At least eighteen dead following Magnitude 7.0 Earthquake beneath Baqên County, Tibet.

The China Earthquake Networks Center recorded a Magnitude 7.0 Earthquake at a depth of 10 km beneath Baqên County in northeast Tibet, close to Mount Everest and the border with Tibet slightly before 10.35 pm local time (slightly before 2.35 pm GMT) on Thursday 22 October 2026. At least eighteen people have died as a result of this event, with seventy six people known to have been injured, eleven of them seriously. The Earthquake is known to have caused the collapse of at least 339 houses, however, the nature of the area, with an average altitude of 4800 m above sealevel, and many people living in scattered villages in steep-sided valleys, where temperatures regularly fall below 0°C at night, means that these figures may worsen. There have been a number of aftershocks in the region, leading local authorities to evacuate 12 000 people from their homes. 

Villagers in a temporary resettlement camp following a Magnitude 7.0 Earthquake in Baqên County, Tibet, on 22 October 2026. Tenzin Nyida/Xinhua.

Earthquake activity in the area is caused by the uplift of the Tibetan Plateau, due to the impact of India into Eurasia to the south. The Indian Plate is moving northwards at a rate of 5 cm per year, causing it to impact into Eurasia, which is also moving northward, but only at a rate of 2 cm per year. The collision of the Indian and Eurasian plates has led to the formation of the Himalayan Mountains, the Tibetan Plateau, and the mountains of southwest China, Central Asia and the Hindu Kush.

Block diagram showing how the impact of the Indian Plate into Eurasia is causing uplift on the Tibetan Plateau. Jayne Doucette/Woods Hole Oceanographic Institution.

Much of Tibet and neighbouring areas of Central Asia and the Himalayas, are prone to Earthquakes caused by the impact of the Indian Plate into Eurasia from the south. When two tectonic plates collide in this way and one or both are oceanic then one will be subducted beneath the other (if one of the plates is continental then the other will be subducted), but if both plates are continental then subduction will not fully occur, but instead the plates will crumple, leading to folding and uplift (and quite a lot of Earthquakes). 

The movement of India into Eurasia over the last 71 million years. United States Geological Survey.

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Norellraptor barsboldi: A new species of Microraptorine Dinosaur from the Early Cretaceous Jehol Biota of northeastern China.

The Microraptines are a small group of Paravian Dinosaurs (the group that includes Birds and their closest relatives, the Dromaeosaurs, Troodontids, and Scansoriopterygids), known mostly from the Early Cretaceous Jehol Biota of northeastern China. The remarkable preservation of the Jehol Biota fossils means that while the Microraptines were not apparently widespread or numerous, the specimens we do have are often exceptionally well preserved. Such fossils have produced Microraptines with feather-like integumentary structures, true pennaceous feathers and remnants of the gut contents, enabling a more detailed reconstruction of their ecology than has been possible for many more numerous Dinosaur groups.

Many Microraptines are interpreted as having been capable of flying, and the close relationship between Microraptines and Birds has made them an important group to palaeontologists studying the origin of flight. The closest sister group to the Microraptines is usually thought to be the Dromaeosaurs, a group of medium-sized Paravian Theropods clearly quite incapable of flight, which raises two possibilities. Either the ability to fly arose twice (or more than twice) within the Paravian clade, or the earliest members of the group had the ability, with groups such as the Dromaeosaurs losing this ability secondarily. 

In a paper published in the journal Nature Communications on 29 September 2026, Xuri Wang of the Key Laboratory of Stratigraphy and Paleontology of the Ministry of Natural Resources, and the Hebei GEO University, Yannan Ji of the Chinese Academy of Geological Sciences, Andrea Cau of the OPHIS Museo Paleontologico e Centro Erpetologico, Martin Kundrát of the Center for Integrative Paleobiology at Pavol Jozef Šafárik University, Yichuan Liu, also of the Key Laboratory of Stratigraphy and Paleontology of the Ministry of Natural Resources, and of the China University of Geosciences, Yang Wang, again of the Key Laboratory of Stratigraphy and Paleontology of the Ministry of Natural Resources, and Qiang Ji, also of the Hebei GEO University describe a new species of Microraptorine Dinosaur from the Early Cretaceous Jehol Biota of northeastern China.

