Members Can Post Anonymously On This Site
-
Similar Topics
-
By USH
In 1992, Dr. Gregory Rogers a NASA flight surgeon and former Chief of Aerospace Medicine witnessed an event that would stay with him for more than three decades. Now, after years of silence, he’s finally revealing the details of a 15-minute encounter that shattered everything he thought he knew about aerospace technology.
With a distinguished career that includes support for 31 space shuttle launches, training as an F-16 pilot, and deep involvement in classified aerospace programs, Dr. Rogers brings unmatched credibility to the conversation. His firsthand account of observing what appeared to be a reverse-engineered craft, emblazoned with "U.S. Air Force" markings, raises profound questions about the true timeline of UAP development and disclosure.
The full interview spans nearly two hours. To help navigate the discussion, here’s a timeline so you can jump to the segments that interest you most.
00:00 Introduction and Dr. Rogers' Unprecedented Credentials 07:25 The 1992 Cape Canaveral Encounter Begins 18:45 Inside the Hangar: First Glimpse of the Craft 26:30 "We Got It From Them" - The Shocking Revelation 35:15 Technical Analysis: Impossible Flight Characteristics 43:40 Electromagnetic Discharges and Advanced Propulsion 52:20 The Cover Story and 33 Years of Silence 1:01:10 Why He's Speaking Out Now: Grush and Fravor's Influence 1:08:45 Bob Lazar Connections and Reverse Engineering Timeline 1:17:20 Flight Surgeon Stories: The Human Side of Classified Work 1:25:50 G-Force Brain Injuries: An Unreported Military Crisis 1:34:30 Columbia Disaster: When Safety Warnings Are Ignored 1:43:15 The Bureaucratic Resistance to Truth 1:50:40 Congressional Testimony and The Path Forward 1:58:25 Final Thoughts: Legacy vs. Truth
View the full article
-
By NASA
ESA/Hubble & NASA, M. J. Koss, A. J. Barth The light that the NASA/ESA Hubble Space Telescope collected to create this image reached the telescope after a journey of 250 million years. Its source was the spiral galaxy UGC 11397, which resides in the constellation Lyra (The Lyre). At first glance, UGC 11397 appears to be an average spiral galaxy: it sports two graceful spiral arms that are illuminated by stars and defined by dark, clumpy clouds of dust.
What sets UGC 11397 apart from a typical spiral lies at its center, where a supermassive black hole containing 174 million times the mass of our Sun grows. As a black hole ensnares gas, dust, and even entire stars from its vicinity, this doomed matter heats up and puts on a fantastic cosmic light show.
Material trapped by the black hole emits light from gamma rays to radio waves, and can brighten and fade without warning. But in some galaxies, including UGC 11397, thick clouds of dust hide much of this energetic activity from view in optical light. Despite this, UGC 11397’s actively growing black hole was revealed through its bright X-ray emission — high-energy light that can pierce the surrounding dust. This led astronomers to classify it as a Type 2 Seyfert galaxy, a category used for active galaxies whose central regions are hidden from view in visible light by a donut-shaped cloud of dust and gas.
Using Hubble, researchers will study hundreds of galaxies that, like UGC 11397, harbor a supermassive black hole that is gaining mass. The Hubble observations will help researchers weigh nearby supermassive black holes, understand how black holes grew early in the universe’s history, and even study how stars form in the extreme environment found at the very center of a galaxy.
Text credit: ESA
Image credit: ESA/Hubble & NASA, M. J. Koss, A. J. Barth
View the full article
-
By NASA
2 min read
Hubble Captures an Active Galactic Center
This Hubble image shows the spiral galaxy UGC 11397. ESA/Hubble & NASA, M. J. Koss, A. J. Barth The light that the NASA/ESA Hubble Space Telescope collected to create this image reached the telescope after a journey of 250 million years. Its source was the spiral galaxy UGC 11397, which resides in the constellation Lyra (The Lyre). At first glance, UGC 11397 appears to be an average spiral galaxy: it sports two graceful spiral arms that are illuminated by stars and defined by dark, clumpy clouds of dust.
What sets UGC 11397 apart from a typical spiral lies at its center, where a supermassive black hole containing 174 million times the mass of our Sun grows. As a black hole ensnares gas, dust, and even entire stars from its vicinity, this doomed matter heats up and puts on a fantastic cosmic light show.
