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AI-induced memory shortage is changing how devices are built, Fairphone says memory now 60% of materials cost — smaller laptop and phone makers are redesigning products and have to test for fake chips

With the ongoing memory shortage, smaller smartphone and laptop manufacturers are reportedly looking at new ways to tackle the problem. While some are changing how they design their products, others are placing orders months in advance and are even forced to test incoming memory chips to make sure they are not fake. A Reuters report suggests that more than the price, availability has become a bigger problem, with manufacturers struggling to secure enough chips in the first place. Still, device makers like Fairphone say that memory now makes up nearly 60% of a device's bill of materials.

Back in July, memory maker SK Hynix’s CEO Kwak Noh-jung said that 2027 will be the "worst year" for the ongoing memory shortage and expects the memory crunch to last until 2030. For smaller manufacturers, however, simply paying more for memory isn't always enough. The situation is particularly difficult for budget-oriented phones and laptops, where memory makes up a much larger portion of the overall product cost.

According to Raymond van Eck, CEO of repairable-phone maker Fairphone, memory can account for almost 60% of the bill of materials in phones costing around $400. That itself is worrying, as a recent Counterpoint Research report expects global smartphone shipments to fall 13.9% this year to 1.08 billion units, marking the largest annual decline on record.

Finnish phone maker Jolla has designed two motherboard versions, allowing it to switch between combined packages for discrete chips depending on availability. The company is also testing samples from every batch it receives to ensure new memory isn't being sold as refurbished hardware.

Similarly, laptop manufacturer Framework has been able to rely on its highly modular approach where customers can install memory salvaged from older laptops or opt for second-hand units, giving the company and its users another way to deal with limited supply. The company is also placing non-cancellable orders well in advance, even when it doesn't know the final price or exact delivery volume.

Back in July, it nearly doubled memory pricing for 32GB and 64GB variants of the Framework Laptop 13 Pro after receiving a cost update from its LPCAMM2 supplier. However, after sourcing new inventory at a reduced cost, the company recently announced a price drop for the same, including retroactive orders that have already shipped.

AI/ML STIG Lecture Series, 21 Sept 2026

15 September 2026 at 21:20

AI/ML STIG Lecture Series

Artificial Intelligence & Machine Learning Science and Technology Interest Group

AI/ML STIG about AI/ML STIG Lecture Series

Location

Virtual

dates

21 September 2026
4:00pm ET

Community

AI/ML STIG

Type

Lecture

Hands-On Session I: Agentic Coding and Research Tools

Speaker

Christopher Stubbs, Harvard University

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post AI/ML STIG Lecture Series, 21 Sept 2026 appeared first on NASA Science.

Cosmic Origins Community Meeting, 22 Sept 2026

15 September 2026 at 21:20

Cosmic Origins Community Meeting

Location

Virtual

Dates

22 September 2026
12:00pm – 1:00pm ET

Community

Cosmic Origins

Type

Meeting

Post-Ad ASTRA Community Science Workshop Update

Hosted by the COPAG Leadership

This community meeting aims to provide you with an overview and explanation of the processes and plans for mission concepts submitted to the Ad ASTRA workshop. The meeting will include a description of how the NASA Astrophysics Division will use the information gathered at the workshop. Additionally, this meeting aims to collect feedback and questions that the COPAG community may have regarding the process and plans that further mission concept selections. 

Please use this form to submit any comments, questions, or feedback for the COPAG community meeting: https://forms.gle/puBBTk1mo34WiGwP7 

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post Cosmic Origins Community Meeting, 22 Sept 2026 appeared first on NASA Science.

AGN SIG Spotlight Series, 22 Sept 2026

15 September 2026 at 21:20

AGN SIG Spotlight Series

Active Galactic Nuclei Science Interest Group

Our Spotlight Series highlights recent advances in AGN science, with a strong emphasis on participation from early-career researchers, and includes plenty of time for community discussion following the presentations. 

AGN SIG about AGN SIG Spotlight Series

Location

Virtual

Dates

22 September 2026
1:00pm ET / 10:00am PT

Community

AGN SIG

Type

Seminar

Unveiling the Role of Multi-Phase AGN Outflows with MIRACLE

Speaker

Dr. Matteo Ceci (Università di Firenze)

Abstract

Galaxy evolution is tightly connected to Active Galactic Nuclei (AGN) through feedback processes in which gas accretion onto the supermassive black hole drives powerful multiphase outflows. Detailed studies in the local Universe are crucial to resolve the physical scales and gas phases involved, enabling a comprehensive view of AGN-host interactions. I will present first results from the MIRACLE (Mid-IR Activity of Circumnuclear Line Emission) program, combining JWST/MIRI, MUSE, and ALMA observations of seven nearby Seyfert galaxies. Thanks to JWST’s spatial resolution (50-150 pc), we probe atomic and molecular gas in the circumnuclear regions and assess the impact of AGN activity on their host galaxies. Focusing on NGC 1365, we trace the ionized outflow up to kiloparsec scales and constrain its energetics and effects on star formation (SF). By combining mid-IR diagnostics with advanced photoionization and kinematic models, we reproduce ~60 optical and mid-IR emission lines, disentangling AGN- and SF-driven components and providing robust estimates of gas density, ionization, extinction, and outflow mass. We show that classical methods commonly adopted in the literature can underestimate outflow masses by up to an order of magnitude.

