The 71 files already ran. The comet map already ran. This is a neutron star and a tape of gas.
NASA’s Goddard Space Flight Center, Friday, Sept. 18, updated 3:38 p.m. ET: the Japan-led XRISM observatory recorded a giant star’s stellar wind being captured by its compact companion — clear indications of wind plasma falling onto a compact object that Goddard says have never been seen before. The system is BP Crucis, about 13,000 light-years away in Crux. The primary, Wray 977, is a blue hypergiant about 40 times the Sun’s mass and 60 times its size. The companion is pulsar GX 301-2: more than the Sun’s mass packed into a ball about 12 miles (20 kilometers) across, rotating every 11 minutes.
Twice in the pulsar’s 41.5-day orbit, near closest and farthest approach, X-ray flares last several days. XRISM pointed on Feb. 1, 2025, for about 16 hours near the end of a stronger flare. Resolve, built by NASA and JAXA, captured iron absorption lines displaced to lower energies — redshifted. The analysis: gas racing toward the pulsar at about 335,000 mph (540,000 kph). Roi Rahin, UMBC, led the work. Brian Williams, Goddard project scientist: BP Crucis is “an ideal laboratory to study wind-driven pulsar accretion.” A laboratory line is not a UAP. A redshift is a speed.
Goddard’s concept: as the pulsar crosses a dense stream, a messy disk forms, then breaks when there is not enough angular momentum, then rebuilds spinning the other way. That is accretion. It is not a craft. 3I/ATLAS already ran as a chemistry map. PURSUE 6 already ran as 71 files. We will not reprint them.
What this means for you
If you came for a saucer, this file is a letdown. If you came for a number, it is 335,000 miles per hour toward a 12-mile star.
Bottom line: Wind in. 335,000 mph. Not a craft. Not PURSUE 6.
GLHR NEWS explains the news. Not investment, tax, or trading advice. Do your own work before you act.