Material trapped by the black hole emits light from gamma rays to radio waves, and can brighten and fade without warning. But in some galaxies, including UGC 11397, thick clouds of dust hide much of this energetic activity from view in optical light. Despite this, UGC 11397’s actively growing black hole was revealed through its bright X-ray emission — high-energy light that can pierce the surrounding dust. This led astronomers to classify it as a Type 2 Seyfert galaxy, a category used for active galaxies whose central regions are hidden from view in visible light by a donut-shaped cloud of dust and gas.
Using Hubble, researchers will study hundreds of galaxies that, like UGC 11397, harbor a supermassive black hole that is gaining mass. The Hubble observations will help researchers weigh nearby supermassive black holes, understand how black holes grew early in the universe’s history, and even study how stars form in the extreme environment found at the very center of a galaxy.
Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contact:
Claire Andreoli (claire.andreoli@nasa.gov)
NASA’s Goddard Space Flight Center, Greenbelt, MD
Share
Details
Last Updated Jun 27, 2025 Related Terms
Hubble Space Telescope Keep Exploring Discover More Topics From Hubble
Hubble Space Telescope
Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
Hubble’s Galaxies
Galaxy Details and Mergers
Hubble’s Night Sky Challenge
View the full article
-
By NASA
4 Min Read NASA to Gather In-Flight Imagery of Commercial Test Capsule Re-Entry
During the September 2023 daytime reentry of the OSIRIS-REx sample return capsule, the SCIFLI team captured visual data similar to what they're aiming to capture during Mission Possible. Credits: NASA/SCIFLI A NASA team specializing in collecting imagery-based engineering datasets from spacecraft during launch and reentry is supporting a European aerospace company’s upcoming mission to return a subscale demonstration capsule from space.
NASA’s Scientifically Calibrated In-Flight Imagery (SCIFLI) team supports a broad range of mission needs across the agency, including Artemis, science missions like OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security – Regolith Explorer), and NASA’s Commercial Crew Program. The SCIFLI team also supports other commercial space efforts, helping to develop and strengthen public-private partnerships as NASA works to advance exploration, further cooperation, and open space to more science, people, and opportunities.
Later this month, SCIFLI intends to gather data on The Exploration Company’s Mission Possible capsule as it returns to Earth following the launch on a SpaceX Falcon 9 rocket. One of the key instruments SCIFLI will employ is a spectrometer detects light radiating from the capsule’s surface, which researchers can use to determine the surface temperature of the spacecraft. Traditionally, much of this data comes from advanced Computational Fluid Dynamics modeling of what happens when objects of various sizes, shapes, and materials enter different atmospheres, such as those on Earth, Mars, or Venus.
“While very powerful, there is still some uncertainty in these Computational Fluid Dynamics models. Real-world measurements made by the SCIFLI team help NASA researchers refine their models, meaning better performance for sustained flight, higher safety margins for crew returning from the Moon or Mars, or landing more mass safely while exploring other planets,” said Carey Scott, SCIFLI capability lead at NASA’s Langley Research Center in Hampton, Virginia.
A rendering of a space capsule from The Exploration Company re-entering Earth’s atmosphere.
Image courtesy of The Exploration CompanyThe Exploration Company The SCIFLI team will be staged in Hawaii and will fly aboard an agency Gulfstream III aircraft during the re-entry of Mission Possible over the Pacific Ocean.
“The data will provide The Exploration Company with a little bit of redundancy and a different perspective — a decoupled data package, if you will — from their onboard sensors,” said Scott.
From the Gulfstream, SCIFLI will have the spectrometer and an ultra-high-definition telescope trained on Mission Possible. The observation may be challenging since the team will be tracking the capsule against the bright daytime sky. Researchers expect to be able to acquire the capsule shortly after entry interface, the point at roughly 200,000 feet, where the atmosphere becomes thick enough to begin interacting with a capsule, producing compressive effects such as heating, a shock layer, and the emission of photons, or light.
Real-world measurements made by the SCIFLI team help NASA researchers refine their models, meaning better performance for sustained flight, higher safety margins for crew returning from the Moon or Mars, or landing more mass safely while exploring other planets.
Carey Scott
SCIFLI Capability Lead
In addition to spectrometer data on Mission Possible’s thermal protection system, SCIFLI will capture imagery of the parachute system opening. First, a small drogue chute deploys to slow the capsule from supersonic to subsonic, followed by the deployment of a main parachute. Lastly, cloud-cover permitting, the team plans to image splashdown in the Pacific, which will help a recovery vessel reach the capsule as quickly as possible.
If flying over the ocean and capturing imagery of a small capsule as it zips through the atmosphere during the day sounds difficult, it is. But this mission, like all SCIFLI’s assignments, has been carefully modeled, choreographed, and rehearsed in the months and weeks leading up to the mission. There will even be a full-dress rehearsal in the days just before launch.
