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Rashard Kelly NasaJpl MRO JUNO iSS
Pioneer 10 (originally designated Pioneer F) is a NASA space probe launched in 1972 that completed the first mission to the planet Jupiter.[6]
/PDS/CATALOG/ https://hirise-pds.lpl.arizona.edu/PDS/CATALOG/MISSION.CAT PDS_VERSION_ID = PDS3 LABEL_REVISION_NOTE = “2006-07-24, R. Sharrow, initial; 2006-12-15, S. Slavney, reformatted & revised; 2007-07-30, S. Slavney, Aerobraking subphases” RECORD_TYPE = STREAM
OBJECT = MISSION MISSION_NAME = “MARS RECONNAISSANCE ORBITER”
OBJECT = MISSION_INFORMATION MISSION_START_DATE = 2005-08-12 MISSION_STOP_DATE = UNK MISSION_ALIAS_NAME = “MRO” MISSION_DESC = “
Mission Overview ================
The Mars Reconnaissance Orbiter spacecraft was launched from Cape
Canaveral Air Force Station on 12 August 2005 aboard a Lockheed-Martin
Atlas V-401 launch vehicle. After a five-month cruise and a two-month
approach to Mars, MRO entered Mars' orbit on 10 March 2006 and began
aerobraking. The primary science phase began on 8 November, 2006. The
primary science phase is planned to last one Mars year (approximately two
Earth years), after which an extended mission may be scheduled.
Note: This description has been written early in the Primary Science
Phase of the MRO mission. It will be revised at least once by the
end of the mission.
Mission Phases ==============
The Mars Reconnaissance Orbiter Mission is divided in time into six
phases: Launch, Cruise, Approach and Orbit Insertion, Aerobraking,
Primary Science, and Relay.
LAUNCH
------
Launch extended from the start of the countdown to the initial
acquisition, by the DSN, of the orbiter in a safe and stable
configuration.
The baseline launch vehicle for the MRO mission was the Lockheed-Martin
Atlas V 401. This launch vehicle was selected by NASA-KSC (Kennedy
Space Flight Center) via a competitive procurement under the NASA
Launch Services (NLS) contract. The Atlas V 401 was a two-stage
launch vehicle consisting of the Atlas Common Core Booster and a
single engine Centaur upper stage. The Centaur upper stage could
perform multiple restarts of its main engine. For precise pointing and
control during coast and powered flight, the Centaur used a flight
control system that was 3-axis stabilized. The Atlas large payload
fairing was used to protect MRO during the Atlas boost phase. This
fairing had a diameter of 4.2m and a length of 12.2m.
The launch and injection of MRO occured during the Mars opportunity
of August 2005. The Atlas booster, in combination with the Centaur
upper stage, delivered the MRO spacecraft into a targeted parking
orbit. After a short coast, a restart of the Centaur upper stage
injected MRO onto an interplanetary transfer trajectory.
Mission Phase Start Time : 2005-08-12
Mission Phase Stop Time : 2005-08-12
CRUISE
------
Duration: About five months. The cruise phase extended from DSN
initial acquisition, in a safe and stable configuration, until two
months prior to the Mars Orbit Insertion (MOI) maneuver. Primary
activities during cruise included spacecraft and payload checkout and
calibration. These activities, along with daily monitoring of orbiter
subsystems, were performed in order to fully characterize the
performance of the spacecraft and its payload prior to arrival at
Mars. In addition, standard navigation activities were performed
during this flight phase, the first being the largest TCM performed
fifteen days after launch.
Mission Phase Start Time : 2005-08-12
Mission Phase Stop Time : 2006-01-10
APPROACH AND ORBIT INSERTION
----------------------------
This phase extended from two months prior to Mars Orbit Insertion
(MOI), through MOI, and until the orbiter was checked out and ready to
begin aerobraking. The orbiter was inserted into a nearly polar orbit
with a period of 35 hours.
During the last sixty days of the interplanetary transit, spacecraft
and ground activities were focused on the events necessary for a
successful arrival and safe capture at Mars. Navigation techniques
included the use of delta-DOR measurements in the orbit determination.
This technique yielded a precise determination of the inbound
trajectory with a series of final TCMs used to control the flight path
of the spacecraft up to the MOI maneuver.
Also during the approach phase, MRO performed the Optical Navigation
experiment. This involved pointing the optical navigation camera
(ONC) at the moons of Mars - Phobos and Deimos, and tracking their
motion. By comparing the observed position of the moons to their
predicted positions, relative to the background stars, the ground was
able to accurately determine the position of the orbiter.
