Japanese engineers aim Akatsuki for a second attempt at orbiting Venus in 2015
Japanese engineers have re-adjusted the course of their science probe Akatsuki for a second attempt at orbiting Venus in 2015.
Japanese engineers have re-adjusted the course of their science probe Akatsuki for a second attempt at orbiting Venus in 2015.
The engine of Japan’s troubled Venus probe, Akatsuki, has been found too damaged to put the probe into Venus orbit.
JAXA conducted a test ignition of the probe’s main engine on Wednesday to prepare for another attempt to send it into orbit in 2015. But the thrust produced was only one-eighth the amount anticipated, the space agency said. The damage the engine suffered last December when JAXA ignited it in the initial attempt to send the probe into orbit around Venus appears to be more serious than thought, JAXA said.
Japan has successfully completed a two second test fire of the engine on its lost Venus probe Akatsuki.
Japan plans to test fire the engine of its failed Venus probe Akatsuki twice this month, in anticipation of another try at Venus orbit in 2015.
The strange fluctuating polar vortex over Venus’s south pole.
Ikaros takes a picture of Venus.
Japan may try to put Akatsuki into orbit around Venus five years from now, rather than six.
Engineers now think that a cracked nozzle caused the Japanese probe Akatsuki to miss Venus.
In a paper published today in Geophysical Research Letters, scientists think they have detected evidence of volcanic activity on Venus that took place sometime in the past two decades.
Venus has a Moon?
Sad news: It appears that Japan’s Venus probe failed to enter orbit, and might have flown past Venus.
Update: It is confirmed that the spacecraft flew past Venus. There is a chance Japan could try again, when Akatsuka returns to Venus — in about seven years.
The status of the Japanese probe Akatsuki in its attempt to go into orbit around Venus remains uncertain. The engines fired as scheduled, but radio signal was not regained at the scheduled time. Engineers are analyzing the spacecraft’s position now to see if it was successfully inserted into orbit.
Apropos of the desire of IPCC chief Rajendra Pachauri to re-engineer the climate to battle global warming, including spraying “sulphate particles high in the atmosphere to scatter the sunβs rays back into space,” planetary scientists have pinpointed the source of Venus’s sulphuric acid clouds, and from this believe that the IPCC scheme might backfire badly, doing more harm than good.
Scientists have detected Venusian lava flows possibly only decades old.
Steve Squyres of Cornell University and the project scientist of the Mars rovers Spirit and Opportunity spoke today at an astrobiology symposium in Arlington, Virginia. He described several spectacular planetary missions that might be flown in the coming decade. All are being considered. None have yet been chosen or funded.
Squyres is the co-chair of a committee of the National Science Foundation that is right now putting together a decadal survey for outlining unmanned planetary research for the next decade. This survey is expected to be released in March, which is when we will find out which of the above missions the planetary science community prefers.
By diving into the upper atmosphere of Venus above its north pole, Venus Express has found that the atmosphere there is 60% less dense than predicted. This from a press conference going on right now at the 42nd meeting of the AAS Division for Planetary Sciences. They plan an additional dive campaign during the next month. And they plan more dives, going deeper each time, as they judge the consequences to the spacecraft each time.
To read the abstracts of the Venus Express papers, go here.
Updated: The full press release, with images, can be seen here.
Using data accumulated over the past four years by Venus Express, scientists have shown that the giant double vortex storm at Venus’s south pole was only a temporary phenomenon. You can download the actual paper here [pdf]. Key quote from the paper:
The polar region of Venus shows a dynamics regime quite different than the rest of the planet, with a separation region delimited by the cold collar zone. Average wind speeds presents an almost solid body rotation, while instantaneous view highlights the complex dynamic structure with air flowing almost toward all directions. The so called dipole shape is not a stable feature and the morphology of the vortex is significantly variable on both short and long timescales.
The “cold collar” is an atmospheric ring of colder temperatures that encircles the planet’s poles.
Evidence continues to build that volcanic activity on Venus has occurred in the very recent past, and might even be going on today.