2018
DOI: 10.1002/2017gc007388
|View full text |Cite
|
Sign up to set email alerts
|

Origin of Light Noble Gases (He, Ne, and Ar) on Earth: A Review

Abstract: We review the different scenarios for the origin of light noble gases (He, Ne, and Ar) on Earth. Several sources could have contributed to the Earth's noble gas budget: implanted solar wind, solar nebula gas, chondrites, and comets. Although there is evidence for “solar‐like” neon in the Earth's mantle, questions remain as to its origin. A new compilation of noble gas data in lunar soils, interplanetary dust particles, micrometeorites, and solar wind allows examination of the implanted solar wind composition, … Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

3
6
0

Year Published

2019
2019
2024
2024

Publication Types

Select...
6
2

Relationship

1
7

Authors

Journals

citations
Cited by 25 publications
(13 citation statements)
references
References 136 publications
3
6
0
Order By: Relevance
“…units. Moreover, a plume imprint on geochemical signatures of Svartenhuk lavas is also consistent with the extremely primitive helium isotopic compositions recently published by Péron et al (2018) for olivines from our V3 samples S33E7 and S35E7 (R/Ra=31.0 and 34.9, respectively), similar to those previously reported for samples from Disko…”
Section: Mantle Source Heterogeneity and Its Temporal Evolutionsupporting
confidence: 92%
“…units. Moreover, a plume imprint on geochemical signatures of Svartenhuk lavas is also consistent with the extremely primitive helium isotopic compositions recently published by Péron et al (2018) for olivines from our V3 samples S33E7 and S35E7 (R/Ra=31.0 and 34.9, respectively), similar to those previously reported for samples from Disko…”
Section: Mantle Source Heterogeneity and Its Temporal Evolutionsupporting
confidence: 92%
“…Except for the deep mantle plume source, signatures of nebular gases are not found elsewhere on our planet. 20 Ne/ 22 Ne ratios in MORBs do not exceed ∼12.5 within the quoted uncertainties of the measurements , Parai et al 2012, Peron et al 2017, Raquin & Moreira 2009, Sarda et al 2000, Tucker et al 2012, which are similar to values of meteoritic material irradiated by the solar wind (e.g., Peron et al 2017Peron et al , 2018. The maximum measured MORB values are similar to an independent estimate of 12.49 ± 0.04 for the MORB source based on continental well gases (Ballentine et al 2005, Holland & Ballentine 2006.…”
Section: Figuresupporting
confidence: 78%
“…Large differences in the primordial Ne isotopic ratio ( 20 Ne/ 22 Ne) among potential sources of Earth's volatiles make Ne a key player in understanding the history of volatile accretion (Ballentine et al 2005;Marty 1989;Moreira 2013;Mukhopadhyay 2012;Peron et al 2017Peron et al , 2018Raquin & Moreira 2009;Yokochi & Marty 2004). The three potential sources of volatiles during the main phase of Earth's accretion are nebular gases, solar wind irradiated meteoritic material, and CI chondrite meteorites.…”
Section: Volatile Sources For the Mantlementioning
confidence: 99%
“…Another possible origin of terrestrial N arises from the combined study of N isotopes and noble gases among solar system bodies. Based on the solar-like Ne isotopic composition of the mantle, Marty (76) discussed the possibility that the mantle has preserved some solar N. This scenario implies that precursor grains accreted during Earth’s formation were first irradiated by the solar wind and preserved their solar volatile isotopic signature during Earth’s accretion and differentiation [δ 15 N IFSW ≤ −240‰; IFSW: implantation-fractionated solar wind (84, 85)]. Alternatively, a primordial solar atmosphere could have been captured by Earth’s gravity and dissolved into the early magma ocean [δ 15 N solar = −383‰ (e.g., ref.…”
Section: On the Origin(s) And Evolution Of Terrestrial Nmentioning
confidence: 99%