Repository logo
Log in(current)
Repository logoMIT Open ScholarshipDSpace@MIT
  1. Home
  2. MIT Open Access Articles
  3. MIT Open Access Articles
  4. Deducing the Composition of Venus Cloud Particles with the Autofluorescence Nephelometer (AFN)

Deducing the Composition of Venus Cloud Particles with the Autofluorescence Nephelometer (AFN)

Thumbnail Image
Download
Name

aerospace-09-00492-v2.pdf

Size

3.42 MB

Format

Adobe PDF

Checksum (MD5)

9bb5ab5695d8c50e0cddf79a1daafe4e

Download all files submitted through automated deposit
packager-6319ecf6.zip (3.15 MB)
Author(s)
Baumgardner, Darrel
•
Fisher, Ted
•
Newton, Roy
•
Roden, Chris
•
Zmarzly, Pat
•
Seager, Sara
•
Petkowski, Janusz J.
•
Carr, Christopher E.
•
Špaček, Jan
•
Benner, Steven A.
more
Date Issued
September 2, 2022
Publisher
Multidisciplinary Digital Publishing Institute
Citation
Aerospace 9 (9): 492 (2022)
Version
Final published version
Abstract
The composition, sizes and shapes of particles in the clouds of Venus have previously been studied with a variety of in situ and remote sensor measurements. A number of major questions remain unresolved, however, motivating the development of an exploratory mission that will drop a small probe, instrumented with a single-particle autofluorescence nephelometer (AFN), into Venus’s atmosphere. The AFN is specifically designed to address uncertainties associated with the asphericity and complex refractive indices of cloud particles. The AFN projects a collimated, focused, linearly polarized, 440 nm wavelength laser beam through a window of the capsule into the airstream and measures the polarized components of some of the light that is scattered by individual particles that pass through the laser beam. The AFN also measures fluorescence from those particles that contain material that fluoresce when excited at a wavelength of 440 nm and emit at 470–520 nm. Fluorescence is expected from some organic molecules if present in the particles. AFN measurements during probe passage through the Venus clouds are intended to provide constraints on particle number concentration, size, shape, and composition. Hypothesized organics, if present in Venus aerosols, may be detected by the AFN as a precursor to precise identification via future missions. The AFN has been chosen as the primary science instrument for the upcoming Rocket Lab mission to Venus, to search for organic molecules in the cloud particles and constrain the particle composition.
MIT Department
Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Department of Aeronautics and Astronautics
Terms of Use
Creative Commons Attribution
https://creativecommons.org/licenses/by/4.0/
Persistent DSpace Link
https://hdl.handle.net/1721.1/145315
DOI of Published Version
https://doi.org/10.3390/aerospace9090492
Repository logo
PrivacyPermissionsAccessibilityContact us
Repository logo
Notify us about copyright concerns.