More than three decades have passed since the publication of the last review of the Venus
clouds and hazes. The paper published in 1983 in the Venus book summarized the …

Venus is the planet in the Solar System most similar to Earth in terms of size and (probably)
bulk composition. Until the mid-20th century, scientists thought that Venus was a verdant …

Venus is known to have been volcanically resurfaced in the last third of solar system history
and to have undergone a significant decrease in volcanic activity a few hundred million …

The NOMAD spectrometer suite on the ExoMars Trace Gas Orbiter will map the composition
and distribution of Mars׳ atmospheric trace species in unprecedented detail, fulfilling many …

The Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) on board the ESA/Venus
Express mission has technical specifications well suited for many science objectives of …

Simultaneous observations of Venus by Visible and Infrared Thermal Imaging Spectrometer
and Venus Monitoring Camera onboard the Venus Express spacecraft are used to map the …

One of the grand challenges in heliophysics is the characterization of coronal mass ejection
(CME) magnetic structure and evolution from eruption at the Sun through heliospheric …

No two rocky bodies offer a better laboratory for exploring the conditions controlling interior
dynamics than Venus and Earth. Their similarities in size, density, distance from the sun, and …

We present zonal and meridional wind measurements at three altitude levels within the
cloud layers of Venus from cloud tracking using images taken with the VIRTIS instrument on …

AKATSUKI is the Japanese Venus Climate Orbiter that was designed to investigate the
climate system of Venus. The orbiter was launched on May 21, 2010, and it reached Venus …