dust devil near center
Mars Perseverance Sol 1314: Left Navigation Camera (Navcam) gif
NASA's Mars Perseverance rover acquired these images using its onboard Left Navigation Camera (Navcam). The camera is located high on the rover's mast and aids in driving.
Images acquired on Oct. 30, 2024 (Sol 1314) at the local mean solar time of 14:52:39 to 14:54:26.
Image Credit: NASA/JPL-Caltech
Assembled by Barley Culiner with GIMP
THE DEPARTMENT OF DEFENSE
ALL-DOMAIN ANOMALY RESOLUTION OFFICE
Report on the Historical Record of U.S. Government Involvement
with Unidentified Anomalous Phenomena (UAP)
Volume I
February 2024
OFFICE OF THE DIRECTOR OF NATIONAL INTELLIGENCE
Preliminary Assessment:
Unidentified Aerial Phenomena
https://www.dni.gov/files/ODNI/documents/assessments/Prelimary-Assessment-UAP-20210625.pdf
https://www.esa.int/Science_Exploration/Space_Science/Rosetta
https://sci.esa.int/web/rosetta/-/14615-comet-67p
Assembled by Barley Culiner with GIMP
| MISSION | HOST | INSTRUMENT | PRINCIPAL INVESTIGATOR(S) |
| Rosetta | Orbiter | ALICE | S. A. Stern (SwRI, Boulder, USA) |
| CONSERT | W. Kofman (LPG, Grenoble, France) | ||
| COSIMA | M. Hilchenbach (MPS, Katlenburg-Lindau, Germany) | ||
| GIADA | A. Rotundi (Università degli studi di Napoli “Parthenope”) | ||
| MIDAS | M. Bentley (IWF, Graz, Austria) | ||
| MIRO | M. Hofstadter (NASA/JPL, Pasadena, USA) | ||
| NAVCAM | The NAVCAM is commanded by the Rosetta Flight Dynamics and Flight Control Teams at ESOC. The data were processed and archived by the Rosetta Science Ground Segment (SGS) and the Planetary Science Archive Team (PSA) at ESAC. | ||
| OSIRIS | H. Sierks (MPS, Goettingen, Germany) | ||
| ROSINA | K. Altwegg (University of Bern, Switzerland) | ||
| RPCICA | H. Nilsson (Swedish Institute of Space Physics, Kiruna, Sweden) | ||
| RPCIES | J. Burch (SwRI, San Antonio, TX., USA) | ||
| RPCLAP | A. Eriksson (Swedish Institute of Space Physics, Uppsala, Sweden) | ||
| RPCMAG | K-H Glassmeier (TU Braunschweig, Germany) | ||
| RPCMIP | P. Henri (LPC2E/CNRS, Orléans, France) | ||
| RSI | M. Paetzold (University of Cologne, Cologne, Germany) | ||
| VIRTIS | F. Capaccioni (IAPS-INAF, Rome, Italy) | ||
| Philae Lander | APXS | G. Klingenhoefer (Gutenberg-University, Mainz, Germany) | |
| CIVA | J.P. Bibring (Institut d'Astrophysique Spatiale, France) | ||
| CONSERT | W. Kofman (LPG, Grenoble, France) | ||
| COSAC | F. Goesmann (MPS, Goettingen, Germany) | ||
| MUPUS | T. Spohn (DLR, Germany) | ||
| PTOLEMY | I. Wright (Open University, UK) | ||
| ROLIS | S. Mottola (DLR, Germany) | ||
| ROMAP | H-U. Auster (Technische Universitaet Braunschweig, Germany) | ||
| SD2 | A. Ercoli-Finzi, (Politecnico di Milano, Italy) | ||
| SESAME | M. Knapmeyer (DLR, Germany) | ||
| Ancillary | Shape Model | The shape models have been produced using data from the OSIRIS and NAVCAM instruments. Consult the CITATION_DESC in the label of each product you use and make sure that you cite / acknowledge the relevant data producer listed there. |
Pulsar Sounds
https://centralbuckscomputer.com/pulsars/audio/0329.mp3
https://centralbuckscomputer.com/pulsars/audio/0437.mp3
https://centralbuckscomputer.com/pulsars/audio/0531.mp3
https://centralbuckscomputer.com/pulsars/audio/0835.mp3
https://centralbuckscomputer.com/pulsars/audio/1055.mp3
Jewish Encyclopedia https://www.jewishencyclopedia.com/
Mars Perseverance Sol 1303: Right Mastcam-Z Camera stitch
NASA's Mars Perseverance rover acquired these images using its Right Mastcam-Z camera. Mastcam-Z is a pair of cameras located high on the rover's mast.
Images acquired on Oct. 19, 2024 (Sol 1303) at the local mean solar time of 12:54:00 to 12:56:37.
Image Credit: NASA/JPL-Caltech/ASU
Assembled by Barley Culiner with Microsoft ICE
Mars Perseverance Sol 1303: Right Mastcam-Z Camera stitch
NASA's Mars Perseverance rover acquired these images using its Right Mastcam-Z camera. Mastcam-Z is a pair of cameras located high on the rover's mast.
Images acquired on Oct. 19, 2024 (Sol 1303) at the local mean solar time of 12:56:52 to 13:00:57.
