[go: nahoru, domu]

Jump to content

Boltysh crater: Difference between revisions

Coordinates: 48°45′N 32°10′E / 48.750°N 32.167°E / 48.750; 32.167
From Wikipedia, the free encyclopedia
Content deleted Content added
No edit summary
Citation bot (talk | contribs)
Add: s2cid, date, website. | Use this bot. Report bugs. | Suggested by AManWithNoPlan | #UCB_toolbar
 
(12 intermediate revisions by 7 users not shown)
Line 1: Line 1:
{{Short description|Asteroid mpact, Kirovohrad Oblast, Ukraine}}
{{Infobox terrestrial impact site
{{Infobox terrestrial impact site
| name = Boltysh crater
| name = Boltysh crater
Line 33: Line 34:
}}
}}
[[File:Boltysh crater location map.png|thumb|right|250px|Location of the Boltysh crater]]
[[File:Boltysh crater location map.png|thumb|right|250px|Location of the Boltysh crater]]
The '''Boltysh crater''' or '''Bovtyshka crater''' is a buried [[impact crater]] in the [[Kirovohrad Oblast]] of [[Ukraine]],<ref name=EIDBoltysh>[http://www.passc.net/EarthImpactDatabase/New%20website_05-2018/Boltysh.html Boltysh at EID]</ref> near the village of Bovtyshka. The crater is {{convert|24|km|mi}} in [[diameter]] and its age of 65.39 ± 0.14/0.16 million years, based on [[Argon–argon dating|argon-argon dating]] techniques, less than 1 million years younger than [[Chicxulub crater]] in Mexico and the [[Cretaceous–Paleogene boundary]] (K–Pg boundary). The Chicxulub impact is believed to have caused the [[mass extinction]] at the end of the [[Cretaceous]] period, which included the extinction of the non-avian [[dinosaur]]s. Unlike the Chicxulub impact's effects, a 2021 study suggests that the Boltysh impact "did not factor into the apocalyptic die-off of the dinosaurs."<ref name="mystery">{{cite web|title=A Mysterious Craters Age May Add Clues to the Dinosaur Extinction |url=https://www.msn.com/en-us/news/technology/a-mysterious-craters-age-may-add-clues-to-the-dinosaur-extinction/ar-AALbXEk?li=BBnb7Kz}}</ref>
The '''Boltysh crater''' or '''Bovtyshka crater''' is a buried [[impact crater]] in the [[Kirovohrad Oblast]] of [[Ukraine]],<ref name=EIDBoltysh>[http://www.passc.net/EarthImpactDatabase/New%20website_05-2018/Boltysh.html Boltysh at EID]</ref> near the village of Bovtyshka. The crater is {{convert|24|km|mi}} in [[diameter]] and its age of 65.39 ± 0.14/0.16 million years, based on [[Argon–argon dating|argon-argon dating]] techniques, less than 1 million years younger than [[Chicxulub crater]] in [[Mexico]] and the [[Cretaceous–Paleogene boundary]] (K–Pg boundary). The Chicxulub impact is believed to have caused the [[mass extinction]] at the end of the [[Cretaceous]] period, which included the extinction of the non-avian [[dinosaur]]s. The Boltysh crater is currently thought to be unrelated to the Chicxulub impact, and to have not generated major global environmental effects.<ref name="mystery">{{cite web|title=A Mysterious Crater's Age May Add Clues to the Dinosaur Extinction |website=[[The New York Times]] |url=https://www.nytimes.com/2021/06/18/science/boltysh-crater-dinosaurs.html}}</ref>


== Overview ==
== Overview ==
Line 41: Line 42:


== Age ==
== Age ==
When first identified, the age of the crater could only be roughly constrained between the age of the impacted rocks (the target) and the age of overlying sediments. The target rocks date from the [[Cenomanian]] (98.9 to 93.5 million years ago) and [[Turonian]] (93.5 to 89 million years ago) epochs. Bore samples of sediments overlying the crater contain fossils dating from the [[Paleocene]] epoch, 66 to 54.8 million years ago. The age of the crater was thus constrained to between 54 and 98 million years.
The Boltysh depression was identified as a fossil meteorite crater by 1975.<ref>{{cite journal |vauthors=((Yurk YuYu)), Yeremko GK, ((Polkanov YuA)) |title=The Boltysh depression-a fossil meteorite crater |journal=Sov Geol |date=1975 |volume=2 |page=138-144}}</ref> By 1987, it was dated to 100 ± 12 million years old.<ref name="Grieve et al.">{{cite journal |last1=Grieve |first1=R.A.F. |last2=Reny |first2=G. |last3=Gurov |first3=E.P. |last4=Ryabenko |first4=Z. |title=The melt rocks of the Boltysh impact crater, Ukraine, USSR |journal=Contributions to Mineralogy and Petrology |date=1987 |volume=96 |page=56 |doi=10.1007/BF00375525|s2cid=140563900 }}</ref> Early age estimates could only be roughly constrained between the age of the impacted rocks (the target) and the age of overlying sediments. The target rocks date from the [[Cenomanian]] (98.9 to 93.5 million years ago) and [[Turonian]] (93.5 to 89 million years ago) epochs. Bore samples of sediments overlying the crater contain fossils dating from the [[Paleocene]] epoch, 66 to 54.8 million years ago. The age of the crater was thus constrained to between 54 and 98 million years.


