Updates Venus Express News

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ESA:
Solar flares over, Venus Express restarts science investigations

16 March 2012

ESA’s Venus Express spacecraft has returned to routine operation after its startracker cameras were temporarily blinded last week by radiation from a pair of large solar flares.

Science observations by ESA’s Venus Express were temporarily suspended on 7 March after the two startrackers – used to help navigate and orient the spacecraft – were overwhelmed by excessive proton radiation.

The proton storm stemmed from the Coronal Mass Ejections (CMEs) emitted by the Sun, which were associated with a pair of massive solar flares that occurred early in the morning on 7 March.

Click on image to enlarge​
The active Sun Spot group AR1429 (top centre in this image) is a very active solar region that recently produced two major solar flares with coronal mass ejections. The first was an X1-class flare on 5 March 2012 04:13UTC, and the second, even more powerful, an X5-class flare, on 7 March 2012 at 00:28 UTC. Several spacecraft were affected by the resulting strong radiation, wave of solar plasma and energetic particles. For example, the star tracker cameras on board Venus Express were temporarily 'blinded' for several days due to the harsh plasma environment in the aftermath of the CME cloud shock wave.
 ​
Credits: ESA/ Michel Breitfellner, Miguel Pérez Ayúcar, Manuel Castillo - ESAC​


With the startrackers unable to function properly, mission controllers at ESOC, ESA’s European Space Operations Centre, Darmstadt, had to place the spacecraft into a special mode to ride out the storm.


Waiting out the storm

This month, Venus Express is going through ‘quadrature’: a period of about five weeks during which the Sun-spacecraft-Earth angle is between 75° and 95°. They occur twice every 19 months.

During quadrature, the spacecraft must maintain a special orientation so that certain instruments are not over-exposed to sunlight and the radio antenna can still be pointed to Earth.


“At any time, if a problem is autonomously detected onboard, the spacecraft might place itself into ‘safe mode’,” says Octavio.

However, if a safe mode were to happen during quadrature operations, and the startrackers were not operating, it would be much more difficult to return the spacecraft to normal operations.

“To be very cautious, we simply stopped science activities to wait out the proton storm,” says Octavio.


The mission operations team used the gyroscopes to maintain a safe attitude while waiting for the startrackers to return to normal.

{...}
 

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ESA:
A curious cold layer in the atmosphere of Venus

1 October 2012

Venus Express has spied a surprisingly cold region high in the planet’s atmosphere that may be frigid enough for carbon dioxide to freeze out as ice or snow.

The planet Venus is well known for its thick, carbon dioxide atmosphere and oven-hot surface, and as a result is often portrayed as Earth’s inhospitable evil twin.

But in a new analysis based on five years of observations using ESA’s Venus Express, scientists have uncovered a very chilly layer at temperatures of around –175ºC in the atmosphere 125 km above the planet’s surface.

Click on image to enlarge​
This image of the Venus southern hemisphere illustrates the terminator – the transitional region between the dayside (left) and nightside of the planet (right). The south pole is near the terminator, just above the centre of the image. The complex atmosphere that surrounds the planet is also clearly visible. The image was taken at ultraviolet wavelengths by the Venus Monitoring Camera (VMC) on ESA’s Venus Express spacecraft on 15 May 2006, when the spacecraft was flying at about 66 500 km distance from the planet.
Credits: ESA/MPS, Katlenburg-Lindau, Germany​


The curious cold layer is far frostier than any part of Earth’s atmosphere, for example, despite Venus being much closer to the Sun.

The discovery was made by watching as light from the Sun filtered through the atmosphere to reveal the concentration of carbon dioxide gas molecules at various altitudes along the terminator – the dividing line between the day and night sides of the planet.

Armed with information about the concentration of carbon dioxide and combined with data on atmospheric pressure at each height, scientists could then calculate the corresponding temperatures.