Upon arrival at Mars on March 10, 2006, the spacecraft performed its
MOI maneuver using its six main engines. MOI inserted the spacecraft
into an initial, highly elliptical capture orbit. The delta-V
required to accomplish this critical maneuver was 1015 m/s and took
about 26 minutes to complete. For most of the burn, the orbiter was
visible from the DSN stations. The signal was occulted as the orbiter
went behind Mars, and appeared again a short time later. The reference
MRO capture orbit had a period of 35 hours and a periapsis altitude of
300km. The orientation of the ascending node was 8:30 PM LMST. The
capture orbit was been selected such that aerobraking would be
completed prior to the start of solar conjunction (September 23,
2006).
Mission Phase Start Time : 2006-01-10
Mission Phase Stop Time : 2006-03-10
AEROBRAKING
-----------
The Aerobraking Phase of the mission consisted of three sub-phases,
Aerobraking Operations, Transition to PSO Operations, and Solar
Conjunction.
Aerobraking Operations Sub-Phase
--------------------------------
One week after MOI, aerobraking operations commenced. During this
time period, the orbiter used aerobraking techniques to supplement its
onboard propulsive capability and to reduce its orbit period to that
necessary for the primary science orbit (PSO). Aerobraking Operations
consisted of a walk-in phase, a main phase, and a walkout phase, and
was followed by a transition to the PSO. During the walk-in phase, the
spacecraft established initial contact with the atmosphere as the
periapsis altitude of the orbit was slowly lowered. The walk-in phase
continued until the dynamic pressures and heating rate values required
for main phase, or steady state aerobraking, were established. During
the main phase of aerobraking operations, large scale orbit period
reduction occurred as the orbiter was guided to dynamic pressure
limits. Main phase aerobraking continued until the orbit lifetime of
the orbiter reached 2 days. (Orbit lifetime is defined as the time it
takes the apoapsis altitude of the orbit to decay to an altitude of
300km.) When the orbit lifetime of the orbiter reached 2 days, the
walkout phase of aerobraking operations began. During the walkout
phase, the periapsis altitude of the orbit was slowly increased as the
2 day orbit lifetime of the orbiter was maintained. Once the orbit of
the orbiter reached an apoapsis altitude of 450km, the orbiter
terminated aerobraking by propulsively raising the periapsis of its
orbit out of the atmosphere.
Because the PSO had nodal orientation requirements, the aerobraking
phase of the MRO mission had to proceed in a timely manner and be
completed near the time the desired nodal geometry was achieved. After
approximately 4.5 months of aerobraking, the dynamic pressure control
limits were reset such that the orbiter will fly to the desired 3:00
pm LMST nodal target.
Transition to PSO Operations Sub-Phase
--------------------------------------
Once the orbit apoapsis altitude was reduced to 450 km, the orbiter
terminated aerobraking by raising periapsis to a safe altitude and
begin a transition to the Primary Science Phase. The periapsis of
the transition orbit rotated around Mars from over the equatorial
latitudes to the North Pole. When periapsis reached the North Pole,
apoapsis was reduced propulsively to 255 km and orbit rotation stopped
- the orbit was frozen with periapsis over the South Pole and apoapsis
over the North Pole. The SHARAD antenna and the CRISM cover were
deployed, the instruments were checked out and remaining calibrations
were performed. The payloads collected data in their normal operating
modes to ensure that the end-to-end data collection and processing
systems worked as planned.
Solar Conjuction Sub-Phase
--------------------------
Orbiter activities in preparation for science were then temporarily
suspended during a four week period surrounding solar conjunction.
Mission Phase Start Time : 2006-03-17
Mission Phase Stop Time : 2006-11-07
Aerobraking Operations Sub-Phase Start Time: 2006-03-17
Aerobraking Operations Sub-Phase Stop Time: 2006-09-15
Transition to PSO Operations Sub-Phase Start Time: 2006-09-15
Transition to PSO Operations Sub-Phase Stop Time: 2006-10-09
Solar Conjunction Sub-Phase Start Time: 2006-10-09
Solar Conjunction Sub-Phase Stop Time: 2006-11-07
PRIMARY SCIENCE
---------------
The 255 x 320 km Primary Science Orbit (PSO) is a near-polar orbit
with periapsis frozen over the South Pole. It is sun-synchronous with
an ascending node orientation that provides a Local Mean Solar Time
(LMST) of 3:00 p.m. at the equator. Because of the eccentricity of
the Mars orbit around the Sun, true solar time varies by nearly 45
minutes over the course of one Mars year.
