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Akatsuki Venus Orbital Insertion


Frida Space

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8 minutes ago, Stone Blue said:

Over 2km/s velocity dropped...Still dropping...

Just to clarify, that's a simulation. If things haven't gone as planned, the velocity should be higher. But let's hope everything went well! We need a Venus orbiter so bad...

VOI C3 window closes in 540 seconds.

3 min to know the result of burn!!

Edited by Frida Space
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2 minutes ago, insert_name said:

so what experiments will it be doing

From SF101:

The instrument suite is comprised of two 12 x 12° infrared imaging instruments, the first covering the 0.90, 0.97 and 1.01-micrometer wavelengths while the second is sensitive at 1.73, 2.26 and 2.32 microns. These cameras will be able to complete imaging of the deepest levels of the dense Venusian atmosphere up to the middle and lower atmosphere at the longer wavelengths. For cloud top mapping, a 12.4 x 16.4° Longwave Infrared Camera at 10 microns will be employed while the Ultraviolet Imager will also look at the cloud tops and associated motion at wavelengths of 263 and 365 nanometers. A Lightning and Airglow Camera with a 16 by 16 ° field of view will be used to capture airglows and lightning on the night side of the planet at wavelengths of 551, 553, 558, 630, and 777 nanometers.

The spacecraft’s instruments will be employed to map the high and low-altitude cloud patterns, measure the distribution of water vapor and carbon monoxide, and image the surface of the planet in the search of active volcanoes using the infrared imagers of Akatsuki that can peer through the thick clouds of the planet to detect the surface. Sulfur dioxide, a precursor to cloud formation, will be mapped with the ultraviolet imaging system and radio waves sent from Earth will be directed through the atmosphere to study its structure by looking at changes introduced into the signals.

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