ESA Venus Express: ESOC have lost contact with Spacecraft

Artist's impression of Venus Express 

Credit: ESA (Image by AOES Medialab)

On 28 November 2014, the flight control team at ESOC reported loss of contact with Venus Express (VEX).

It is possible that the remaining fuel on board VEX was exhausted during the recent periapsis-raising manoeuvres and that the spacecraft is no longer in a stable attitude (the spacecraft’s high-gain antenna must be kept pointed toward Earth to ensure reliable radio contact).

Repeated attempts to re-establish contact using ESA and NASA deep-space tracking stations have been made since then, and there has been some limited success in the period since 3 December.

Although a stable telemetry link is not available, some telemetry packets were successfully downlinked.

These confirm that the spacecraft is oriented with its solar arrays pointing toward the Sun, and is rotating slowly.

The operations team is currently attempting to downlink the table of critical events that is stored in protected memory on board, which may give details of the sequence of events which occurred over the past few days.

The root cause of the anomaly (fuel situation or otherwise) remains to be established.

ESA will provide an update as soon as something more concrete is known.

International Action Against Ozone Depleting Substances Claim Gains

Minimum concentration of ozone in the southern hemisphere for each year from 1979-2013 (there is no data from 1995). 

Each image is the day of the year with the lowest concentration of ozone. A graph of the lowest ozone amount for each year is shown.

Image Credit: NASA's Goddard Space Flight Center/M. Radcliff

Worldwide action to phase out ozone-depleting substances has resulted in remarkable success, according to a new assessment by 300 international scientists.

The stratospheric ozone layer, a fragile shield of gas that protects Earth from harmful ultraviolet light, is on track to recovery over the next few decades.

The Assessment for Decision-Makers, a summary of the Scientific Assessment of Ozone Depletion 2014, provides new information to affirm that the 1987 international agreement known as the Montreal Protocol on Substances that Deplete the Ozone Layer has successfully resulted in global international policies to reduced levels of ozone-depleting substances.

The report is conducted by the World Meteorological Organization (WMO), and the United Nations Environmental Program (UNEP), and co-sponsored by NASA, National Oceanic and Atmospheric Administration (NOAA), and the European Commission.

Science teams from these organizations and other countries have been monitoring the ozone layer on the ground, by balloon and with a variety of satellite instruments dating back to NASA's Nimbus 4 satellite, launched in 1970.

The most current ozone hole satellite data comes from the Ozone Monitoring and Profiler Suite (OMPS) instrument on the NASA-NOAA Suomi National Polar-orbiting Partnership satellite (Suomi NPP), and the Ozone Monitoring Instrument and Microwave Limb Sounder (OMIMLS) on NASA's Aura satellite.

"It is particularly gratifying to report that the ozone layer is on track for recovery to 1980 benchmark levels by mid-century," said Paul A. Newman, chief scientist for atmospheres at NASA's Goddard Space Flight Center in Greenbelt, Maryland, and a co-chair of the WMO/UNEP report.

"Many of these early signs of ozone improvements are due to decades of work and contributions by NASA and NOAA instruments and scientists."

Ozone depleting substances are also powerful greenhouse gases. The Montreal Protocol provided a double benefit: stopping ozone depletion, and slowing the growth of greenhouse gases.

“Substitutes for ozone depleting substances are ozone safe, but many are powerful greenhouse gases.

These substitutes could offset the climate gains achieved by the Montreal Protocol in the future," Newman said.

The Assessment for Decision-Makers, a summary of the Scientific Assessment of Ozone Depletion 2014 is the first comprehensive update in four years.

The full report will be available in early 2015.

NASA Voyager-1: On the edge of the Solar System

Artist's concept of NASA's Voyager spacecraft. 

Credit: NASA/JPL-Caltech 

Data from NASA's Voyager 1 spacecraft continues to provide new insight on the outskirts of our solar system, a frontier thought to be the last that Voyager will cross before becoming the first man-made object to reach interstellar space.

In papers published this week in the journal Science, scientists from the Johns Hopkins University Applied Physics Laboratory (APL) in Laurel, Md., and other Voyager partner institutions provide more clarity on the region they named the "magnetic highway" in December 2012.