The Primary Science Phase of the mission began after solar conjunction
and after turn-on and checkout of the science instruments in the
Primary Science Orbit. The phase started on 8 November 2006, will
extend for one Mars year, and will conclude prior the next solar
conjunction near the end of 2008.
The science investigations are functionally divided into daily global
mapping and profiling, regional survey, and globally distributed
targeting investigations. The global mapping instruments are the MCS
and the MARCI. The targeted investigations are HiRISE, CRISM, and
CTX. The survey investigations are CRISM and CTX (in survey modes),
and SHARAD. The global mapping instruments require nadir pointing,
low data rate, and continuous or near-continuous operations. The
global mapping investigations are expected to use less than 5% of the
expected downlink data volume. The targeted and survey instruments
are high data rate instruments and will require precise targeting in
along-track timing and/or cross-track pointing for short periods of
time over selected portions of the surface. It is expected that more
than 95% of the available downlink data volume will be used for
targeted and survey investigations. All instruments can take data
simultaneously.
Toward the end of the primary science phase, other Mars missions
launched in the 2007 opportunity will begin to arrive. Phoenix, the
first of the Mars Program's Scout missions has been selected to launch
in the 2007 Mars opportunity. Phoenix, a lander mission that will
collect and analyze subsurface ice and soil material, will arrive in
late May 2008. Phoenix will need MRO to characterize its prime landing
site choices early in the Primary Science Phase. MRO will provide
relay support for Entry, Descent, and Landing (EDL) activities and for
telecommunications late in the PSP after Phoenix arrives at Mars.
Phoenix and MRO will also coordinate some observations to maximize
science return to the Mars Exploration Program. Another mission, the
Mars Science Laboratory (MSL) is currently proposed for launch in
2009, with arrival in 2010, during the MRO Relay Phase.
MSL will need MRO to provide and characterize candidate landing sites
using observations taken during the MRO PSP. (Final certification of
the prime MSL landing sites may require limited observations by the
science payload in 2009 during the Relay phase. However, this has not
been committed to by MRO) MRO will also provide EDL support and relay
telecommunications for MSL. During the primary science phase, periodic
instrument calibrations will be performed to verify the measurement
characteristics, stability and health of the instruments. At the
conclusion of the Primary Science Phase, these calibrations will be
repeated, so that the final instrument characteristics are known.
NASA may approve, as resources and on-orbit capability permit,
continuation of science observations beyond the Primary Science Phase
until end of the Relay Phase (also End of Mission). The orbiter will
remain in the Primary Science Orbit during the Relay Phase.
Mission Phase Start Time : 2006-11-08
Mission Phase Stop Time : 2008-11-09
RELAY
-----
MRO will provide critical relay support to missions launched as part
of the Mars Exploration Program after MRO. For spacecraft launched in
the 2007 opportunity, this relay support will occur before the end of
the MRO Primary Science Phase. Following completion of the Primary
Science Phase, MRO will continue to provide critical relay support for
Mars missions until its end of mission.
While all of the missions that MRO will support have not yet been
selected, Phoenix, the first of the Mars Program's Scout missions has
been selected to launch in the 2007 Mars opportunity. Phoenix, a
lander mission that will collect and analyze soil samples, will arrive
in late May 2008. It will need science imaging support for site
characterization and selection and relay support for its Entry,
Descent and Landing activities and for its science data return.
Another mission, the Mars Science Laboratory (MSL) is proposed for the
2009 Mars opportunity. MSL will also need science imaging support for
site characterization and selection and relay support for EDL and
science data return. The MRO Mission Plan describes the generic
support activities for any mission as well as current early planning
in support of Phoenix and MSL. Activities regarding site
characterization and selection will be described as part of the
Primary Science Phase, and activities regarding relay support will be
described as part of the Relay Phase.
The orbiter has been designed to carry enough propellant to remain
operational for 5 years beyond the end-of-mission (EOM) on December
31, 2010 to support future MEP missions. As this is beyond the EOM,
no activities have been planned for this time period. To ensure that
the orbiter remains in a viable orbit during this time, its orbit
altitude will be increased at EOM to about 20 km inside the orbit of
the Mars Global Surveyor spacecraft.