Subsequent [[radiometric dating]] reduced the uncertainty. The concentration of {{chem|U|238|link=uranium-238}} decay products in impact glasses from the crater were used to derive an age of 65.04 ± 1.10 million years. [[Argon-argon dating|Analysis of argon radioactive decay products]] yielded an age of 65.17 ± 0.64 million years.<ref name=Kelley-2002>{{Cite journal |last1=Kelley|first1=Simon P.|last2=Gurov|first2=Eugene|date=August 2002 |title=Boltysh, another end-Cretaceous impact|journal=Meteoritics & Planetary Science|volume=37|issue=8|pages=1031–1043|doi=10.1111/j.1945-5100.2002.tb00875.x|bibcode=2002M&PS...37.1031K|issn=1086-9379|doi-access=free}}</ref> These ages are similar to that of [[Chicxulub Crater]] which [[argon–argon dating]] yielded an age of 66.043 ± 0.011 million years.
Subsequent [[radiometric dating]] reduced the uncertainty. The concentration of {{chem|U|238|link=uranium-238}} decay products in impact glasses from the crater were used to derive an age of 65.04 ± 1.10 million years. A 2002 [[Argon-argon dating|analysis of argon radioactive decay products]] yielded an age of 65.17 ± 0.64 million years.<ref name=Kelley-2002>{{Cite journal |last1=Kelley|first1=Simon P.|last2=Gurov|first2=Eugene|date=August 2002 |title=Boltysh, another end-Cretaceous impact|journal=Meteoritics & Planetary Science|volume=37|issue=8|pages=1031–1043|doi=10.1111/j.1945-5100.2002.tb00875.x|bibcode=2002M&PS...37.1031K|issn=1086-9379|doi-access=free}}</ref> While these radiometric dating measurements place the Boltysh crater hundreds of thousands of years after the Chicxulub crater, a 2010 radiometric and [[palynological]] study of fern spore ([[fern spike]]s) abundance suggested the Boltysh impact may have occurred several thousand years before Chicxulub.<ref>{{Cite journal|last1=Jolley|first1=David|last2=Gilmour|first2=Iain|last3=Gurov|first3=Eugene|last4=Kelley|first4=Simon|last5=Watson|first5=Jonathan|date=September 2010|title=Two large meteorite impacts at the Cretaceous-Paleogene boundary|url=http://pubs.geoscienceworld.org/geology/article/38/9/835/130359/Two-large-meteorite-impacts-at-the|journal=Geology|language=en|volume=38|issue=9|pages=835–838|doi=10.1130/G31034.1|bibcode=2010Geo....38..835J|s2cid=120172960 |issn=1943-2682}}</ref> However, in response, a follow-up study in 2021 estimated using argon–argon dating that Boltysh formed about 65.39 ± 0.14/0.16 million years ago, 650,000 years after the Chicxulub catastrophe, and suggested that the fern spike was plausibly a result of the impact itself. The authors of the paper suggested that the impact may have disrupted recovery after the K/Pg extinction.<ref name="Pickerg-2021">{{Cite journal |last1=Pickersgill|first1=Annemarie E. |last2=Mark|first2=Darren F. |last3=Lee|first3=Martin R. |last4=Kelley|first4=Simon P. |last5=Jolley|first5=David W. |date=2021-06-01 |title=The Boltysh impact structure: An early Danian impact event during recovery from the K-Pg mass extinction|journal=Science Advances|language=en|volume=7|issue=25|pages=eabe6530|doi=10.1126/sciadv.abe6530|issn=2375-2548|pmid=34144979|pmc=8213223|bibcode=2021SciA....7.6530P|doi-access=free}}</ref>

