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Chondritic meteorites provide valuable opportunities to investigate the origins of the solar system. We explore impact jetting as a mechanism of chondrule formation and subsequent pebble accretion as a mechanism of accreting chondrules onto…

地球与行星天体物理 · 物理学 2016-03-23 Yasuhiro Hasegawa , Neal J. Turner , Joseph Masiero , Shigeru Wakita , Yuji Matsumoto , Shoichi Oshino

Mean-motion resonances play an important role in the evolution of various meteoroid streams. Previous works have studied the effects of two-body resonances in different comets and streams. These already established two-body resonances were…

地球与行星天体物理 · 物理学 2016-05-23 Aswin Sekhar , David Asher , Jeremie Vaubaillon

Since 2009 the double station meteor observation by the all-sky video cameras of the Slovak Video Meteor Network (SVMN) brought hundreds of orbits. Thanks to several amateur wide field video stations of the Central European Meteor Network…

On June 2, 2016 at 10h56m UTC, a $-20.4 \pm 0.2$ magnitude superbolide was observed over Arizona. Fragments were located a few days later and the meteorites were given the name Dishchii'bikoh. We present analysis of this event based on 3…

地球与行星天体物理 · 物理学 2020-01-10 Csaba Palotai , Ramanakumar Sankar , Dwayne L. Free , J. Andreas Howell , Elena Botella , Daniel Batcheldor

Meteors can be classified into either sporadic meteors or showery meteors. We compile the meteor records in the astronomical archives in the Chronicle of the Koryo dynasty (918-1392), and investigate the spatial distribution of meteor…

天体物理学 · 物理学 2009-11-07 Sang-Hyeon Ahn

This concept article discusses the possibilities for identifying sedimentary-origin meteorites. The paper concerns (i) the macroscopic candidate for sedimentary meteorite in the epicenter of the 1908 Tunguska catastrophe; (ii) potential…

地球与行星天体物理 · 物理学 2017-06-21 Yana Anfinogenova , John Anfinogenov , Larisa Budaeva , Dmitry Kuznetsov

We present initial observations of the newly-discovered active asteroid 313P/Gibbs (formerly P/2014 S4), taken to characterize its nucleus and comet-like activity. The central object has a radius $\sim$0.5 km (geometric albedo 0.05…

地球与行星天体物理 · 物理学 2015-06-23 David Jewitt , Jessica Agarwal , Nuno Peixinho , Harold Weaver , Max Mutchler , Man-To Hui , Jing Li , Stephen Larson

We investigate the conditions under which Leonid meteoroids might generate short duration (burster) electrophonic sounds. A `first order' theory is employed to estimate the approximate electron number density in the meteoroid ablation…

天体物理学 · 物理学 2009-10-31 Martin Beech , Luigi Foschini

We report on high-resolution imaging and spectral observations of eruptions of a spiral structure in the transition region, which were taken with the Interface Region Imaging Spectrometer (IRIS), the Atmospheric Imaging Assembly (AIA) and…

太阳与恒星天体物理 · 物理学 2018-02-28 Zhenghua Huang , Lidong Xia , Chris J. Nelson , Jiajia Liu , Thomas Wiegelmann , Hui Tian , James A. Klimchuk , Yao Chen , Bo Li

Context. The existence of meteor clusters has long since been a subject of speculation and so far only seven events have been reported, among which two involve less than five meteors, and three were seen during the Leonid storms. Aims. The…

Many previous works have shown the relevance and dynamics of Jovian mean motion resonances (MMR) in various meteoroid streams. These resonant swarms are known to have produced spectacular meteor displays in the past. In this work we…

地球与行星天体物理 · 物理学 2015-06-16 Aswin Sekhar , David J. Asher

On 2013 September 11 at 20h07m28.68 $\pm$ 0.01 s UTC, two telescopes operated in the framework of our lunar impact flashes monitoring project recorded an extraordinary flash produced by the impact on the Moon of a large meteoroid at…

地球与行星天体物理 · 物理学 2014-02-25 Jose M. Madiedo , Jose L. Ortiz , Nicolas Morales , Jesus Cabrera-Caño

Dynamically linking a meteor shower with its parent body can be challenging. This is in part due to the limits of the tools available today (such as D-criteria) but is also due to the complex dynamics of meteoroid streams. We choose a…

地球与行星天体物理 · 物理学 2023-05-30 Ariane Courtot , Jérémie Vaubaillon , Marc Fouchard

The paper presents numerical models of mean-motion resonances detected in the Quadrantid meteoroid stream consisting of particles of mass 0.003 to 0.03 g, which helps to prove the presence of the following mean-motion resonances: the 1:9…

地球与行星天体物理 · 物理学 2023-10-12 Georgy E. Sambarov , Anna P. Kartashova , Tatyana Yu. Galushina

The gamma-ray activities of 33 meteorite samples (30 ordinary chondrites, 1 Mars meteorite, 1 iron, 1 howardite) collected during Omani-Swiss meteorite search campaigns 2001-2008 were nondestructively measured using an ultra-low background…

地球与行星天体物理 · 物理学 2017-05-31 Patrick Weber , Beda Hofmann , Tamer Tolba , Jean-Luc Vuilleumier

We have developed a statistical framework that uses collisional evolution models, shock physics modeling and scaling laws to determine the range of plausible collisional histories for individual meteorite parent bodies. It is likely that…

地球与行星天体物理 · 物理学 2013-09-11 Thomas M Davison , David P O'Brien , Fred J Ciesla , Gareth S Collins

Here we report on the results of meteor observations with 9-channel Mini-MegaTORTORA (MMT-9) wide-field optical monitoring system with high temporal resolution. During first 1.5 years of operation more than 90 thousands of meteors have been…

地球与行星天体物理 · 物理学 2016-02-26 S. Karpov , N. Orekhova , G. Beskin , A. Biryukov , S. Bondar , E. Ivanov , E. Katkova , A. Perkov , V. Sasyuk

This paper presents the results of a nearly two year long campaign to detect and analyze meteor persistent trains (PTs) - self-emitting phenomena which can linger up to an hour after their parent meteor. The modern understanding of PTs has…

地球与行星天体物理 · 物理学 2024-07-29 L. E. Cordonnier , K. S. Obenberger , J. M. Holmes , G. B. Taylor , D. Vida

We present a color-magnitude diagram (CMD) for a field in the giant tidal stream of the Andromeda galaxy (M31). These observations, taken with the Advanced Camera for Surveys on the Hubble Space Telescope, are 50% complete at V~30 mag,…

We present the identification and preliminary analysis of a dust trail following the orbit of (3200) Phaethon as seen in white light images recorded by the Wide-field Imager for Parker Solar Probe (WISPR) instrument on the NASA Parker Solar…