All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

Ejection velocities, age, and formation process of SPE meteoroid cluster

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00563699" target="_blank" >RIV/67985815:_____/22:00563699 - isvavai.cz</a>

  • Result on the web

    <a href="https://hdl.handle.net/11104/0337521" target="_blank" >https://hdl.handle.net/11104/0337521</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/202243055" target="_blank" >10.1051/0004-6361/202243055</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Ejection velocities, age, and formation process of SPE meteoroid cluster

  • Original language description

    The goal is to determine ejection velocities of the cluster members and SPE's age, as well as to estimate the most probable formation process. Authors determined mutual positions and masses of all meteoroids including the errors. They assumed that the massdominated meteoroid is the parent body of the cluster and that the observed positions of meteoroids are controlled by the ejection velocities and the action of solar radiation pressure. A formula for the dependence of meteoroid ejection velocities on the mutual positions, masses, and cluster age was derived. It was assumed that the time at which the initial kinetic energy of all meteoroids reached a minimum value corresponds to the age of the cluster. Knowing values and directions of ejection velocities together with meteoroid masses then allowed us to determine the most likely process of cluster formation.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GA20-10907S" target="_blank" >GA20-10907S: Meteor clusters: An evidence for fragmentation of meteoroids in interplanetary space</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2022

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astronomy & Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

    1432-0746

  • Volume of the periodical

    666

  • Issue of the periodical within the volume

    October

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    10

  • Pages from-to

    A144

  • UT code for WoS article

    000870425900002

  • EID of the result in the Scopus database