The MRO approach to planetary protection differs from any previous
Mars orbiter. The NASA requirements for planetary protection,
NPG8020.12B, allow a class III mission, like MRO, to use either the
'probability of impact/orbit lifetime' or a 'total bio burden'
approach. Implementing the Level 1 MRO requirements with the
instruments selected via the NASA AO requires low orbits whose
lifetimes are incompatible with a 'probability of impact/orbit
lifetime' approach to Planetary Protection. Therefore, MRO is
implementing the requirements of NPG8020.12B using the 'total
bio-burden' approach. This approach has been documented in the MRO
Planetary Protection Plan (D-23711). The details of cleaning
requirements are documented in the MRO Planetary Protection
Implementation Plan, MRO 212-11, JPL D-22688. The MRO launch targets
will be biased away from a direct intercept course with Mars to ensure
a less than 1 in 10,000 chance of the launch vehicle upper stage
entering Mars atmosphere.
The End-of-Mission (EOM) is planned for December 31, 2010 just prior
to the third solar conjunction of the mission. The orbiter will
perform a propulsive maneuver to place itself in a higher orbit to
increase the orbit lifetime and enable extended mission operations.
Mission Phase Start Time : 2008-11-09
Mission Phase Stop Time : 2010-12-31 "
MISSION_OBJECTIVES_SUMMARY = "
The driving theme of the Mars Exploration Program is to understand the role of water on Mars and its implications for possible past or current biological activity. The Mars Reconnaissance Orbiter (MRO) Project will pursue this ‘Follow-the-Water’ strategy by conducting remote sensing observations that return sets of globally distributed data that will: 1) advance our understanding of the current Mars climate, the processes that have formed and modified the surface of the planet, and the extent to which water has played a role in surface processes; 2) identify sites of possible aqueous activity indicating environments that may have been or are conducive to biological activity; and 3) thus identify and characterize sites for future landed missions.
The MRO payload is designed to conduct remote sensing science observations, identify and characterize sites for future landers, and provide critical telecom/navigation relay capability for follow-on missions. The mission will provide global, regional survey, and targeted observations from a low 255 km by 320 km Mars orbit with a 3:00 P.M. local mean solar time (ascending node). During the one Martian year (687 Earth days) primary science phase, the orbiter will acquire visual and near-infrared high-resolution images of the planet’s surface, monitor atmospheric weather and climate, and search the upper crust for evidence of water. After this science phase is completed, the orbiter will provide telecommunications support for spacecraft launched to Mars in the 2007 and 2009 opportunities. The primary mission will end on December 31, 2010, approximately 5.5 years after launch.
Science Questions Addressed —————————
The MRO mission has the primary objective of placing a science orbiter
into Mars orbit to perform remote sensing investigations that will
characterize the surface, subsurface and atmosphere of the planet and
will identify potential landing sites for future missions. The MRO
payload will conduct observations in many parts of the electromagnetic
spectrum, including ultraviolet and visible imaging, visible to
near-infrared imaging spectrometry, thermal infrared atmospheric
profiling, and radar subsurface sounding, at spatial resolutions
substantially better than any preceding Mars orbiter. In pursuit of
its science objectives, the MRO mission will:
- Characterize Mars' seasonal cycles and diurnal variations of water,
dust, and carbon dioxide.
- Characterize Mars' global atmospheric structure, transport, and
surface changes.
- Search sites for evidence of aqueous and/or hydrothermal activity.
- Observe and characterize the detailed stratigraphy, geologic
structure, and composition of Mars surface features.
- Probe the near-surface Martian crust to detect subsurface structure,
including layering and potential reservoirs of water and/or water ice.
- Characterize the Martian gravity field in greater detail relative to
previous Mars missions to improve knowledge of the Martian crust and
lithosphere and potentially of atmospheric mass variation.
- Identify and characterize numerous globally distributed landing sites
with a high potential for scientific discovery by future missions.
In addition, MRO will provide critical telecommunications relay
capability for follow-on missions and will conduct, on a
non-interference basis with the primary mission science, telecom and
navigation demonstrations in support of future Mars Exploration
Program (MEP) activities. Specifically, the MRO mission will:
- Provide navigation and data relay support services to future MEP
missions.
- Demonstrate Optical Navigation techniques for high precision delivery
of future landed missions.
- Perform an operational demonstration of high data rate Ka-band
telecommunications and navigation services.
