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Some observers may have access to cameras operating at wavelengths beyond 1.0 microns. The images have been edited for the purpose of fitting them in a single figure. On occasion, images taken with a green filter have proved useful in the study of intermediate clouds.Įxamples of observations in these wavelengths are given in the figure on the right composed from observations available in the PVOL databaseĪnd acquired by T. The contrast in RGB images of the Venus' clouds is extremely low. Interview of Martin Lewis with a different approach.Ĭloud contrast is strongest in UV, strong in Vio, very weak in blue, and weak (but with real feature) Surface observations of Venus written by Anthony Wesley and Phil Miles and on this

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Help on this excellent guide on how to obtain night-side Require a combination of filters to block light by the illuminated part of Venus.

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Peralta et al., Icarus, 288, 235-239 (2017)Īmateur observations in the following windows are desired:

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Overview of useful spectral regions for Venus: An update to encourage observations complementary to the Akatsuki mission. Observation windows of Venus are discussed in this publication:

Initial results from the August 2020 observations will be presented at the We expect that the large number of observations obtained byĭifferent teams around the BepiColombo flyby in combination with the ground-based amateur campaign will produce a unique Observations of Venus surface are also welcome. Provided by amateur astronomers was published recently and shows the value of amateur images in combination with

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ApJL, 2016).Īmateur observations of Venus in 2007 were also analyzed in the context of the MESSENGER flyby (Ī recent study combining observations obtained by the Akatsuki mission, professional telescopes and observations Will be able to cover Venus atmosphere and study its atmospheric superrotation as it was done prior to theĪkatsuki orbit insertion in 2015 ( Sanchez-Lavega et al. We expect that observations provided by a large group of collaborators from different locations on Earth Study the atmospheric activity visible in Venus clouds. Observations obtained also in smaller telescopes with similar techniques (fast cameras) have a high potential to Images on the right show Venus observed from the Pic du Midi 1.05m telescope by a group of amateur astronomers in 2017 and processedīy D.

The 3rd flyby of Venus by the Parker Solar Probe (NASA) on 11 July 2020. Observations around 11 July 2020 will be used to support the analysis of data acquired during We encourage amateur observers to observe Venus in mid-July, late August and mid-October 2020. To enhance the scientific return of the BepiColombo flyby in October 15, 2020. We are seeking context observations of Venus provided by amateur astronomers In addition, a large ground-based campaign to observe Venus has been organized not only during the flyby,īut also in August 2020, when Venus reaches its maximum elongation (45 deg), with an apparent size from Earth of 23-24 arcsec. The flybys will be a unique opportunity to study Venus from a multiple perspective.ĭuring the flybys BepiColombo will obtain observations of Venus in coordination with the JapaneseĪkatsuki mission (JAXA), currently in an equatorial orbit around the planet. Of Venus on 15 October 2020 (03:58 UT, the exact time may vary)Īnd 10 August 2021. (ESA/JAXA) will arrive to Mercury on December 2025 after an interplanetary trajectory in which it will perform two flybys The European-Japanese joint mission BepiColombo