While these radiometric dating measurements place the Boltysh crater thousands of years after the Chicxulub crater, an August 2010 radiometric and [[palynological]] study of fern spore ([[fern spike]]s) abundance suggested the Boltysh impact may have occurred several thousand years before Chicxulub.<ref>{{Cite journal|last1=Jolley|first1=David|last2=Gilmour|first2=Iain|last3=Gurov|first3=Eugene|last4=Kelley|first4=Simon|last5=Watson|first5=Jonathan|date=September 2010|title=Two large meteorite impacts at the Cretaceous-Paleogene boundary|url=http://pubs.geoscienceworld.org/geology/article/38/9/835/130359/Two-large-meteorite-impacts-at-the|journal=Geology|language=en|volume=38|issue=9|pages=835–838|doi=10.1130/G31034.1|bibcode=2010Geo....38..835J|issn=1943-2682}}</ref>
However, in response, a follow-up study in June 2021 estimated using argon–argon dating that Boltysh formed about 65.39 ± 0.14/0.16 million years ago, 650,000 years after the Chicxulub catastrophe, suggesting that the fern spike was plausibly a result of the impact itself. The authors of the paper suggested that the impact may have disrupted recovery after the K/Pg extinction.<ref name=Pickerg-2021>{{Cite journal |last1=Pickersgill|first1=Annemarie E. |last2=Mark|first2=Darren F. |last3=Lee|first3=Martin R. |last4=Kelley|first4=Simon P. |last5=Jolley|first5=David W. |date=2021-06-01 |title=The Boltysh impact structure: An early Danian impact event during recovery from the K-Pg mass extinction|journal=Science Advances|language=en|volume=7|issue=25|pages=eabe6530|doi=10.1126/sciadv.abe6530|issn=2375-2548|pmid=34144979|pmc=8213223|bibcode=2021SciA....7.6530P|doi-access=free}}</ref>


== References ==
== References ==
Line 61: Line 59:


{{commons category|Boltysh crater}}
{{commons category|Boltysh crater}}
{{Portal bar|Astronomy|Geology|Ukraine}}
{{KT boundary}}
{{KT boundary}}
{{Impact cratering on Earth}}
{{Impact cratering on Earth}}
Line 66: Line 65:
{{DEFAULTSORT:Boltysh Crater}}
{{DEFAULTSORT:Boltysh Crater}}
[[Category:Impact craters of Ukraine]]
[[Category:Impact craters of Ukraine]]
[[Category:Paleocene impact craters]]
[[Category:Geography of Kirovohrad Oblast]]
[[Category:Geography of Kirovohrad Oblast]]
[[Category:Paleocene impact craters]]
[[Category:Cretaceous–Paleogene boundary]]

Latest revision as of 18:21, 29 August 2023

Boltysh crater
Boltysh crater is located in Ukraine
Boltysh crater
Location in Ukraine
Impact crater/structure
ConfidenceConfirmed[1]
Diameter24 kilometres (15 mi)
Depth550 metres (1,800 ft)
Age65.39 ± 0.14/0.16 mya, Danian
ExposedNo
DrilledYes
Location
Coordinates48°45′N 32°10′E / 48.750°N 32.167°E / 48.750; 32.167
CountryUkraine
RegionKirovohrad Oblast
Location of the Boltysh crater

The Boltysh crater or Bovtyshka crater is a buried impact crater in the Kirovohrad Oblast of Ukraine,[1] near the village of Bovtyshka. The crater is 24 kilometres (15 mi) in diameter and its age of 65.39 ± 0.14/0.16 million years, based on argon-argon dating techniques, less than 1 million years younger than Chicxulub crater in Mexico and the Cretaceous–Paleogene boundary (K–Pg boundary). The Chicxulub impact is believed to have caused the mass extinction at the end of the Cretaceous period, which included the extinction of the non-avian dinosaurs. The Boltysh crater is currently thought to be unrelated to the Chicxulub impact, and to have not generated major global environmental effects.[2]

Overview

[edit]

Boltysh crater is located in central Ukraine, in the basin of the Tiasmyn River, a tributary of the Dnieper River. It is 24 kilometres (15 mi) in diameter, and is surrounded by an ejecta blanket of breccia preserved over an area of 6,500 square kilometres (2,500 sq mi). It is estimated that immediately after the impact, ejecta covered an area of 25,000 square kilometres (9,700 sq mi) to a depth of 1 metre (3.3 ft) or greater, and was some 600 metres (2,000 ft) deep at the crater rim.

The crater contains a central uplift about 6 kilometres (3.7 mi) in diameter, rising about 550 metres (1,800 ft) above the base level of the crater. This uplift currently lies beneath about 500 metres (1,600 ft) of sediment deposited since the impact, and was discovered in the 1960s during oil shale deposits exploration.

