Jump to content
 







Main menu
   


Navigation  



Main page
Contents
Current events
Random article
About Wikipedia
Contact us
Donate
 




Contribute  



Help
Learn to edit
Community portal
Recent changes
Upload file
 








Search  

































Create account

Log in
 









Create account
 Log in
 




Pages for logged out editors learn more  



Contributions
Talk
 



















Contents

   



(Top)
 


1 Description  





2 Impact basins  





3 Relationship to Earth's geologic time scale  





4 See also  





5 References  





6 External links  














Pre-Nectarian






Brezhoneg
Català
Dansk
Español
Euskara
Français

Bahasa Indonesia
Italiano
Latina
Nederlands

Русский
Svenska
Українська
Tiếng Vit

 

Edit links
 









Article
Talk
 

















Read
Edit
View history
 








Tools
   


Actions  



Read
Edit
View history
 




General  



What links here
Related changes
Upload file
Special pages
Permanent link
Page information
Cite this page
Get shortened URL
Download QR code
Wikidata item
 




Print/export  



Download as PDF
Printable version
 
















Appearance
   

 






From Wikipedia, the free encyclopedia
 


Pre-Nectarian
4533 – 3920 Ma

I

N

E

C

Chronology
Usage information
Celestial bodyEarth's Moon
Time scale(s) usedLunar Geologic Timescale
Definition
Chronological unitPeriod

The pre-Nectarian period of the lunar geologic timescale runs from 4.533 billion years ago (the time of the initial formation of the Moon) to 3.920 billion years ago, when the Nectaris Basin was formed by a large impact. It is followed by the Nectarian period.

Description

[edit]

Pre-Nectarian rocks are rare in the lunar sample suite; they are mostly composed of lunar highlands material which have been heavily churned, brecciated, and thermally affected by subsequent impacts, particularly during the Heavy Bombardment Eon[1][2] (HBE; a period of 0.6-1 Gy from the formation of the Moon until at least the formation of the Imbrium Basin ~3.9 Ga, or even later with the formation of Orientale Basin) that marks the approximate beginning of the Nectarian period. The primary pre-Nectarian lunar highland material is dominated by the rock type anorthosite, which suggests that the early stage of lunar crustal formation occurred via mineral crystallization of a global magma ocean.

This geologic period has been informally subdivided into the Cryptic Era (4.533 - 4.172 Ga ago) and Basin Groups 1-9 (4.172 - 3.92 Ga ago),[3] but these divisions are not used on any geologic maps. Similarly the later period has also been called the Aitkenian period.

Early ImbrianLate ImbrianPre-NectarianNectarianEratosthenianCopernican period
Millions of years before present


Impact basins

[edit]
Lunar impact basins
as categorized by Wilhelms et al. (1987)[4]
Basin name Diameter Age-
group
(km) (nr.)
Procellarum 3,200 1
South Pole-Aitken 2,500
Tsiolkovskiy-Stark 700 2
Grissom-White 600
Insularum 600
Marginis 580
Flamsteed-Billy 570
Balmer-Kapteyn 550
Werner-Airy 500
Pingré-Hausen 300
Al-Khwarizmi / King 590
Fecunditatis 990 3
Australe 880
Tranquillitatis 800
Mutus-Vlacq 700
Nubium 690
Lomonosov-Fleming 620
Basin name Diameter Age-
group
(km) (nr.)
Ingenii 650 4
Poincaré 340
Keeler-Heaviside 780
Coulomb-Sarton 530 5
Smythii 840
Lorentz 360 6
Arnundsen-Ganswindt 355 7
Schiller-Zucchius 325
Planck 325
Birkhoff 330
Freundlich-Sharonov 600 8
Grimaldi 430 9
Apollo 505
For basins with no article, the two prominent
craters' names are separately linked to their
respective articles.
Names of proposed basins are italicized.
 

Relationship to Earth's geologic time scale

[edit]

Since little or no geological evidence on Earth exists from the time spanned by the pre-Nectarian period of the Moon, the pre-Nectarian has been used as a guide by at least one notable scientific work[5] to subdivide the unofficial terrestrial Hadean eon. In particular, it is sometimes found that the Hadean eon is subdivided into the Cryptic era, Basin Groups 1-9, Nectarian and Lower Imbrian, though the first two of these lunar divisions are informal and collectively make up the pre-Nectarian.

See also

[edit]

References

[edit]
  1. ^ Fernandes V. A., Fritz J., Weiss B., Garrick-Bethel and Shuster D. (2013) The bombardment history of the Moon as recorded by 40Ar-39Ar chronology. Meteor. and Planet. Sci. 48, 241–269. DOI: 10.1111/maps.12054.
  • ^ Fritz J., Bitsch B., Kührt E., Morbidelli A., Tornow C., Wünnemann K., Fernandes V.A., Grenfell L.J., Rauer H., Wagner R. and Werner S.C. (2014) Earth-like habitats in planetary systems. Planetary and Space Science 98, 254–267. https://dx.doi.org/ 10.1016/j.pss.2014.03.003i
  • ^ Don Wilhelms (1987). Geologic History of the Moon. U.S. Geological Survey Professional Paper 1348.
  • ^ Wilhelms, Don; McCauley, John; Trask, Newell (1987). The geologic history of the Moon. Professional Paper. US Geological Survey. p. 148. doi:10.3133/pp1348.
  • ^ W. Harland; R. Armstrong; A. Cox; L. Craig; A. Smith; D. Smith (1990). A Geologic time scale 1989. Cambridge University Press.
  • [edit]
    Retrieved from "https://en.wikipedia.org/w/index.php?title=Pre-Nectarian&oldid=1198524310"

    Categories: 
    Pre-Nectarian
    Hadean
    Hidden categories: 
    Pages using the EasyTimeline extension
    Articles with short description
    Short description matches Wikidata
    Webarchive template wayback links
     



    This page was last edited on 24 January 2024, at 09:58 (UTC).

    Text is available under the Creative Commons Attribution-ShareAlike License 4.0; additional terms may apply. By using this site, you agree to the Terms of Use and Privacy Policy. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc., a non-profit organization.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Mobile view



    Wikimedia Foundation
    Powered by MediaWiki