California’s grape growers have a tough row to hoe. The root-sucking
phylloxera parasite is threatening their vines, and the public has reportedly
gone off wine. To cap it all, a tiny sap-sucking insect called the sharpshooter
has returned to spread disease among the vines.
Sharpshooters are leaf-hoppers that suck nutrients from the water-transport
systems of plants. The worst of them is the blue-green sharpshooter, Graphocephala
atropunctata. They are voracious feeders, guzzling hundreds of times their
body weight in plant fluid each day. As they feed, they inadvertently inoculate
the plants with a bacterium that lives in their gut. The bacterium, Xylella
fastidiosa, multiplies in the plant’s water conduits and clogs them. The
leaves turn brown and the plant eventually dies from dehydration.
This condition, known as Pierce’s disease, wiped out thousands of hectares
of grapes in southern California earlier this century and prevents wine
growers from moving into the southeast of the US. The Napa valley north
of San Francisco, California’s prime grape growing region, has always suffered
from small outbreaks of Pierce’s disease. But it is generally confined
to the edges of vineyards, next to rivers or areas of natural scrub or
woodland harbouring plants that are host to the sharpshooter.
For the past two years, however, the disease has been on the rise in
Napa county, and is cropping up in previously trouble-free areas. This may
be because recent wet springs, and the resulting lush vegetation, have produced
a population boom of sharpshooters. But it might also be an unforeseen consequence
of the epidemic of phylloxera that has swept through California. Terrified
of losing their livelihood to this root-sucking insect, growers are ripping
up their vines and planting new stocks that are resistant to it. Unfortunately,
young vines are particularly susceptible to Pierce’s disease.
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It is even possible that a new strain of Xylella fastidiosa may have
arisen, according to Alexander Purcell, an entomologist at the University
of California at Berkeley. Cold weather is probably critical in killing
off the bacterium each winter, says Purcell. ‘If you got a strain that would
survive the winter better you’d be in trouble.’
Such changes do happen. A similar disease, also caused by Xylella,
arose suddenly among citrus trees in Brazil, says Purcell. In 1987, farmers
noticed three trees with blotchy leaves; today more than a million are infected.
‘That was definitely a new strain,’ he says.
If a region is prone to Pierce’s disease, there is little to be done,
short of continuously replanting the infected parts of the vineyard or clearing
away nearby vegetation. All attempts to breed resistant varieties of wine
grape have failed so far.
For now, while phylloxera threatens all the Napa valley’s vineyards,
Pierce’s disease has hit only 5 per cent of the vines. Experts suggest
that the sharpshooter will never do as much damage as phylloxera, although
they cannot be certain. ‘The disease has been present in Napa county for
a very long time, and historically it has had these cycles of severity,’
says Ed Weber, a farm adviser with the University of California. ‘My sense
is that in a year or two we will see the incidence taper off once again.’



![Astronomers have long known that understanding how star clusters come to be is key to unlocking other secrets of galactic evolution. Stars form in clusters, created when clouds of gas collapse under gravity. As more and more stars are born in a collapsing cloud, strong stellar winds, harsh ultraviolet radiation and the supernova explosions of massive stars eventually disperse the cloud, and their light can bear down on other star-forming regions in the galaxy. This process is called stellar feedback, and it means that most of the gas in a galaxy never gets used for star formation. Researching how star clusters develop can answer questions about star formation at a galactic scale. Now, the state of the art has been further developed with both Hubble and Webb working together to provide a broad-spectrum view of thousands of young star clusters. An international team of astronomers has pored over images of four nearby galaxies from the FEAST observing programme (#1783), trying to solve this mystery. Their results show that it is the most massive star clusters that clear away their gaseous shroud the fastest, and begin lighting their galaxy the earliest. The team identified nearly 9000 star clusters in the four galaxies in different evolutionary stages: young clusters just starting to emerge from their natal clouds of gas, clusters that had partially dispersed the gas (both from Webb images), and fully unobstructed clusters visible in optical light (found in Hubble images). With Webb???s ability to peer inside the gas clouds, they were able to then estimate the mass and age of each cluster from its light spectrum. This image shows a section of one of the spiral arms of Messier 51 (M51), one of the four galaxies studied in this work, as seen by Webb???s Near-Infrared Camera (NIRCam). The thick clumps of star-forming gas are shown here in red and orange, representing infrared light emitted by ionised gas, dust grains, and complex molecules such as polycyclic aromatic hydrocarbons (PAHs). Within these gas complexes, each tens or hundreds of light years across, Webb reveals the dense, extremely bright clusters of massive stars that have just recently formed. The countless stars strewn across the arm of the galaxy, many of which would be invisible to our eyes behind layers of dust, are also laid bare in infrared light. [Image description: A large, long portion of one of the spiral arms in galaxy M51. Red-orange, clumpy filaments of gas and dust that stretch in a chain from left to right comprise the arm. Shining cyan bubbles light up parts of the gas clouds from within, and gaps expose bright star clusters in these bubbles as glowing white dots. The whole image is dotted with small stars. A faint blue glow around the arm colours the otherwise dark background.]](https://images.newscientist.com/wp-content/uploads/2026/05/13114322/SEI_296271016.jpg)