection of basaltic meteorites. Basaltic asteroids can be identified from…

Astrophysics · Physics 2008-01-14 R. Duffard , F. Roig