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Quantification of Near-Earth Objects Between 1990-2021: An Overview

Received: 31 May 2023    Accepted: 19 June 2023    Published: 27 June 2023
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Abstract

In this work, the quantification of Near-Earth Object (NEO) has been carried out between 1990 to 2021. The emphasis is to examine the total number NEO discovered, the relationship between them and the earth-orbit especially with respect to their magnitude and distance (objects, aphelion and perihelion). Three categories of data (Amors, Apollos and Atens) were sourced from Minor Planet Center data repository (minorplanetcenter.net//iau/lists/Unusual.html), based on their orbital revolution and the pattern. Exploratory data analysis (EDA) of 5700 NEOs samples using python analytics was carried out and the result shows the average distribution of minimum distance between earth-orbit and NEOs. The result also shows yearly distribution of mean distance and magnitude. Furthermore, out of the 5700 NEOs analyzed, 22.9% were found to be potentially hazardous asteroids (PHAs) with higher possibility of an encounter with the earth, found at 0.01AU distance from the earth-orbit.

Published in American Journal of Astronomy and Astrophysics (Volume 10, Issue 1)
DOI 10.11648/j.ajaa.20231001.12
Page(s) 9-13
Creative Commons

This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.

Copyright

Copyright © The Author(s), 2024. Published by Science Publishing Group

Keywords

Quantification, Near-Earth Object, Earth-Orbit, Asteroids

References
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[3] Binzel, R. P., Morbidelli, A., Merouane, S., DeMeo, F. E., Birlan, M., Vernazza, P.,... & Tokunaga, A. T. (2010). Earth encounters as the origin of fresh surfaces on near-Earth asteroids. Nature, 463 (7279), 331-334.
[4] Popova, O. P., Jenniskens, P., Emel’yanenko, V., Kartashova, A., Biryukov, E., Khaibrakhmanov, S.,... & Chelyabinsk Airburst Consortium). (2013). Chelyabinsk airburst, damage assessment, meteorite recovery, and characterization. Science, 342 (6162), 1069-1073.
[5] Delbo’, M., Walsh, K., Bolin, B., Avdellidou, C., & Morbidelli, A. (2017). Identification of a primordial asteroid family constrains the original planetesimal population. Science, 357 (6355), 1026-1029.
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[7] Binzel, R. P., Reddy, V., & Dunn, T. L. (2015). The Near-Earth Object Population: Connections to Comets. Main-Belt Asteroids, and Meteorites, 243-256.
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[10] Perna, D., Barucci, M. A., Drube, L., Falke, A., Fulchignoni, M., Harris, A. W., & Kanuchova, Z. (2015). A global response roadmap to the asteroid impact threat: the NEOShield perspective. Planetary and Space Science, 118, 311-317.
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[12] Schweickart, R. L. (2009). Decision program on asteroid threat mitigation. Acta Astronautica, 65 (9-10), 1402-1408.
[13] Mainzer, A., Grav, T., Masiero, J., Bauer, J., Wright, E., Cutri, R. M.,... & Eisenhardt, P. (2011). Thermal model calibration for minor planets observed with wide-field infrared survey explorer/NEOWISE. The Astrophysical Journal, 736 (2), 100.
[14] Ipatov, S. I., & Mather, J. C. (2004). Comet and asteroid hazard to the terrestrial planets. Advances in Space Research, 33 (9), 1524-1533.
[15] Tricarico, P. (2017). The near-Earth asteroid population from two decades of observations. Icarus, 284, 416-423.
[16] Galache, J. L., Beeson, C. L., McLeod, K. K., & Elvis, M. (2015). The need for speed in Near-Earth Asteroid characterization. Planetary and Space Science, 111, 155-166.
Cite This Article
  • APA Style

    Osuji Emmanuel Uchenna, Ugwu Monday, Aernan Andofa, Ojima Ocheni, Aneke Ukpabi, et al. (2023). Quantification of Near-Earth Objects Between 1990-2021: An Overview. American Journal of Astronomy and Astrophysics, 10(1), 9-13. https://doi.org/10.11648/j.ajaa.20231001.12

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    ACS Style

    Osuji Emmanuel Uchenna; Ugwu Monday; Aernan Andofa; Ojima Ocheni; Aneke Ukpabi, et al. Quantification of Near-Earth Objects Between 1990-2021: An Overview. Am. J. Astron. Astrophys. 2023, 10(1), 9-13. doi: 10.11648/j.ajaa.20231001.12

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    AMA Style

    Osuji Emmanuel Uchenna, Ugwu Monday, Aernan Andofa, Ojima Ocheni, Aneke Ukpabi, et al. Quantification of Near-Earth Objects Between 1990-2021: An Overview. Am J Astron Astrophys. 2023;10(1):9-13. doi: 10.11648/j.ajaa.20231001.12