Disk Reflection as the Origin of the X-ray Polarization of NGC 4151 with IXPE

Speaker

Dr. Elias Kammoun (California Institute of Technology) 

Abstract

The geometry of the X-ray emitting region around accreting supermassive black holes remains poorly constrained, but X-ray polarimetry now offers a new and direct perspective on it. I will present a spectro-polarimetric study of the nearby type-1 AGN NGC 4151, combining two long IXPE observations from 2022 and 2024 with simultaneous XMM-Newton and NuSTAR spectroscopy. IXPE reveals a polarization degree of 6–7% above 4 keV aligned with the radio jet, plus a distinct low-energy component at a different angle, providing evidence for at least two polarized components in the 2–8 keV band. While earlier work read the hard X-ray signal as a radially extended, slab-like corona, I will test an alternative: that the polarization is instead dominated by relativistic reflection from an accretion disk illuminated by a compact, lamp-post corona. Fitting the IXPE Stokes spectra with recently developed models, we find the data favor a low coronal height and a wide torus opening angle, with disk reflection supplying ~20% of the 2–8 keV flux. The same configuration reproduces the full 0.4–79 keV spectrum, showing that disk reprocessing by a compact corona can account for both the polarization and the broadband spectral properties of NGC 4151.

Seminar Connection

Zoom Registration, you will receive connection details by email after registration: 

https://alaska.zoom.us/meeting/register/V1okit8uSk2ql97gegbdzg

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post AGN SIG Spotlight Series, 22 Sept 2026 appeared first on NASA Science.

DGCE SIG Seminar, 24 Sept 2026

15 September 2026 at 21:20

DGCE SIG Seminar

Diffuse Gas in Cosmic Ecosystems Science Interest Group

DGCE SIG about DGCE SIG Seminar

Location

Virtual

Dates

24 September 2026
4:00pm ET / 1:00pm PT

Community

DGCE SIG

Type

Seminar

How the Faint Radio Sky is Changing Our Understanding of Star Formation and Galactic Outflows

Speaker

Allison Matthews (Carnegie Observatories)

Abstract

In the last decade, with the commissioning of high sensitivity radio telescopes, we have opened a new window into the faint radio sky. These novel facilities probe fundamental physical processes that regulate star formation and characterize star formation in normal galaxies like our Milky Way over nearly all cosmic time. Deep observations from MeerKAT and LOFAR have revealed that prior observations may have missed half the star formation at all cosmic times. This discrepancy has critical implications across astrophysics: estimates of gravitational wave events, the frequency of astrophysical transients, and the chemical evolution of galaxies. These same high-sensitivity radio facilities are simultaneously placing critical constraints on the physical drivers of galactic winds that we believe regulate star formation across all of cosmic time. In this talk, I will present these findings and outline programs with next generation radio facilities that will improve our observational constraints on the rate and regulation of star formation across cosmic time.

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post DGCE SIG Seminar, 24 Sept 2026 appeared first on NASA Science.

Install iOS 27 today — there’s no reason to wait

12 September 2026 at 14:00
iOS 27 has so much to offer. Why wait? Install it now.

You can install the final version of iOS 27 right now and explore Siri AI and other new features before the official release. Here's how.

(via Cult of Mac - Your source for the latest Apple news, rumors, analysis, reviews, how-tos and deals.)

Deepfakes are wrecking influencers’ credibility, one fake ad at a time

12 September 2026 at 13:00

Influencers aren’t just battling competitors for brand deals. They’re now battling AI versions of themselves

Earlier this year, Emily Schuman, the creator of the lifestyle blog Cupcakes and Cashmere, saw a photo of herself she didn’t recognize on Instagram. In a sponsored ad, Schuman, who has more than 500,000 Instagram followers, is holding up a vial of GLP-1 drugs, advertising the telehealth company Gala. There was just one problem: Schuman had never heard of Gala and had nothing to do with the ad.

The ad was based on a digitally altered version of a selfie Schuman had taken in her car and posted on Instagram years earlier. Once her followers got wind, they flooded her inbox with questions about the sponsorship as it didn’t seem consistent with Schuman’s personal brand. Soon after, Schuman discovered this was just the beginning. There was also an Instagram post where an AI version of her with darker hair appears to apply foundation to promote a makeup brand called Meroda Cosmetics, and TikTok posts with generated images of her promoting the blood testing company Superpower.

Continue reading...

© Illustration: Guardian Design/Tiktok

© Illustration: Guardian Design/Tiktok

© Illustration: Guardian Design/Tiktok

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