“Since the temperature at some heights dips below the freezing temperature of carbon dioxide, we suspect that carbon dioxide ice might form there,” says Arnaud Mahieux of the Belgian Institute for Space Aeronomy and lead author of the paper reporting the results in the Journal of Geophysical Research.

Clouds of small carbon dioxide ice or snow particles should be very reflective, perhaps leading to brighter than normal sunlight layers in the atmosphere.

“However, although Venus Express indeed occasionally observes very bright regions in the Venusian atmosphere that could be explained by ice, they could also be caused by other atmospheric disturbances, so we need to be cautious,” says Dr Mahieux.

Click on image to enlarge​
The temperature profile along the terminator for altitudes of 70–160 km above the surface of Venus. The values were derived from the volume density of carbon dioxide molecules measured during solar occultation experiments by Venus Express’ SOIR instrument. The graphic provides the average range of values calculated from 59 measurements taken along the terminator from 88ºN to 77ºS, during different orbits between 2006 and 2011. The new report finds a prominent cold layer at 125 km sandwiched between two comparatively warmer layers at around 100 km and 140 km. At some locations, the temperatures occasionally dip below the freezing temperature of carbon dioxide, which suggests that carbon dioxide ice or snow could exist at these altitudes.
Credits: ESA/AOES–A.V. Bernus​


The study also found that the cold layer at the terminator is sandwiched between two comparatively warmer layers.

“The temperature profiles on the hot dayside and cool night side at altitudes above 120 km are extremely different, so at the terminator we are in a regime of transition with effects coming from both sides.

“The night side may be playing a greater role at one given altitude and the dayside might be playing a larger role at other altitudes.”

Similar temperature profiles along the terminator have been derived from other Venus Express datasets, including measurements taken during the transit of Venus earlier this year.

Models are able to predict the observed profiles, but further confirmation will be provided by examining the role played by other atmospheric species, such as carbon monoxide, nitrogen and oxygen, which are more dominant than carbon dioxide at high altitudes.

“The finding is very new and we still need to think about and understand what the implications will be,” says Håkan Svedhem, ESA’s Venus Express project scientist.

“But it is special, as we do not see a similar temperature profile along the terminator in the atmospheres of Earth or Mars, which have different chemical compositions and temperature conditions.”

{...}



Universe Today: Surprise! Hot Venus has a Cold Upper Atmosphere

SPACE.com: Strange Layer of Venus Surprisingly Cold

SpaceRef: Cold Layer in the Atmosphere of Venus
 

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ESA: Chasing clouds on Venus

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False-colour image of cloud features seen on Venus by the Venus Monitoring Camera (VMC) on Venus Express. The image was captured from a distance of 30 000 km on 8 December 2011. The VMC was designed and built by a consortium of German institutes lead by the Max-Planck Institute for Solar System Research in Katlenburg-Lindau. Venus Express has been in orbit around the planet since 2006.
Credits: ESA/MPS/DLR/IDA​

SpaceRef: Chasing clouds on Venus
 

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ESA: Have Venusian volcanoes been caught in the act?

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The rise and fall of sulphur dioxide in the upper atmosphere of Venus over the last 40 years, expressed in units of parts per billion by volume (ppbv). The dataset on the left is mostly from NASA’s Pioneer Venus, which was in orbit around Venus from 1978 to 1992. The dataset on the right is from ESA’s Venus Express, which has been studying Venus since 2006. A clear rise in the concentration of sulphur dioxide (SO2) concentration was observed at the start of the mission, with a subsequent decrease. The increase in sulphur dioxide can be interpreted either as evidence for volcanic activity or for decadal-scale variations in the circulation of Venus’ vast atmosphere.​
The data are superimposed on an artist impression of Venus, depicting a volcanic terrain surrounded by a thick, noxious atmosphere.​
Credits: Data: E. Marcq et al. (Venus Express); L. Esposito et al. (earlier data); background image: ESA/AOES​

Universe Today: Are Venus’ Volcanoes Still Active?

Science Daily: Have Venusian Volcanoes Been Caught in the Act?

