Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

Seasonal Variability of Pluto’s Haze Formation Revealed by Laboratory Simulations

  • Authors: Zhengbo Yang, Chao He, Yu Liu, Sai Wang, Haixin Li, Yingjian Wang, Xiao'ou Luo, Sarah M. Hörst, Sarah E. Moran, Véronique Vuitton, Laurène Flandinet, Patricia McGuiggan

Zhengbo Yang et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 3.

(a) FTIR spectra of three tholins from 4000 to 500 cm−1, where the red, black, and blue lines represent the 0.1%, 0.6%, and 5% CH4 tholins, respectively. (b) Comparison of 5% CH4 tholin in this study with Titan tholins in previous work (90% N2/5% CH4/ 5% CO, Z. Yang et al. 2025). The corresponding functional groups are marked near their absorption features.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse