Friday, 22 August 2025

Asteroid 6 Hebe approaches opposition.

Asteroid 6 Hebe will reach opposition (the point at which it is directly opposite the Sun when observed from the Earth) at 4.46 pm GMT on Monday 25 August 2025, when it will also be at the closest point on its orbit to the Earth, 1.03 AU (i.e. 1.03 times as far from the Earth as the Sun, or about 153 787 000 km), and be completely illuminated by the Sun. While it is not obvious to the naked eye observer, asteroids have phases just like those of the Moon; being further from the Sun than the Earth, 6 Hebe is 'full' when directly opposite the Sun. As 6 Hebe is only about 205 km in diameter, it will not be visible to the naked eye, but with a maximum Apparent Magnitude (luminosity) of 7.6 at opposition, it should be visible in the Constellation of Aquarius to viewers equipped with a good pair of binoculars or small telescope. Because 6 Hebe is directly opposite the Sun in the sky, it will be best observed at around midnight local time from anywhere on Earth.

The orbits of 6 Hebe and the planets of the Inner Solar System, and their positions at 5.00 pm on Monday 25 August 2025. JPL Small Body Database.

Asteroid 6 Hebe was discovered on 1 July 1847 by Prussian amateur astronomer Karl Ludwig Hencke in the town of Driesen (now Drezdenko in Poland). As implied by the '6' in its modern designation, it was the sixth asteroid ever detected. It was given the name Hebe, in reference to the Greek goddess of youth by Carl Friedrich Gauss, director of the Göttingen Observatory

6 Hebe has a 1380 day (3.78 year) orbital period and an eccentric orbit tilted at an angle of 1.94° to the plane of the Solar System, which takes it from 1.94 AU from the Sun (i.e. 194% of the average distance at which the Earth orbits the Sun) to 2.92 AU from the Sun (i.e. 292% of the average distance at which the Earth orbits the Sun). As an asteroid that never comes within 1.666 AU of the Sun and has an average orbital distance less than 3.2 AU from the Sun, 4 Vesta is classed as a Main Belt Asteroid. 

6 Hebe is unusually dense for a large asteroid (denser than the Moon), containing about 0.5% of the mass of the Main Asteroid Belt, despite measuring only 205 km by 185 km by 170 km. This suggests that it is a solid object, unlike many large asteroids which are loosely connected 'rubble piles'. 

6 Hebe lies close to the '3:1 Kirkwood Gap' in the Main Asteroid Belt, an area where any asteroids present would have a 3:1 resonance with Jupiter (i.e. complete three orbits for every one orbit of Jupiter). This is an unstable area, devoid of asteroids, as any body in this area would likely be flung out by the tidal influence of Jupiter. Because of this, and its spectral profile (i.e. the specific wavelengths of light it reflects, which directly relates to its mineralogy, 6 Hebe is thought to be a likely parent body for H chondrites and IIE iron meteorites, two of the most common meteorite types on Earth, as well as the Near Earth Asteroids (4953) 1990 MU and 2007 LE. Furthermore, 6 Hebe appears to have an orbital and spectral relationship with a group of other Main Belt Asteroids, including bodies such as 695 Bella, 1166 Sakuntala, and 1607 Mavis which lie on the other side of the Kirkwood Gap, which have been tentatively identified as the 'Hebe Family' of asteroids, with a presumed common origin, either in a collision between two large bodies, or possibly from a single large body close to the Kirkwood Gap which was pulled apart by Jupiter's tidal influence.

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Fifteen confirmed deaths following landslide in the Republic of Guinea.

Fifteen people have now been confirmed dead following a landslide which hit the Manéah area of the town of Coyah, in the Kindea Region of the Republic of Guinea, about 50 km to the east of the capital, Conakry, at about 7.00 pm local time on Wednesday 20 August 2025. A further ten people are being treated in hospitals for serious injuries, and the number of deaths is expected to rise.The incident happened following heavy rains associated with the West African rainy season. Landslides are a common problem after severe weather, as excess pore water pressure can overcome cohesion in soil and sediments, allowing them to flow like liquids. Approximately 90% of all landslides are caused by heavy rainfall.

Rescue operations in Manéah following a landslide on Wednesday 20 August 2025. Journal Horoya/AP.

West Africa has a distinct two season climatic cycle, with a cool dry season during the northern winter when prevalent winds blow from the Sahara to the northeast, and a warm rainy season during the northern summer when prevalent winds blow from the Atlantic Ocean to the southwest. These warm winds from the Atlantic are laden with moisture, which can be lost rapidly when the air encounters cooler conditions, such as when it is pushed up to higher altitudes by the mountains of the Fouta Djallon in Guinea.

