Editing Pyroclastic flow (section)

===On other celestial bodies===
In 1963, NASA astronomer [[Winifred Cameron]] proposed that the lunar equivalent of terrestrial pyroclastic flows may have formed sinuous [[rille]]s on the [[Moon]]. In a lunar volcanic eruption, a pyroclastic cloud would follow local relief, resulting in an often sinuous track. The Moon's [[Schroter's Valley|Schröter's Valley]] offers one example.<ref>
{{cite journal | last1 = Cameron | first1 = W. S. | year = 1964 
| title = An Interpretation of Schröter's Valley and Other Lunar Sinuous Rills 
| journal = [[Journal of Geophysical Research]] | volume = 69 | issue = 12
| pages = 2423–2430 | doi = 10.1029/JZ069i012p02423 
| bibcode=1964JGR....69.2423C
}}
</ref>{{Primary source inline|date=July 2019}}
Some volcanoes on [[Mars]], such as [[Tyrrhenus Mons]] and [[Hadriacus Mons]], have produced layered deposits that appear to be more easily eroded than lava flows, suggesting that they were emplaced by pyroclastic flows.<ref>{{cite book |last1=Zimbelman |first1=James R. |last2=Garry |first2=William Brent |last3=Bleacher |first3=Jacob Elvin |last4=Crown |first4=David A. |editor1-last=Sigurdsson |editor1-first=Haraldur |editor2-last=Houghton |editor2-first=Bruce |editor3-last=McNutt |editor3-first=Steve |editor4-last=Rymer |editor4-first=Hazel |editor5-last=Stix |editor5-first=John |title=The Encyclopedia of Volcanoes |date=2015 |publisher=Zimbelman |location=Amsterdam |isbn=978-0-12-385938-9 |pages=717–728 |edition=Second |chapter-url=https://www.sciencedirect.com/science/article/pii/B9780123859389000419 |chapter=Volcanism on Mars}}</ref>