Not that there aren’t always a few anxious moments right as the entry interface is imminent and the team is looking out for its target. According to Scott, once the target is acquired, the SCIFLI team has its procedures nailed down to a — pardon the pun — science.
“We rehearse, and we rehearse, and we rehearse until it’s almost memorized,” he said.
Ari Haven, left, asset coodinator for SCIFLI’s support of Mission Possible, and Carey Scott, principal engineer for the mission, in front of the G-III aircraft the team will fly on.
Credit: NASA/Carey ScottNASA/Carey Scott The Exploration Company, headquartered in Munich, Germany, and Bordeaux,
France, enlisted NASA’s support through a reimbursable Space Act Agreement and will use SCIFLI data to advance future capsule designs.
“Working with NASA on this mission has been a real highlight for our team. It shows what’s possible when people from different parts of the world come together with a shared goal,” said Najwa Naimy, chief program officer at The Exploration Company. “What the SCIFLI team is doing to spot and track our capsule in broad daylight, over the open ocean, is incredibly impressive. We’re learning from each other, building trust, and making real progress together.”
NASA Langley is known for its expertise in engineering, characterizing, and developing spacecraft systems for entry, descent, and landing. The Gulfstream III aircraft is operated by the Flight Operations Directorate at NASA’s Armstrong Flight Research Center in Edwards, California.
Share
Details
Last Updated Jun 18, 2025 EditorJoe AtkinsonContactJoe Atkinsonjoseph.s.atkinson@nasa.govLocationNASA Langley Research Center Related Terms
Langley Research Center General Space Operations Mission Directorate Explore More
4 min read Career Exploration: Using Ingenuity and Innovation to Create ‘Memory Metals’
Article 20 hours ago 3 min read NASA Engineers Simulate Lunar Lighting for Artemis III Moon Landing
Article 23 hours ago 2 min read NASA Seeks Commercial Feedback on Space Communication Solutions
Article 2 days ago Keep Exploring Discover More Topics From NASA
Missions
Humans in Space
Climate Change
Solar System
View the full article
-
By NASA
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
NASA / DIP Start
July 27, 2022 at 10:00 AM EDTEnd
June 27, 2022 at 12:00 PM EST What It’s About?
DIP is hosting an online session to provide detailed information on the CDDR service, scope of the collaborative opportunity, partner responsibilities and ACO response submission instructions. The intent is to share information for interested parties to make an informed decision to collaborate and successfully respond to the ACO. (For the details of the collaboration, please read the full Announcement on sam.gov website (ID: 80ARC022JAI-DIP)).
The ACO is the first step to collaborate with NASA on this project. Flight Operators selected from the ACO process will contribute and benefit from the Sustainable Aviation (SA) demonstration to test and validate a cloud-based departure reroute service called Collaborative Digital Departure Reroute (CDDR) during FY22-24. CDDR has been shown to reduce fuel burn and emissions through reduced surface departure delays, which benefits re-routed flights as well as all other related departures in the operational area.
Agenda
Sustainable Aviation (SA) demonstrations overview DIP platform and digital services overview Expectations of partners ACO walkthrough and how to submit What to expect after an ACO is submitted Q/A Who Should Register?
This information session is primarily designed to assist flight operators with the ACO process. While other aviation industry participants are not discouraged from attending this session, the focus will be on the flight operator portion of our audience. An additional ACO for service providers will be announced on a future date.
Resources
Presentation slides Session Recording Request materials via email (arc-dip-ext@mail.nasa.gov) Digital Information Platform
Digital Information Platform Events
Facebook logo @NASA@NASAaero@NASA_es @NASA@NASAaero@NASAes Instagram logo @NASA@NASAaero@NASAes Linkedin logo @NASA Explore More
1 min read Digital Information Platform Library
Article 10 minutes ago 1 min read DIP Events
Article 11 minutes ago 1 min read DIP Request for Information (RFI) Information Session
Article 11 minutes ago Keep Exploring Discover More Topics From NASA
Missions
Humans In Space
Solar System Exploration
Eyes on the Solar System
Explore NASA’s History
Share
Details
Last Updated Jun 18, 2025 EditorLillian GipsonContactJim Bankejim.banke@nasa.gov Related Terms
Digital Information Platform Air Traffic Management – Exploration View the full article
-
-
Check out these Videos
Recommended Posts
Join the conversation
You can post now and register later. If you have an account, sign in now to post with your account.
Note: Your post will require moderator approval before it will be visible.