Rainfall and prevalent winds during the West African dry and rainy seasons. Encyclopedia Britanica.

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Thursday, 21 August 2025

Two deaths following Magnitude 5.8 Earthquake beneath Central Sulawesi, Indonesia.

The United States Geological Survey recorded a Magnitude 5.8 Earthquake at a depth of 12 km, approximately 12 km to the northwest of the town of Poso in Central Sulawesi Province, Indonesia, slightly before 6.40 am local time on Sunday 17 August 2025 (slightly before 10.40 pm on Sunday 16 August, GMT). Twenty nine people are known to have been injured during this event, two of whom subsequently died, one later on the day of the event, and one on Tuesday 19 August. The initial quake was followed by a series of aftershocks.

The approximate location of the 17 August 2025  Central Sulawesi Province Earthquake. USGS.

The tectonic situation beneath Sulawesi is complex, as it is caught in the collisional zone between the Eurasian, Pacific and Australian Plates. The north of the island is located on a breakaway section of the Eurasian Plate, called the Sangihe Plate. To the east lies the remnant Molucca Sea Plate, which is being subducted beneath both the Sangihe Plate and the more easterly Halmahera Plate, leading to Earthquakes and volcanism on Sulawesi and the islands of the Sangihe Arc in the west and the islands of the Halmahera Arc in the east.

The subduction zones beneath Sulawesi and the surrounding islands. Hall & Spakman (2015).

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Monday, 18 August 2025

Fireball over Arkansas and Missouri.

Witnesses across Arkansas, Iowa, Illinois, Indiana, Kentucky, Louisiana, Mississippi, Missouri, Oklahoman Tennessee, and Texas have reported observing a bright fireball meteor slightly after 1.30 am local time (slightly after 6.30 am GMT) on Sunday 17 August 2025. The fireball is described as having moved from southeast to northwest, appearing to the northwest of Walnut Ridge and disappearing close to Reeds Spring. A fireball is defined as a meteor (shooting star) brighter than the planet Venus. These are typically caused by pieces of rock burning up in the atmosphere, but can be the result of man-made space-junk burning up on re-entry.

The 17 August 2025 fireball meteor seen from Waxahachie, Texas. Garrett Griffen/American Meteor Society

Objects of this size probably enter the Earth's atmosphere several times a year, though unless they do so over populated areas they are unlikely to be noticed. They are officially described as fireballs if they produce a light brighter than the planet Venus. The brightness of a meteor is caused by friction with the Earth's atmosphere, which is typically far greater than that caused by simple falling, due to the initial trajectory of the object. Such objects typically eventually explode in an airburst called by the friction, causing them to vanish as a luminous object. However, this is not the end of the story as such explosions result in the production of a number of smaller objects, which fall to the ground under the influence of gravity (which does not cause the luminescence associated with friction-induced heating).

Heat map showing areas where sightings of the meteor were reported (warmer colours indicate more sightings), and the apparent path of the object (blue arrow). American Meteor Society.

These 'dark objects' do not continue along the path of the original bolide, but neither do they fall directly to the ground, but rather follow a course determined by the atmospheric currents (winds) through which the objects pass. Scientists are able to calculate potential trajectories for hypothetical dark objects derived from meteors using data from weather monitoring services.

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Friday, 15 August 2025

Determining the contents of bronze jars from an Ancient Greek shrine in southern Italy.

In 1954 archaeologists excavated a shrine to an unknown deity at the Greek settlement of Paestum in southern Italy, which was dated to the sixth century BC. Within this shrine they found six bronze hydriai (storage jars) and two amphorae, arranged around a large iron bed. The jars contained a pasty residue with a wax-like aroma. Traces of this substance were also found on the outside of the jars, which were originally sealed with cork, leading the archaeologists to conclude that it was originally a liquid, although possibly a fairly viscous one. It was interpreted that the bed was intended to be the residing place of the unknown deity, with the contents of the hydriai and amphorae were intended as offerings. 

Honey, in the Greek and Roman worlds, was a substance of some significance. As the only practical way to sweeten food and drinks, it was economically important, but it also had spiritual significance, being associated with wisdom and immortality, and therefore a suitable offering to the gods. With this in mind, it seemed highly likely that the original contents of the Paestum hydriai was honey.

With this in mind, the Bee Research Association in London arranged for an analysis of the residue to be carried out. The substance was found to be insoluble in water, but soluble in organic solvents, and to contain trace amounts of Plant and Insect remains, Fungi, and pollen, which led the scientists carrying out the analysis to conclude that it was probably a remnant of the wax which had originally sealed the jars.

