Guoqiang Tang

Dr. Guoqiang Tang

orcid

Research Focus & Metrics

Academic Career Length

13Years (2014-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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19 October 2021 in Nature
Verified
Journal Article
Open access
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QLQiuli Li
Qiuli Li
QZQin Zhou
Qin Zhou
YLYu Liu
Yu Liu
ZXZhiyong Xiao
Zhiyong Xiao
YLYangting Lin
Yangting Lin
XLXian-Hua Li
Xian-Hua Li
The Moon has a magmatic and thermal history that is distinct from that of the terrestrial planets1. Radioisotope dating of lunar samples suggests that most lunar basaltic magmatism ceased by around 2.9–2.8 billion years ago (Ga)2,3, although younger basalts between 3 Ga and 1 Ga have been suggested by crater-counting chronology, which has large uncertainties owing to the lack of returned samples for calibration4,5. Here we report a precise lead–lead age of 2,030 ± 4 million years ago for basalt clasts returned by the Chang’e-5 mission, and a 238U/204Pb ratio (µ value)6 of about 680 for a source that evolved through two stages of differentiation. This is the youngest crystallization age reported so far for lunar basalts by radiometric dating, extending the duration of lunar volcanism by approximately 800–900 million years. The µ value of the Chang’e-5 basalt mantle source is within the range of low-titanium and high-titanium basalts from Apollo sites (µ value of about 300–1,000), but notably lower than those of potassium, rare-earth elements and phosphorus (KREEP) and high-aluminium basalts7 (µ value of about 2,600–3,700), indicating that the Chang’e-5 basalts were produced by melting of a KREEP-poor source. This age provides a pivotal calibration point for crater-counting chronology in the inner Solar System and provides insight on the volcanic and thermal history of the Moon.

11 June 2021 in Geostandards and Geoanalytical Research
Verified
Journal Article
Closed access
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SWShitou Wu
Shitou Wu
YYYueheng Yang
Yueheng Yang
KJKlaus Peter Jochum
Klaus Peter Jochum
RRRolf L. Romer
Rolf L. Romer
JGJohannes Glodny
Johannes Glodny
FWFuyuan Wu
Fuyuan Wu

6 September 2024 in Science
Verified
Journal Article
Closed access
BWBi-Wen Wang
Bi-Wen Wang
QZQian W. L. Zhang
Qian W. L. Zhang
Yi ChenYi Chen
Yi Chen
WZWenhao Zhao
Wenhao Zhao
YLYu Liu
Yu Liu
QLQiuli Li
Qiuli Li
There is extensive geologic evidence of ancient volcanic activity on the Moon, but it is unclear how long that volcanism persisted. Magma fountains produce volcanic glasses, which have previously been found in samples of the Moon’s surface. We investigated ~3000 glass beads in lunar soil samples collected by the Chang’e-5 mission and identified three as having a volcanic origin on the basis of their textures, chemical compositions, and sulfur isotopes. Uranium-lead dating of the three volcanic glass beads shows that they formed 123 ± 15 million years ago. We measured high abundances of rare earth elements and thorium in these volcanic glass beads, which could indicate that such recent volcanism was related to local enrichment of heat-generating elements in the mantle sources of the magma.

23 April 2021 in Meteoritics & Planetary Science
Verified
Journal Article
Closed access
PDF file
PJPeter Jenniskens
Peter Jenniskens
MGMohutsiwa Gabadirwe
Mohutsiwa Gabadirwe
QYQing‐Zhu Yin
Qing‐Zhu Yin
APAlexander Proyer
Alexander Proyer
OMOliver Moses
Oliver Moses
KBKoketso Botepe
Koketso Botepe

17 March 2019 in Meteoritics & Planetary Science
Verified
Journal Article
Closed access
PDF file
OUOzan Unsalan
Ozan Unsalan
PJPeter Jenniskens
Peter Jenniskens
QYQing‐Zhu Yin
Qing‐Zhu Yin
EKErsin Kaygısız
Ersin Kaygısız
JAJim Albers
Jim Albers
(C(The Sariçiçek Meteorite Consortium)
(The Sariçiçek Meteorite Consortium)

20 January 2019 in Meteoritics & Planetary Science
Verified
Journal Article
Closed access
PDF file
PJPeter Jenniskens
Peter Jenniskens
JUJason Utas
Jason Utas
QYQing‐Zhu Yin
Qing‐Zhu Yin
RMRobert D. Matson
Robert D. Matson
MFMarc Fries
Marc Fries
(C(The Creston Meteorite Consortium)
(The Creston Meteorite Consortium)