A broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18b.

Close-in giant exoplanets with temperatures greater than 2,000 K ('ultra-hot Jupiters') have been the subject of extensive efforts to determine their atmospheric properties using thermal emission measurements from the Hubble Space Telescope (HST) and Spitzer Space Telescope. However, previous studies have yielded inconsistent results because the small sizes of the spectral features and the limited information content of the data resulted in high sensitivity to the varying assumptions made in the treatment of instrument systematics and the atmospheric retrieval analysis. Here we present a dayside thermal emission spectrum of the ultra-hot Jupiter WASP-18b obtained with the NIRISS instrument on the JWST.

A reflective, metal-rich atmosphere for GJ 1214b from its JWST phase curve.

There are no planets intermediate in size between Earth and Neptune in our Solar System, yet these objects are found around a substantial fraction of other stars. Population statistics show that close-in planets in this size range bifurcate into two classes on the basis of their radii. It is proposed that the group with larger radii (referred to as 'sub-Neptunes') is distinguished by having hydrogen-dominated atmospheres that are a few percent of the total mass of the planets.

Hemocyanins in spiders, XIV. Subunit composition of dissociation intermediates and its bearing on quaternary structure of Eurypelma hemocyanin.

The 37 S hemocyanin (24 subunits of 7 types) isolated from the tarantula, Eurypelma californicum, was dissociated partially by various agents and the dissociation intermediates analyzed for their subunit composition by crossed immunoelectrophoresis. The subunit composition of the native hemocyanin was reexamined and the pending problem of the ratio between subunits a and g (= c2) clarified. The subunits are present in the ratio of a:b:c:d:e:f:g = 4:2:2:4:4:4:4.

On the role of dimeric subunits in the quaternary structure of arthropod hemocyanins.

Partial alkaline dissociation of 24 S (12-meric), 35 S (24-meric) and 60 S (48-meric) hemocyanin from various arthropods was studied by polyacrylamide gradient gel electrophoresis and, in some cases, by electron microscopy. If there are no stable dimers among the subunits, dissociation starts by cleavage of interhexamer bonds, leading to intermediates which are hexamers or multiples of hexamers. Whenever a hemocyanin contained stable dimers, inter-hexamer bonds were also very stable as indicated by the formation of 30 S (19-meric) or 18 S (7-eric) intermediates as primary products.

Hemocyanins in spiders, IX. Homogeneity, subunit composition and the basic oligomeric structure of Eurypelma californicum hemocyanin.

37S hemocyanin isolated from the tarantula Eurypelma californicum was subjected to a variety of fractionation procedures: Electrophoresis in polyacrylamide gels, isoelectrofocusing, and ion exchange chromatography. Single fractions were dissociated at alkaline pH and/or by sodium dodecyl sulfate and the resulting subunits separated by polyacrylamide gel electrophoresis in gradient slab gels followed, in many cases, by quantitative estimation of the subunit bands. In addition, crossed immunoelectrophoresis was employed to analyze the subunit composition.