In 1970 scientist at the Istituto Centrale del Restauro in Rome carried out an analysis on residues found around the neck and in the bottom of one of the amphorae from Paestum. This was found to comprise a saponifiable substance (substance which will react with an alkali to form a soap), such as a wax, fat, or resin, but contain no detectable sugar or protein (the major components of honey).

The residue was tested again in 1983 by the Laboratory of the Rome Chamber of Commerce, who again found that it was a saponifiable substance insoluble in water but soluble in organic solvents, and did not contain any sugary or starchy substances. On this occasion gas chromatography was also used to analyse the residue, concluding that it was 77.4% palmitic acid, 6.1% oleic acid, 5.2% stearic acid, 1.0% heptadecanoic acid, 1.0% linoleic acid + arachidic acid, 0.4% linoleic acid, and 6.5% unidentified substance. Since triglycerides of palmitic acid are extremely common in nature, the researchers concluded that the container had held animal fat or a vegetable oil.

In 2019, the residue from the Paestum hydriai was loaned to the Ashmolean Museum in Oxford, for an exhibition, 'Last Supper in Pompeii', and permission was obtained to carry out a new analysis of the biomolecular composition of the substance, using modern equipment not available when the previous tests were carried out.

In a paper published in the Journal of the American Chemical Society on 30 July 2025, Luciana da Costa Carvalho and Elisabete Pires of the Mass Spectrometry Research Facility at the University of Oxford, Kelly Domoney of the Ashmolean Museum, Gabriel Zuchtriegel of the Parco Archeologico di Pompei, and James McCullagh, also of the Mass Spectrometry Research Facility at the University of Oxford, present the results of this new analysis, and confidently identify the original material within the Paestum hydriai.

(A) Underground shrine in Paestum. (B) One of the hydriai on display alongside a Perspex box containing the residue at the Ashmolean Museum in 2019. (C) Graphic representation of the arrangement of the bronze jars inside the shrine. (D) Sample from the core of the residue.  Carvalho et al. (2025).

The residue arrived at the Ashmolean Museum in a non-hermetically sealed Perspex box, in which it had apparently been displayed at the Paestum Museum. In order to reduce the chances of modern contamination affecting their results, Carvalho et al. took samples from 40 mm below the surface for analysis, as well as from each distinct colour zones observed on the exterior of the material; black, orange, and green, colours which suggest some sort of interaction with the bronze vessel itself over the past 2500 years. Carvalho et al. also obtained modern beeswax, honey, and honeycombs from locations in Italy and Greece in order to compare these to the residue sample.

Carvalho et al. first used Fourier Transform Infrared Spectroscopy to obtain an overview of the chemical substances present within the sample. This yielded a spectrum almost identical to that of modern beeswax for the interior sample, strongly supporting the idea that this was the original substance. They also compared the spectra of new and artificially aged honeycombs from both Greece and Italy, establishing that there was little difference in these, and that these structures appear to be chemically stable at least 

Fourier Transform Infrared Spectrum  of the core sample of the archaeological residue superimposed on beeswax (a) and honey’s (b). Carvalho et al. (2025).

Next, Carvalho et al. carried out a Gas Chromatography coupled to Quadrupole Time-Of-Flight Mass Spectrometry analysis of the sample, along with samples of honey, beeswax, and fresh and artificially aged honeycomb. This produced almost no results for the beeswax, suggesting that the bulk components of this material were broken down by the high temperature at which this method operates (over 300°C), but did produce results from the sample, as well as from the honey and honeycomb controls, suggesting that the sample was never pure beeswax.

Electron ionisation chromatograms from the Quadrupole Time-Of-Flight Mass Spectrometry analysis of beeswax (a), the residue core sample (b), honey (c), and honeycomb from Greece, fresh (d) and aged (e). Compounds identified: (1) Hexadecanoic acid, (2) Heneicosane, (3) Octadecanoic acid, (4) Pentacosane, (5) Heptacosane, (6) Nonacosane, and (7) Hentriacontane. Carvalho et al. (2025).

Anion exchange Ion-Chromatography coupled to Mass Spectrometry identified seven hexose sugars, hexadecanoic acid, heneicosane, octadecanoic acid, pentacosane, heptacosane, nonacosane, and hentriacontane within the sample at levels higher than would be expected in beeswax, but lower than would be expected in honey. It also found significant levels of the sulphur amino acid taurine, which was not present in any of the control samples.

These hexose sugars were also recovered from aqueous extracts of honeycomb (i.e. the liquid obtained by soaking honeycomb in water)along with gluconolactone (a derivative of glucose) and galacturonic acid, and low levels of succinic, malic, and citric acids. All of these compounds were yielded at higher levels by the fresh honeycombs than by the artificially aged honeycombs.