The new species is named Norellraptor barsboldi, where 'Norellraptor' means 'Norell's Raptor' in honour of American palaeontologist Mark Allen Norell, and 'barsboldi' honours the late Mongolian palaeontologist Rinchen Barsbold (1957-2025), these being two scientists who have made exceptional contributions to the study of Paravian Dinosaurs. It is described from a single specimen (130108-MHGU-F4281) from an exposure of the Jiufotang Formation in the town of Lamadong, in Jianchang County, which is in western Liaoning Province.

Norellraptor barsboldi 130108-MHGU-F4281. (a) Whole specimen. (b) Skull in lateral view. (c) Close up of the rostrum. (d) Close up of the posterior part of skull. (e) Pectoral region. (f) Distal end of tail. Abbreviations: aof, antorbital fossa; arm, ascending ramus of maxilla; at, anterior tympanic recess; bt, basal tuber; bp, basypterygoid process; cf, coracoid fenestra; ct, caudal tympanic recess; cnV, 5th cranial nerve opening; cnVII, 7th cranial nerve opening; cv, cervical vertebra; d1, first dorsal vertebra; de, dentary; dt, dorsal tympanic recess; fo, foramen; fr, frontal; fu, furcula; gl, glenoid; h, humerus; la, lacrimal; lat, laterosphenoid; lcv, last caudal vertebra; lp, lateral pneumatic recess; mc, metacarpus; mxf, maxillary fenestra; na, nasal; oc, oto￾sphenoid crest; or, otic region; pa, parietal; paw, postantral wall; pmx, premaxilla; pp, paroccipital process; ppd, posterior processes of dentary; pt, pterygoid; pxf, promaxillary fenestra; r, radius; rp, retroarticular process; sa, surangular; sc, sca￾pula; so, supraoccipital; sp, sternal plate; sr, sclerotic ring; u, ulna; up, uncinate process; vor, ventral otic recess. Arrow indicates point of histological sampling. Scale bars are 50 mm (a); and 10 mm (b)–(f). Wang et al. (2026).

Norellraptor barsboldi has a skull triangular in lateral view, with an elongated snout, a vaulted area between the eyes, and very enlarged fenestra (skull openings). Its teeth are differentiated, with the premaxilary teeth being small and unserrated, while the maxilary teeth are larger, particularly so towards the back of the mouth, serrated, and hooked. Preserved plumage can be seen close to the right humerus and the synsacrum, ventral to the proximal caudal vertebrae, attached to the distal caudal vertebrae, ventral to the right tibiotarsus, and lateral to the right tarsometatarsus. However, the preservation of this is poor, preventing a detailed assessment of its structure.

Plumage of Norellraptor barsboldi (130108-MHGU-F4281). (a) whole specimen. (b) Distal tips of primary feathers. (c) Tibial plumage. (d) Distal tip of metatarsal feathers. (e) Plumage adjacent to humerus and thorax. (f) Plumage adjacent to ilium and tail base. (g) Distal tail feathers. Scale bars are 10 mm. Wang et al. (2026).

An osteological sample was taken from the distal portion of the mid-diaphysis of the left radius of specimen 130108-MHGU-F4281, and serial sectioned to give a view of its bone-structure. This section of bone had been crushed post-mortem, due to the weight of overlaying sediment. The bone is less than half a millimetre in diameter, and has a large medullary cavity lacking any internal structures, suggesting that the bone was heavily pneumatized in life. This is surrounded by a layer of laminated endosteal bone, making up 8-15% of the total bone thickness, then a thicker layer of periosteal bone, split into three layers by two lines of arrested growth (such lines typically form as an animal grows, with slowed growth in a season with less favourable conditions, such as winter or a dry season). This might be taken to mean the living Microraptor had lived at least two years after hatching. However, the large size of the inner cavity probably implies some total reabsorption of bone as the Dinosaur grew, making it several years older.