Image Credit: NASA/JPL-Caltech/ASU
Assembled by Barley Culiner with Microsoft ICE
Additional editing with GIMP
Mars Perseverance Sol 1299: Right Mastcam-Z Camera stitch
NASA's Mars Perseverance rover acquired these images using its Right Mastcam-Z camera. Mastcam-Z is a pair of cameras located high on the rover's mast.
Images acquired on Oct. 15, 2024 (Sol 1299) at the local mean solar time of 12:46:35 to 12:55:28.
Image Credit: NASA/JPL-Caltech/ASU
Assembled by Barley Culiner with Microsoft ICE
Additional editing with GIMP
full size image:
dust devil near center left
Mars Perseverance Sol 1299: Left Navigation Camera (Navcam) gif
NASA's Mars Perseverance rover acquired these images using its onboard Left Navigation Camera (Navcam). The camera is located high on the rover's mast and aids in driving.
Images acquired on Oct. 15, 2024 (Sol 1299) at the local mean solar time of 13:02:48 to 13:04:09.
Image Credit: NASA/JPL-Caltech
Assembled by Barley Culiner with GIMP
Disassemble Mercury in order to construct Dyson swarm
from
 |
| Gezeichnet Dan Gallagher (KBR Wyle Services, LLC) |
 |
| Gezeichnet Karl Bednarik |
if we disassembled Mercury to create a Dyson swarm would the rotation of the inner planets change
Disassembling Mercury to create a Dyson swarm would likely have a negligible effect on the rotation of the inner planets.
Here's why:
Mercury's small mass: Compared to the other planets, especially the gas giants, Mercury's mass is relatively insignificant. Its gravitational influence on the other planets is minimal.
Dyson swarm's distribution: A Dyson swarm would be distributed around the star, creating a relatively symmetrical mass distribution. This would minimize any gravitational perturbations on the inner planets.
Orbital mechanics: The orbits of the inner planets are primarily determined by the Sun's gravity. The removal of Mercury's mass would not significantly alter this balance.
While there might be some minor adjustments due to gravitational interactions, the overall stability of the inner planets' orbits would likely remain largely unaffected.
reorient satellite swarm to reduce the effects of climate change
collect solar energy and utilize power beaming technology
---------
Robotic swarm technology for rapid Mercury satellite construction factories
Mesh data and power beaming network required for Dyson swarm
---------
Viability of a Dyson Swarm as a Form of Dyson Sphere https://arxiv.org/abs/2109.11443
Power beaming comes of age https://www.technologyreview.com/2022/10/06/1060650/power-beaming-comes-of-age/
Researchers Enlist Robot Swarms to Mine Lunar Resources https://news.arizona.edu/news/researchers-enlist-robot-swarms-mine-lunar-resources
Autonomous Robot Swarms for Lunar Orbit Servicing and Space Asset Assembly https://techport.nasa.gov/view/106703
PJ65 Marble Movie Outbound
2024-09-20 17:00 UT
NASA / SwRI / MSSS
Mission Phase : PERIJOVE 65
PJ65 Marble movie outbound raw image frames
Assembled by Barley Culiner with GIMP
dust devil on left
Mars Perseverance Sol 1297: Right Navigation Camera (Navcam) gif
NASA's Mars Perseverance rover acquired these images using its onboard Right Navigation Camera (Navcam). The camera is located high on the rover's mast and aids in driving.
Images acquired on Oct. 13, 2024 (Sol 1297) at the local mean solar time of 14:08:52. to 14:11:05.
Image Credit: NASA/JPL-Caltech
Assembled by Barley Culiner with GIMP
dust devil on Right
dust devil near near center
Mars Perseverance Sol 1295: Left Navigation Camera (Navcam) gif
NASA's Mars Perseverance rover acquired these images using its onboard Left Navigation Camera (Navcam). The camera is located high on the rover's mast and aids in driving.
This image was acquired on Oct. 11, 2024 (Sol 1295) at the local mean solar time of 14:36:46 to 14:36:54.
Image Credit: NASA/JPL-Caltech
Assembled by Barley Culiner with GIMP
https://www.esa.int/Science_Exploration/Space_Science/Mars_Express
https://www.sciencedirect.com/science/article/pii/S0032063316304688?via%3Dihub
| MISSION | INSTRUMENT | PRINCIPAL INVESTIGATOR(S) |
| Mars Express | ASPERA-3 | R. Lundin (Swedish Institute of Space Science, Kiruna, Sweden) |
| HRSC | G. Neukum (Freie Universitaet, Berlin, Germany) | |
| MARSIS | G. Picardi (Universita di Roma 'La Sapienza', Rome, Italy), R. Orosei (IAPS, Rome, Italy) and J. Plaut (JPL, Pasadena, USA) | |
| MRS | M. Paetzold (University of Cologne, Germany) | |
| OMEGA | J.P. Bibring (Institut d'Astrophysique Spatiale, France) | |
| PFS | M. Giuranna (IAPS, Rome, Italy) | |
| SPICAM | F. Montmessin (LATMOS, Paris, France) | |
| VMC | A. Sanchez-Lavega (UPV-EHU, Bilbao, Spain) |
Extracted by Barley Culiner with NASAView
Additional editing with GIMP and Microsoft ICE