Finally Carvalho et al. used a proteomic approach to try to identify specific proteins within the sample, as well as the beeswax and honeycomb controls, which were compared to the UniProt All Proteins database. The reesidue sample produced matches for three proteins derived from the royal jelly produced by the Western Honeybee, Apis mellifera, several Bacteria-derived proteins, and a number of common contaminant proteins, including keratins, caseins, lysyl endopeptidase, and trypsin. Encouraged by this, they then compared the sample to the Bee-specific UniProt Honey database, a search which yielded eight matches, including some associated with the Eastern Honeybee, Apis cerana cerana,

Proteins were also recovered from the modern honeycomb samples, but not the beeswax, indicating that they were derived from the honey portion of the comb. Notably, the royal jelly protein signature from the Greek and Italian honeycombs was quite different, although this was not completely unexpected as the two looked different. Carvalho et al. note that factors such as climate and the floral sources from which nectar is obtained can affect protein expression in Bee products, so this difference does not necessarily mean the Bees were particularly different.

Finally, a sample of the surface residue showing orange, black, and green colouration was subjected to X-ray photoelectron spectroscopy. This determined that the green areas of this residue were composed of 74.98% carbon, 20.78% oxygen, and 4.24% copper, with the copper portion largely dominated by Cu²⁺ ions, while the black areas were composed of 77.96% carbon, 20.12% oxygen, and 1.92% copper, with the copper dominated by Cu⁺ ions, and the orange areas were comprised of 86.50% carbon and 13.50% oxygen. The discoloration in these areas is, therefore, presumed to be derived by interactions between the original substance and the copper portion of the bronze vessel.

Honey is comprised primarily of sugars (typically 79% of the total mass, including 39% fructose), along with water (typically 18% of total mass), acids (0.17-1.17% of total mass) and trace amounts of other substances, such as vitamins, enzymes, flavonoids, and phenolic compounds. Over time this mixture undergoes Maillard reactions ('browning') as the amino acids of the proteins react with the sugars. This will occur more rapidly if the honey is stored at a warmer temperature. Eventually, the honey will take on a dark hue, as the sugars break down into furans and the acid content rises.

Previous studies of the Paestum hydriai residues concluded that this was a wax, most likely used to seal the vessels. The most commonly use wax in the ancient world was beeswax, a substance with quite different properties to honey. Beeswax is typically comprised of about 64% esters, 14% odd medium chain alkanes, 12% free acids, 2% acid polyesters, 1% acid monoesters, 1% free alcohols, and 6% other materials. Beeswax is much more stable than honey, but over time the acid and alcohol contents will increase as the was esters hydrolyse and the shorter chain alkanes are eliminated. 

The Fourier Transform Infrared Spectrum obtained by Carvalho et al. yielded results very similar to beeswax, suggesting that this may have formed a significant portion of the material from which the residue was derived. However, the Gas Chromatography coupled to Quadrupole Time-Of-Flight Mass Spectrometry analysis carried out suggested that the substance could not be pure beeswax. A study of the proteins present within the sample found several associated with honey production in the Western Honeybee, Apis mellifera, with a subsequent search of the Bee-specific UniProt Honey database yielded proteins associated with the Eastern Honeybee, Apis cerana cerana. Also produced were proteins associated with the wood-decay Fungus Armillaria gallica, and the parasitic Mite Tropilaelaps mercedesae, which targets Honeybees.

Eastern and Western Honeybees are closely related, and even where divergence has occurred, their proteins tend to be very similar. Furthermore, there is ample evidence for the cultivation of the Western Honeybee in ancient Italy, but none for the Eastern Honeybee. For these reasons, Carvalho et al. conclude that the readings suggesting the Eastern Honeybee as a source of proteins are probably erroneous, caused by the software trying to 'best fit' ancient degraded proteins.

The presence of proteins associated with the Mite Tropilaelaps mercedesae is also interesting. This Mite originated in Asia, and has a long historic connection with the Eastern Honeybee, but is generally thought only to have begun to infect Western Honeybees in the past few centuries. Carvalho et al. observe that it would be tempting to interpret this as evidence that the material at Paestum originated in Central Asia, but that a more likely scenario is that the proteins in question are common to a range of Acarid Mites.

Carvalho et al, conclude that a bulk composition similar to beeswax combined with the presence of proteins and other molecules found in honey make it likely that the material within the Paestum hydriai was almost certainly a honeycomb. This matches well with ancient literature, which frequently cites honey and other Bee-products as being suitable offerings for the gods, but contradicts earlier studies which were unable to obtain this result. Carvalho et al. emphasise that this underlines the importance of revisiting samples which have previously been analysed with less modern techniques, thus allowing our imptoving technology to improve our understanding of the past.

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