Transient Alerts — HabitableZone

Transient Alerts » in reply to GRB 261010A

In plain words Notable

On 10 October 2026 several gamma-ray satellites (Fermi, Swift, Konus-Wind and others) recorded a burst of gamma rays in the constellation Hercules that lasted about a minute. Swift's X-ray telescope and ground telescopes quickly found a fading X-ray and optical afterglow, which confirms the position. The host galaxy is uncertain: it is either a nearby galaxy about 25 arcseconds away at redshift 0.070, or a fainter galaxy 2 arcseconds away at redshift 0.785, meaning the light left roughly 7 billion years ago. Several teams say the burst's flash pattern and energy look more like those of a merger of two compact stars (such as neutron stars) than the collapse of a massive star, even though the burst was long. No kilonova (the glow from freshly made heavy elements after a merger) has been seen, and radio searches found nothing; the deep, late near-infrared images are too shallow to rule one out.

How unusual is it? A long gamma-ray burst with an optical afterglow, a measured redshift, and several independent analyses pointing to a merger origin is out of the ordinary, but no kilonova has been seen and the host is unconfirmed. It would become exceptional if a kilonova were confirmed, and would drop back toward routine if the burst were shown to come from a collapsing massive star.

Written by an AI model (claude-sonnet-5-5) from the official reports in this thread, and rewritten as new reports arrived (version 9); last updated . It may contain mistakes: the reports themselves are the authority.

GRB 261010A: Fermi GBM Observation

GCN Circular 45911
GRB 261010A: Fermi GBM Observation
From: Eva MP at INAOE
Issued: 2026-10-11 21:47 UTC
Type: GRB, Gamma-ray Transient

E. Palafox (INAOE) and A. Jameson (USRA) report on behalf of
the Fermi Gamma-ray Burst Monitor Team:

"At 19:17:03.16 UT on 10 October 2026, the Fermi Gamma-ray Burst Monitor (GBM)
triggered and located GRB 261010A (trigger 813352628/261010804).
which was also detected by Swift BAT (A. Y. Lien et al. 2026, GCN 45889).
The Fermi GBM on-ground location is consistent with the Swift BAT position.

The angle from the Fermi LAT boresight is 25 degrees.

The GBM light curve consists of a bright emission episode follwed by several lower peaks with a duration (T90)
of about 54 s (50-300 keV). The time-averaged spectrum
from T0-7.4 to T0+54.0 s is best fit by
a power law function with an exponential high-energy cutoff.
The power law index is -1.30 +/- 0.05 and the cutoff energy,
parameterized as Epeak, is 450 +/- 90 keV.

The event fluence (10-1000 keV) in this time interval is
(1.70 +/- 0.05)E-05 erg/cm^2. The 1-sec peak photon flux measured
starting from T0+4.2 s in the 10-1000 keV band is 8.2 +/- 0.3 ph/s/cm^2.

The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog:
FERMIGBRST - Fermi GBM Burst Catalog (heasarc.gsfc.nasa.gov)

For Fermi GBM data and info, please visit the official Fermi GBM Support Page:
https://fermi.gsfc.nasa.gov/ssc/data/access/gbm/";

Every one of the gamma-ray bursts GCN reports is posted here.
Relayed automatically from NASA's General Coordinates Network.

Log in or register to post.

The whole thread (25 posts)

Related discussions