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1. Outgassing from the OSIRIS-REx sample return capsule: characterization and mitigation

2. Development and testing of a pyro-driven launcher for harpoon-based comet sample acquisition

3. On the origin & thermal stability of Arrokoth's and Pluto's ices

5. Laboratory spectra of CO2 vibrational modes in planetary ice analogs

6. XANES analysis of organic residues produced from the UV irradiation of astrophysical ice analogs

7. Carbon dioxide on the satellites of Saturn: Results from the Cassini VIMS investigation and revisions to the VIMS wavelength scale

8. Optical constants of amorphous and crystalline H2O-ice in the near infrared from 1.1 to 2.6 μm

9. Astrobiology explorer mission concepts (ABE/ASPIRE)

10. Near-infrared spectra of laboratory H2O–CH4 ice mixtures

11. A spectroscopic study of the surfaces of Saturn's large satellites: HO ice, tholins, and minor constituents

12. Laboratory IR spectra of 4-azachrysene in solid H2O

13. The infrared spectrum of matrix isolated aminoacetonitrile, a precursor to the amino acid glycine

14. An evolutionary connection between interstellar ices and IDPs? Clues from mass spectroscopy measurements of laboratory simulations

16. Ultraviolet irradiation of the polycyclic aromatic hydrocarbon (PAH) naphthalene in H2O. Implications for meteorites and biogenesis

17. Variations in the strength of the infrared forbidden 2328.2 cm−1 fundamental of solid N2 in binary mixtures

18. Infrared Spectroscopy of Triton and Pluto Ice Analogs: The Case for Saturated Hydrocarbons

19. New Narrow Infrared Absorption Features in the Spectrum of Io between 3600 and 3100 cm-1 (2.8-3.2 μm)

20. Is H2O Present on Io? The Detection of a New Strong Band Near 3590 cm-1 (2.79 μm)

21. An Experimental Study of the Organic Molecules Produced in Cometary and Interstellar Ice Analogs by Thermal Formaldehyde Reactions

22. Laboratory simulation of the photoprocessing and warm-up of cometary and pre-cometary ices: Production and analysis of complex organic molecules

23. Laboratory studies of the newly discovered infrared band at 4705.2 cm−1 (2.1253 μm) in the spectrum of Io: The tentative identification of CO2

24. The 2.5–5.0 μm spectra of Io: Evidence for H2S and H2O frozen in SO2

25. Infrared transmission spectra from 2.5 to 25 μm of various meteorite classes

26. The condensation and vaporization behavior of H2O: CO ices and implications for interstellar grains and cometary activity

27. Solar flare track densities in interplanetary dust particles: The determination of an asteroidal versus cometary source of the zodiacal dust cloud

28. A multicomponent model of the infrared emission from Comet Halley

29. Photochemical and thermal evolution of interstellar/precometary ice analogs

30. Interplanetary dust particles collected in the stratosphere: Observations of atmospheric heating and constraints on their interrelationship and sources

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