Histology of the left radius of 130108-MHGU-F4281. (a)–(c) Close-up of the left radius midshaft microstructure (d), (e). Physical transversal sections in transmitted (a), (d) fluorescent (b) and elliptically polarised light (c), (e). In (a)–(c) note an irregular interface between the inner periosteal bone and the endosteal bone (red arrow); a high difference in fluorescence between well-developed primary osteons of the zone 1 and of the inner group of osteons of the zone 2 (blue arrow); and ill￾developed primary of the outer group of osteons of the zone 2 (yellow arrow); a low fluorescence in the secondary osteonal bone (orange arrow). Compare the higher birefringence of the endosteal bone, an annulus-like tissue (white arrow), and early bone deposited to form zone 3 (black arrow). In (d), (e) note the occurrence of more organised osteocyte lacunae in the outer region of zone 1 and throughout the zone 2; increased birefringence in primary osteons of zone 1 (green arrow); in an annulus associate with Layer of Arrested Growth 1 (white arrow) and zone 3 (yellow arrow); and highly birefringent endosteal bone tissue (orange arrow). Abbreviations: ?ans, putative annulus; avbl, avascular layer; avr, avascular region; END, endosteal bone; FLB, fibro-lamellar bone; ICL, inner circumferential line; LAG, line of arrested growth; LAG-nvc, LAG crossing neurovascular canal; LAG1, inner circumferential layer; LAG2, outer line of arrested growth; ipos, ill developed primary osteon; lanvc, laminar neurovascular canal; lonvc, longitudinal neurovascular canal; meca, medullary cavity; onvc, neurovascular canal open on outer surface; osla, osteocyte lacuna; PER, periosteal bone; PFBM, parallel-fibered bone matrix; pos, primary osteon; pnvc, primary neurovascular canal; prpos, partially resorbed primary osteon; prsos, partially resorbed secondary osteon; ranvc, radial neurovascular canal; rel, resorption line; rupt, postfossilization rupture; snvc, secondary vascular canal; sos, secondary osteon; z1-3, first through third zone. Scale bars are 200 microns (a)-(c) and 100 microns (d), (e). Wang et al. (2026).

Norellraptor barsboldi shares many features with early Birds, but this appears to be a case of convergent evolution, with a phylogenetic reconstruction recovering it as a highly derived Microraptorine, and the Microraptors as the earliest branching group within the Paraves, i.e. the most distantly related group to the Birds within that larger group. This phylogeny shows the Microraptorines progressively acquiring 'Bird-like' traits over their history, apparently in response to similar evolutionary stimuli, something which Wang et al. interpret as evidence for the independent evolution of flight.

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Dwarf Planet 136199 Eris approaches opposition.

The dwarf planet 136199 Eris will reach opposition (i.e. be directly opposite the Sun seen from Earth) on Sunday 18 October 2026 at 6.32 pm GMT. This means that it will both be at its closest to the Earth this year, about 94.47 AU (94.47 times the average distance between the Earth and the Sun, or about 14, 133 000 000 km), and completely illuminated by the Sun. While it is not visible to the naked eye observer, the planets have phases just like those of the Moon; being further from the Sun than the Earth, 136199 Eris is 'full' when directly opposite the Sun. 

The orbit and position of 136199 Eris and selected Solar System planets at 7.00 pm GMT on Sunday 18 October 2026. JPL Small Body Database Browser.

Although this coincides with a First Quarter Moon, the prospects for viewing without a very powerful telescope are not as good. The dwarf planet will be in the constellation of Cetus and will be at its highest point in the sky at about midnight local time, from anywhere on Earth (this is because the rising and setting of objects in the sky is caused by the Earth's rotation, not the movement of the object). (Even at it's very brightest 136199 Eris will only have a Magnitude of 18.6, making it almost impossible to see with any but the largest of Earth-based telescopes, and where resolvable it will only be possible to see it as a point of light indistinguishable from a faint star.

136199 Eris orbits the Sun on an eccentric orbit tilted at an angle of 44.1° to the plane of the Solar System, which takes it from 35.9 AU from the Sun (35.9 times the average distance at which the Earth orbits the Sun) to 97.5 AU from the Sun (97.5 times the average distance at which the Earth orbits the Sun. With an average distance of 67.74 AU, 136199 Eris completes one orbit around the Sun every 558 years. This means that the planet is almost stationary compared to the faster moving Earth, so that it reaches Opposition only four days later each year than the year before, and reaches Solar Conjunction (when it is directly on the opposite side of the Sun to the Earth), roughly six months later.

136199 Eris was discovered on 5 January 2005 by a team led by Mike Brown of the Palomar Observatory in California. With a diameter of 2326 km it is considered to be the second largest dwarf planet in the Solar System (after 134340 Pluto) as well as the sixteenth largest body in the Solar System, excluding the Sun (though several moons, including our own, are larger). It is also the largest body in the Solar System never to have been visited by a spacecraft (again, with the exception of the Sun). 136199 Eris has a single moon, Dysnomia, which has a diameter of about 700 km and obits at a distance of about 37 350 km.

Labelled Hubble Space Telescope Image of 136199 Eris, showing its satellite Dysnomia. Captured on 12 June 2007. Mike Brown/NASA/European Space Agency/Wikimedia Commons.

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