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  • @article{10.11648/j.ajaa.20231001.12,
      author = {Osuji Emmanuel Uchenna and Ugwu Monday and Aernan Andofa and Ojima Ocheni and Aneke Ukpabi and Wash Albert and Madike Emeka Michael and Justus Chukwunonyerem and Okolo Obinna and Okoro Emmanuel Chineche and Okpara Richard Tobechi and Vincent Osinachi Ezinwa and Ekechukwu Uzoamaka and Obasi Rita Chioma and Ezenwukwa Nnenna Dorathy},
      title = {Quantification of Near-Earth Objects Between 1990-2021: An Overview},
      journal = {American Journal of Astronomy and Astrophysics},
      volume = {10},
      number = {1},
      pages = {9-13},
      doi = {10.11648/j.ajaa.20231001.12},
      url = {https://doi.org/10.11648/j.ajaa.20231001.12},
      eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajaa.20231001.12},
      abstract = {In this work, the quantification of Near-Earth Object (NEO) has been carried out between 1990 to 2021. The emphasis is to examine the total number NEO discovered, the relationship between them and the earth-orbit especially with respect to their magnitude and distance (objects, aphelion and perihelion). Three categories of data (Amors, Apollos and Atens) were sourced from Minor Planet Center data repository (minorplanetcenter.net//iau/lists/Unusual.html), based on their orbital revolution and the pattern. Exploratory data analysis (EDA) of 5700 NEOs samples using python analytics was carried out and the result shows the average distribution of minimum distance between earth-orbit and NEOs. The result also shows yearly distribution of mean distance and magnitude. Furthermore, out of the 5700 NEOs analyzed, 22.9% were found to be potentially hazardous asteroids (PHAs) with higher possibility of an encounter with the earth, found at 0.01AU distance from the earth-orbit.},
     year = {2023}
    }
    

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    T1  - Quantification of Near-Earth Objects Between 1990-2021: An Overview
    AU  - Osuji Emmanuel Uchenna
    AU  - Ugwu Monday
    AU  - Aernan Andofa
    AU  - Ojima Ocheni
    AU  - Aneke Ukpabi
    AU  - Wash Albert
    AU  - Madike Emeka Michael
    AU  - Justus Chukwunonyerem
    AU  - Okolo Obinna
    AU  - Okoro Emmanuel Chineche
    AU  - Okpara Richard Tobechi
    AU  - Vincent Osinachi Ezinwa
    AU  - Ekechukwu Uzoamaka
    AU  - Obasi Rita Chioma
    AU  - Ezenwukwa Nnenna Dorathy
    Y1  - 2023/06/27
    PY  - 2023
    N1  - https://doi.org/10.11648/j.ajaa.20231001.12
    DO  - 10.11648/j.ajaa.20231001.12
    T2  - American Journal of Astronomy and Astrophysics
    JF  - American Journal of Astronomy and Astrophysics
    JO  - American Journal of Astronomy and Astrophysics
    SP  - 9
    EP  - 13
    PB  - Science Publishing Group
    SN  - 2376-4686
    UR  - https://doi.org/10.11648/j.ajaa.20231001.12
    AB  - In this work, the quantification of Near-Earth Object (NEO) has been carried out between 1990 to 2021. The emphasis is to examine the total number NEO discovered, the relationship between them and the earth-orbit especially with respect to their magnitude and distance (objects, aphelion and perihelion). Three categories of data (Amors, Apollos and Atens) were sourced from Minor Planet Center data repository (minorplanetcenter.net//iau/lists/Unusual.html), based on their orbital revolution and the pattern. Exploratory data analysis (EDA) of 5700 NEOs samples using python analytics was carried out and the result shows the average distribution of minimum distance between earth-orbit and NEOs. The result also shows yearly distribution of mean distance and magnitude. Furthermore, out of the 5700 NEOs analyzed, 22.9% were found to be potentially hazardous asteroids (PHAs) with higher possibility of an encounter with the earth, found at 0.01AU distance from the earth-orbit.
    VL  - 10
    IS  - 1
    ER  - 

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Author Information
  • National Space Research and Development Agency-Center for Basic Space Science, University of Nigeria, Enugu, Nigeria

  • National Space Research and Development Agency-Center for Basic Space Science, University of Nigeria, Enugu, Nigeria

  • National Space Research and Development Agency-Center for Basic Space Science, University of Nigeria, Enugu, Nigeria

  • National Space Research and Development Agency-Center for Basic Space Science, University of Nigeria, Enugu, Nigeria

  • National Space Research and Development Agency-Center for Basic Space Science, University of Nigeria, Enugu, Nigeria

  • National Space Research and Development Agency-Center for Basic Space Science, University of Nigeria, Enugu, Nigeria

  • National Space Research and Development Agency-Center for Basic Space Science, University of Nigeria, Enugu, Nigeria

  • National Space Research and Development Agency-Center for Basic Space Science, University of Nigeria, Enugu, Nigeria

  • National Space Research and Development Agency-Center for Basic Space Science, University of Nigeria, Enugu, Nigeria

  • National Space Research and Development Agency-Center for Basic Space Science, University of Nigeria, Enugu, Nigeria

  • National Space Research and Development Agency-Center for Basic Space Science, University of Nigeria, Enugu, Nigeria

  • National Space Research and Development Agency-Center for Basic Space Science, University of Nigeria, Enugu, Nigeria

  • National Space Research and Development Agency-Center for Basic Space Science, University of Nigeria, Enugu, Nigeria

  • National Space Research and Development Agency-Center for Basic Space Science, University of Nigeria, Enugu, Nigeria

  • National Space Research and Development Agency-Center for Basic Space Science, University of Nigeria, Enugu, Nigeria

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