Age

[edit]

The Boltysh depression was identified as a fossil meteorite crater by 1975.[3] By 1987, it was dated to 100 ± 12 million years old.[4] Early age estimates could only be roughly constrained between the age of the impacted rocks (the target) and the age of overlying sediments. The target rocks date from the Cenomanian (98.9 to 93.5 million years ago) and Turonian (93.5 to 89 million years ago) epochs. Bore samples of sediments overlying the crater contain fossils dating from the Paleocene epoch, 66 to 54.8 million years ago. The age of the crater was thus constrained to between 54 and 98 million years.

Subsequent radiometric dating reduced the uncertainty. The concentration of U
238
decay products in impact glasses from the crater were used to derive an age of 65.04 ± 1.10 million years. A 2002 analysis of argon radioactive decay products yielded an age of 65.17 ± 0.64 million years.[5] While these radiometric dating measurements place the Boltysh crater hundreds of thousands of years after the Chicxulub crater, a 2010 radiometric and palynological study of fern spore (fern spikes) abundance suggested the Boltysh impact may have occurred several thousand years before Chicxulub.[6] However, in response, a follow-up study in 2021 estimated using argon–argon dating that Boltysh formed about 65.39 ± 0.14/0.16 million years ago, 650,000 years after the Chicxulub catastrophe, and suggested that the fern spike was plausibly a result of the impact itself. The authors of the paper suggested that the impact may have disrupted recovery after the K/Pg extinction.[7]

References

[edit]
  1. ^ a b Boltysh at EID
  2. ^ "A Mysterious Crater's Age May Add Clues to the Dinosaur Extinction". The New York Times.
  3. ^ Yurk YuYu, Yeremko GK, Polkanov YuA (1975). "The Boltysh depression-a fossil meteorite crater". Sov Geol. 2: 138-144.
  4. ^ Grieve, R.A.F.; Reny, G.; Gurov, E.P.; Ryabenko, Z. (1987). "The melt rocks of the Boltysh impact crater, Ukraine, USSR". Contributions to Mineralogy and Petrology. 96: 56. doi:10.1007/BF00375525. S2CID 140563900.
  5. ^ Kelley, Simon P.; Gurov, Eugene (August 2002). "Boltysh, another end-Cretaceous impact". Meteoritics & Planetary Science. 37 (8): 1031–1043. Bibcode:2002M&PS...37.1031K. doi:10.1111/j.1945-5100.2002.tb00875.x. ISSN 1086-9379.
  6. ^ Jolley, David; Gilmour, Iain; Gurov, Eugene; Kelley, Simon; Watson, Jonathan (September 2010). "Two large meteorite impacts at the Cretaceous-Paleogene boundary". Geology. 38 (9): 835–838. Bibcode:2010Geo....38..835J. doi:10.1130/G31034.1. ISSN 1943-2682. S2CID 120172960.
  7. ^ Pickersgill, Annemarie E.; Mark, Darren F.; Lee, Martin R.; Kelley, Simon P.; Jolley, David W. (2021-06-01). "The Boltysh impact structure: An early Danian impact event during recovery from the K-Pg mass extinction". Science Advances. 7 (25): eabe6530. Bibcode:2021SciA....7.6530P. doi:10.1126/sciadv.abe6530. ISSN 2375-2548. PMC 8213223. PMID 34144979.

Further reading

[edit]
  • Grieve, R. A. F., Reny, G., Gurov, E. P., & Ryabenko, V. A. (1987). The melt rocks of the Boltysh impact crater, Ukraine, USSR. Contributions to Mineralogy and Petrology, 96(1), 56–62.
  • Grieve R.A.F., Reny G., Gurov, E.P., Ryabenko V. A. (1985), Impact Melt Rocks of the Boltysh Crater, Meteoritics, v. 20, p. 655
  • Gurov, E. P., Kelley, S. P., Koeberl, C., & Dykan, N. I. (2006). Sediments and impact rocks filling the Boltysh impact crater. In Biological processes associated with impact events (pp. 335–358). Springer Berlin Heidelberg.
  • Gurov E.P., Gurova H.P. (1985), Boltysh Astrobleme: Impact Crater Pattern with a Central Uplift, Lunar & Planetary Science XVI, pp. 310–311
  • Jolley D., Gilmour I., Gurov E., Kelley S., Watson J. (2010) Two large meteorite impacts at the Cretaceous-Paleogene boundary Geology September 2010, v. 38, pp. 835–838, doi:10.1130/G31034.1
  • Kashkarov L.L., Nazarov M.A., Lorents K.A., Kalinina G.V., Kononkova N.N. (1999), The Track Age of the Boltysh Impact Structure, Astronomicheskii Vestnik, v. 33, p. 253
  • Kelley S.P., Gurov E. (2002), The Boltysh, another end-Cretaceous impact, Meteoritics & Planetary Science, v. 37, pp. 1031–1043