EurekAlert: Have Venusian volcanoes been caught in the act?

SpaceRef: Have Venusian Volcanoes Been Caught in the Act?

Space Daily: A new episode of active volcanism on Venus?
 

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The Planetary Society: "Venus Express science mission ends; aerobraking experiment beginning"
Venus Express, currently the only spacecraft orbiting our nearest planetary neighbor, will soon meet a fiery end in Venus' atmosphere. According to a press release from the European Space Agency today, its science mission has ended. But its work isn't over yet. Just as NASA did with the Magellan Venus orbiter, ESA will maneuver Venus Express to dip into the uppermost Venus atmosphere and study how the spacecraft responds to atmospheric pressure. The work will give ESA valuable experience in aerobraking, in which the atmosphere of a planet like Venus or Mars is used to slow and shrink the orbit of a spacecraft -- saving fuel weight and making smaller, circular orbits possible.

Soon after -- or perhaps even during -- the aerobraking experiment, Venus Express will burn up in Venus' atmosphere, bringing the highly productive mission to an end.

[...]


ESA: "Venus Express gets ready to take the plunge"
 

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Whether contact is reestablished with the spacecraft or not, the mission has been very successful. It's just sad that humanity will have no outpost at Venus and no planned replacement, although there's still hope for Akatsuki. NASA's next Discovery mission might target Venus but there is strong competition from other destinations.
 

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Darn, I was hoping that next year we would add Pluto and Ceres to ALL of the planets being probed are having a probe enroute out to Saturn.
 

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This place gets better and better as we explore it. Now you can be cooked inside an acid storm OR be turned into a frozen statue before some wind gust spreads you in the form of little ice cubes. :lol:

Venus might soon be renamed "The place that human beings should avoid at all costs". Godess of Love... :hmm:
 

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This place gets better and better as we explore it. Now you can be cooked inside an acid storm OR be turned into a frozen statue before some wind gust spreads you in the form of little ice cubes. :lol:

Venus might soon be renamed "The place that human beings should avoid at all costs". Godess of Love... :hmm:

I've read that, in the middle of these extremes, there is a layer of clouds in which the environment is, in fact, the most habitable of the entire solar system for the human beings, with a temperature and a pressure strictly comparable to those of the Earth.
 

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I've read that, in the middle of these extremes, there is a layer of clouds in which the environment is, in fact, the most habitable of the entire solar system for the human beings, with a temperature and a pressure strictly comparable to those of the Earth.

Yes. Here it is: [ame="http://www.orbithangar.com/searchid.php?ID=3488"]Shukra_Venus_Station_080813[/ame]
 

jedidia

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A giant vortex at the south pole of Venus is actually a shape-shifter that changes form at least once a day, at times bizarrely taking on the appearance of a giant letter "S" or the number "8," a new study reveals.

Darn. Now we need animated textures in orbiter! :lol:

EDIT: Whoops, looks I'm over a year late.
 

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Title Cloudy Venus
Released 09/04/2018 9:00 am
Copyright ESA, NASA, J. Peralta & R. Hueso
Description
Our sister planet Venus is a dynamic and unusual place. Strong winds swirl around the planet, dragging thick layers of cloud with them as they go. These fierce winds move so speedily that they display ‘super-rotation’: Earth’s can move at up to a fifth of our planet’s rotation speed, but winds on Venus can travel up to 60 times faster than the planet.
Observations from ESA’s Venus Express, which orbited Venus from 2006 to 2014, and other international spacecraft have probed deeper into this wind and cloud in past years, and uncovered some peculiar behaviour.

http://www.esa.int/spaceinimages/Images/2018/04/Cloudy_Venus
 

Andy44

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60 times faster than the planet is not so impressive when you consider how slow the planet rotates. Equatorial rotation velocity, according to Wikipedia, is about six and a half km/h.
 

MaverickSawyer

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That's still 390 km/h, which is some pretty stiff winds if I do say so myself. :lol:
 
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