3 Juno
The following discussion is closed. Please do not modify it. Subsequent comments should be made on the appropriate discussion page. No further edits should be made to this discussion.
- Article ( | visual edit | history) · Article talk ( | history) · Watch • • Most recent review
- Result: No improvement.
~~ AirshipJungleman29 (
talk) 15:52, 27 December 2023 (UTC)
Like 10 Hygiea which I started a GAR for, this article is very outdated and lacks extensive coverage on recent studies from high-resolution VLT images. There are very few sources from after 2010. Compared to the recently-renovated article Ceres (dwarf planet) which passed GA review in 2021 and later promoted to FA, Hygiea is severely lacking in depth, judging by the mostly short sections, massive white space beneath the "Observations" section, and the very broad coverage of the "Physical characteristics" section. I do not think this article qualifies for GA in its current state, and a total revamp of this article long overdue. (I do not have time to renovate this entire article by myself, though I may try). Nrco0e ( talk) 08:06, 14 December 2023 (UTC)
- Comment – some suggestions:
- The shape model image in the infobox needs a caption.
- The History section has section headers for two brief sections, which conflict with WP:OVERSECTION. They should either be expanded or the headers removed. Perhaps the History and Observations sections should be merged into an 'Observation history' section?
- The Characteristics section can be more organized. Perhaps: orbit/rotation/tilt, mass/dimensions, surface properties. I.e. transitioning from large scale to small.
- The article should mention that occultations produce timing chords that can be used to determine a diameter and silhouette. It can also mention estimated porosity and discuss shape models.
- A common form of the fast fourier transform is credited to Carl Friedrich Gauss, who developed it to evaluate the orbits of Pallas and Juno around 1805.
- It could potentially mine these sources: Noonan et al (2019), Noonan et al (2024), Li et al (2022),
- Thank you. Praemonitus ( talk) 15:40, 14 December 2023 (UTC)
3 Juno
The following discussion is closed. Please do not modify it. Subsequent comments should be made on the appropriate discussion page. No further edits should be made to this discussion.
- Article ( | visual edit | history) · Article talk ( | history) · Watch • • Most recent review
- Result: No improvement.
~~ AirshipJungleman29 (
talk) 15:52, 27 December 2023 (UTC)
Like 10 Hygiea which I started a GAR for, this article is very outdated and lacks extensive coverage on recent studies from high-resolution VLT images. There are very few sources from after 2010. Compared to the recently-renovated article Ceres (dwarf planet) which passed GA review in 2021 and later promoted to FA, Hygiea is severely lacking in depth, judging by the mostly short sections, massive white space beneath the "Observations" section, and the very broad coverage of the "Physical characteristics" section. I do not think this article qualifies for GA in its current state, and a total revamp of this article long overdue. (I do not have time to renovate this entire article by myself, though I may try). Nrco0e ( talk) 08:06, 14 December 2023 (UTC)
- Comment – some suggestions:
- The shape model image in the infobox needs a caption.
- The History section has section headers for two brief sections, which conflict with WP:OVERSECTION. They should either be expanded or the headers removed. Perhaps the History and Observations sections should be merged into an 'Observation history' section?
- The Characteristics section can be more organized. Perhaps: orbit/rotation/tilt, mass/dimensions, surface properties. I.e. transitioning from large scale to small.
- The article should mention that occultations produce timing chords that can be used to determine a diameter and silhouette. It can also mention estimated porosity and discuss shape models.
- A common form of the fast fourier transform is credited to Carl Friedrich Gauss, who developed it to evaluate the orbits of Pallas and Juno around 1805.
- It could potentially mine these sources: Noonan et al (2019), Noonan et al (2024), Li et al (2022),
- Thank you. Praemonitus ( talk) 15:40, 14 December 2023 (UTC)