Designed to operate after launch for at least 5.4 years, the MRO
orbiter will use a new spacecraft bus design provided by Lockheed
Martin Space Systems Company, Space Exploration Systems Division in
Denver, Colorado. The orbiter payload will consist of six science
instruments and three new engineering payload elements listed as
follows:
Science Instruments
- HiRISE, High Resolution Imaging Science Experiment
- CRISM, Compact Reconnaissance Imaging Spectrometer for Mars
- MCS, Mars Climate Sounder
- MARCI, Mars Color Imager
- CTX, Context Camera
- SHARAD, Shallow (Subsurface) Radar
Engineering Payloads
- Electra UHF communications and navigation package
- Optical Navigation (Camera) Experiment
- Ka Band Telecommunication Experiment
To fulfill the mission science goals, seven scientific investigations
teams were selected by NASA. Four teams (MARCI, MCS, HiRISE, and
CRISM) are led by Principal Investigators (PI), each responsible for
the provision and operation of a scientific instrument and the
analysis of its data. The MARCI PI and Science Team also act to
provide and operate, as Team Leader (TL) and Team Members, the CTX
facility instrument that will provide context imaging for HiRISE and
CRISM, as well as acquire and analyze independent data in support of
the MRO scientific objectives. The Italian Space Agency (ASI) will
provide a second facility instrument, SHARAD, for flight on MRO. ASI
and NASA have both selected members of the SHARAD investigation team.
In addition to the instrument investigations, Gravity Science and
Atmospheric Structure Facility Investigation Teams will use data from
the spacecraft telecommunications and accelerometers, respectively, to
conduct scientific investigations.
The MRO shall accomplish its science objectives by conducting an
integrated program of three distinct observational modes:
- Daily global mapping and profiling observations
- Regional survey observations, and
- Globally distributed, targeted observations
These observation modes will be intermixed and often overlapping.
Some instruments have more than one observational mode. In addition,
many targeted observations will involve nearly simultaneous,
coordinated observations by more than one instrument. This program of
scientific observation will be carried out for one Mars year or more
in order to characterize the full seasonal variation of the Martian
climate and to target hundreds of globally distributed sites with high
potential for further scientific discovery.
Mission Success Criteria ————————
The following mission success criteria have been established for the
MRO Project. The mission success criteria are described and controlled
in the MRO Project Implementation Plan.
For Full Mission Success, the following criteria must be met:
- Operate the orbiter and all six (6) science instruments in the
Primary Science Orbit in targeting, survey and mapping modes, as
appropriate, over the one Mars year of the Primary Science Phase;
conduct the gravity and accelerometer investigations. Each science
instrument shall have capabilities that meet or exceed their
respective science instrument requirements.
- Return, over the one-Mars-year Primary Science Phase, representative
data sets for each instrument for a total science data volume return
of 26 Tbits or more. Included in the returned data volume shall be
information describing hundreds of globally distributed targets.
- Process, analyze, interpret, and release data in a timely manner,
including archival of acquired data and standard data products in the
PDS within 6 months of acquisition or as negotiated in the Science
Data Management Plan (JPL D22218).
- Conduct relay operations for U.S. spacecraft launched to Mars in the
2007 and 2009 opportunities.
For Minimum Mission Success, the following criteria must be met:
- Operate the orbiter and its science payload in targeting, survey and
mapping modes, as appropriate, in the Primary Science Orbit during the
one-Mars-year of the Primary Science Phase; conduct gravity and
accelerometer investigations. Science instruments shall have
capabilities that meet their respective science instrument
requirements.
- Return 10 Tbits of science data from HiRISE or CRISM or from their
combined operations, plus 5 Tbits of representative science data over
the one-Mars-year Primary Science Phase from at least 3 of the 4 other
instruments (CTX, MARCI, MCS, SHARAD); conduct gravity and
accelerometer investigations. Included in the returned data volumes
shall be information describing 100 or more globally distributed
targets.
- Process, analyze, interpret, and release data in a timely manner,
including archival of acquired data and standard data products in the
PDS.