Cruising through what scientists describe as a curious, unexpected charged-particle environment, Voyager has detected, for the first time, low-energy galactic cosmic rays, now that particles of the same energy from inside the bubble around our Sun disappeared.

As a result, Voyager now sees the highest level so far of particles from outside our solar bubble that originate from the death of other nearby stars.

"Voyager 1 may be months or years from leaving the solar system—we just don't know," says APL's Stamatios Krimigis, principal investigator for Voyager's Low-Energy Charged Particle (LECP) instrument.

"But the wait itself is incredibly exciting, since Voyager continues to defy predictions and change the way we think about this mysterious and wonderful gateway region to the galaxy."

This artist's concept shows NASA's Voyager 1 spacecraft exploring a region called the "depletion region" or "magnetic highway" at the outer limits of our heliosphere, the bubble the sun blows around itself. 

In this region, the magnetic field lines generated by our sun (yellow arcs) are piling up and intensifying and low-energy charged particles that are accelerated in the heliosphere's turbulent outer later (green dots) have disappeared. 

Scientists think the depletion region is the last region Voyager 1 has to cross before reaching interstellar space, which is the space between stars, Voyager 1 passed a shockwave known as the termination shock in 2004, where solar wind suddenly slowed down and became turbulent. 

In 2010, it then passed into an area called the "stagnation region" where the outward velocity of the solar wind slowed to zero and sporadically reversed direction. 

In the slow-down and stagnation regions, the prevalence of low-energy charged particles from our heliosphere jumped dramatically and is indicated by the green dots. 

On Aug. 25, 2012. Voyager 1 entered the depletion or magnetic highway region, where the magnetic field acts as a kind of "magnetic highway" allowing energetic ions from inside the heliosphere to escape out, and cosmic rays from interstellar space zoom in. 

Magnetic field lines form a spiral around the solar system because of the rotation of the sun, and at the edge of the heliosphere they form roughly parallel arcs. 

Because an interstellar wind outside is pushing back on the heliosphere, magnetic field lines pile up as the solar wind slows, like cars back up at a freeway off-ramp. 

The compression of field lines increases the strength of the magnetic field as Voyager approaches interstellar space. 

Since scientists don't know the exact location of the heliopause - which is the border to interstellar space - that area has been labeled with a question mark. 

Image credit: NASA/JPL-Caltech 

Voyager 1 and 2 were launched in 1977 and between them visited Jupiter, Saturn, Uranus and Neptune.

Since 1990, the twin spacecraft have been on their Interstellar Mission, on track to leave the heliosphere, which is the bubble of magnetic field and charged particles the Sun blows around itself.

On Aug. 25, 2012, when Voyager 1 was about 11 billion miles (18 billion kilometers) from the Sun, the spacecraft reached the so-called magnetic highway where charged particles from inside the heliosphere zoomed out along the magnetic field as cosmic rays from far outside zoomed in.

The lack of a detectable change in the direction of that magnetic field, however, convinced scientists that Voyager remained within the Sun's influence.

The new Science papers focus on observations from the summer and fall of 2012 by LECP as well as Voyager 1's Cosmic Ray and Magnetometer instruments, with additional LECP data through April 2013.

More information: References:

* "Magnetic Field Observations as Voyager 1 Entered the Heliosheath Depletion Region," L. F. Burlaga, N. F. Ness, and E. C. Stone, Science, DOI: 10.1126/science.1235451; www.sciencemag.org/content/early/2013/06/26/science.1235451.abstract 
* "Search for the Exit: Voyager 1 at Heliosphere's Border with the Galaxy," S. M. Krimigis, R. B. Decker, E. C. Roelof, M. E. Hill, T. P. Armstrong, G. Gloeckler, D. C. Hamilton, and L. J. Lanzerotti, Science, DOI:10.1126/science.1235721; www.sciencemag.org/content/early/2013/06/26/science.1235721.abstract 
* "Voyager 1 Observes Low-Energy Galactic Cosmic Rays in a Region Depleted of Heliospheric Ions," E. C. Stone, A. C. Cummings, F. B. McDonald, B. C. Heikkila, N. Lal, and W. R. Webber, Science, DOI:10.1126/science.1236408; www.sciencemag.org/content/early/2013/06/26/science.1236408.abstract