The Deep Composition of Uranus and Neptune from In Situ Exploration and Thermochemical Modeling
Space Science Reviews, ISSN: 1572-9672, Vol: 216, Issue: 4
2020
- 20Citations
- 29Captures
- 2Mentions
Metric Options: CountsSelecting the 1-year or 3-year option will change the metrics count to percentiles, illustrating how an article or review compares to other articles or reviews within the selected time period in the same journal. Selecting the 1-year option compares the metrics against other articles/reviews that were also published in the same calendar year. Selecting the 3-year option compares the metrics against other articles/reviews that were also published in the same calendar year plus the two years prior.
Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Most Recent Blog
How Uranus and Neptune are key to unlocking how planets form
A flagship mission to the ice giants — Uranus and Neptune — will forever change our understanding of the origin and evolution of our solar system.
Most Recent News
How Uranus and Neptune are key to unlocking how planets form – The Planetary Society
Learn how our members and community are changing the worlds. Our citizen-funded spacecraft successfully demonstrated solar sailing for CubeSats. Exploring the watery planets and moons
Review Description
The distant ice giants of the Solar System, Uranus and Neptune, have only been visited by one space mission, Voyager 2. The current knowledge on their composition remains very limited despite some recent advances. A better characterization of their composition is however essential to constrain their formation and evolution, as a significant fraction of their mass is made of heavy elements, contrary to the gas giants Jupiter and Saturn. An in situ probe like Galileo would provide us with invaluable direct ground-truth composition measurements. However, some of the condensibles will remain out of the grasp of a shallow probe. While additional constraints could be obtained from a complementary orbiter, thermochemistry and diffusion modeling can further help us to increase the science return of an in situ probe.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=85084644850&origin=inward; http://dx.doi.org/10.1007/s11214-020-00677-8; https://link.springer.com/10.1007/s11214-020-00677-8; https://link.springer.com/content/pdf/10.1007/s11214-020-00677-8.pdf; https://link.springer.com/article/10.1007/s11214-020-00677-8/fulltext.html; https://dx.doi.org/10.1007/s11214-020-00677-8; https://link.springer.com/article/10.1007/s11214-020-00677-8
Springer Science and Business Media LLC
Provide Feedback
Have ideas for a new metric? Would you like to see something else here?Let us know