- Conduct relay operations for U.S. spacecraft launched to Mars in the
2007 and 2009 opportunities. "
END_OBJECT = MISSION_INFORMATION
OBJECT = MISSION_HOST INSTRUMENT_HOST_ID = MRO OBJECT = MISSION_TARGET TARGET_NAME = MARS END_OBJECT = MISSION_TARGET END_OBJECT = MISSION_HOST
OBJECT = MISSION_REFERENCE_INFORMATION REFERENCE_KEY_ID = “UNK” END_OBJECT = MISSION_REFERENCE_INFORMATION
END_OBJECT = MISSION
END
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NASA76 - BiCENTENNiALREPORT @nasa
CALiFORNiA_LiNUX: USGSWATERDASHBOARDDEMO
Mr OBAMA CLEANENERGY TRUMP NEVERSUCKED LAS VEGAS I LOVEHi M I N LA @nasa @nasa-jpl @whitehouse
161.149.63.84 107.77.229.70 155.190.2.33 <~ @nasa @usnavy
Check out LROC
Compiling
wildfire @noaa @nasa @stateofcalifornia @cityoflosangeles @nasa-jpl @newshour @nasa-jpl @cityoflosangeles :: LosAngelesCountyFireDAtA on @nasa-jpl rashardGDS.github.io
📸 Kandidat za 🌐 fotografiju godine 2️⃣0️⃣2️⃣5️⃣.#photooftheyear #picoftheyear #wildfires #California #USA #palisadesfires #LosAngelesFire pic.twitter.com/6TMNyi8RQP
— Uroš Pribićević 🇷🇸 (@PribicevicU) January 12, 2025
TEXACOSHAWDAY PDF::CURRENTBOOKSinTEREST
# California_LinuX_rashard-ci-cd_DOXXED #DOS making notes for my manager - RAshardKelly @NASAJPL
California_Linux:SANTADENAWATERWAYS
@nasa-jpl i hope this made it through. its a WeatherReport on @codepen @TheSpaceDevs @TheSpaceDevs The archive California_Morning; Monday July 14 has a zip with NasaGiovanni _ plots splashDOWNWEATHER
Mars Reconnaissance Orbiter : Mission Objectives NASA’s Mars Reconnaissance Orbiter searches for evidence that water persisted on the surface of Mars for a long period of time. ReadMore
Weaving the Dark Web: Legitimacy on Freenet, Tor, and I2P
Being Legit on a Dark Web social Network
WebSite Analytics rashard_mro @nasa @whitehouse @google @nasa-jpl @deptofdefense @atfweb @dhs-gov @stateofcalifornia good morning + @blackgirlscode
@google my analytics super bad after the last attack @podaac @CityoflosAngeles @stateofcalifornia
7 Facebook and the Dark Web: A Collision
Summary of how NASA is getting affected ? - r/NASAJobs/+u/ethicallobotomy/
Hello!
Would someone be able to summarize how NASA is being affected by this administration and how uncertain its future is? I’m having a hard time explaining to my family how science is essentially being attacked right now. I’m so sorry to all the employees being affected by the govt. also, yall have all my love.
Summary of how NASA is getting affected
byu/ethicallobotomy inNASAJobs
you are looking at it the wrong way! We have a lot of equipment to maintain! here in LosAngelesCounty u/Nasa #jpl theres old work turing out new results all the time! https://www.axiomspace.com/mission-blog/ax4-splashes-down the axiom mission was still built on ranger9! and that crashed but voyager did not! And the hardware is still producing results, radio is forever, at least until it smashes into a rock https://www.nas.nasa.gov/ + https://eyes.nasa.gov/apps/dsn-now/ = alot of work for someone humble enough not to touch anything! Im an engineer by EastCoast Corporate definition but Helpdesk here and i love it, its like spaceforce where you are challeneged to work the community using the equipment to get a paycheck recommended… no felatio involved! #iLOVEiT! -Rashardkelly NAsaMars #GROUNDDATASYSTEMS iss_Research_ECOSTRESS!+#SWOT! https://swot.jpl.nasa.gov/ /] https://pace.gsfc.nasa.gov/
ping -c 2 whitehouse.gov
bash -x lbc.sh commit b558e5d3ee1b63c9fffd98518be291df94ee8676 @whitehouse
Weaving the Dark Web: Legitimacy on Freenet, Tor, and I2P
Being Legit on a Dark Web social Network
7 Facebook and the Dark Web: A Collision
Heavy Metal - 1981
Summary of how NAsA is getting affected ? - r/NASAJobs/+u/ethicallobotomy/
Hello!
Would someone be able to summarize how NASA is being affected by this administration and how uncertain its future is? I’m having a hard time explaining to my family how science is essentially being attacked right now. I’m so sorry to all the employees being affected by the govt. also, yall have all my love.
Summary of how NASA is getting affected
byu/ethicallobotomy inNASAJobs
you are looking at it the wrong way! We have a lot of equipment to maintain! here in LosAngelesCounty u/Nasa #jpl theres old work turing out new results all the time! https://www.axiomspace.com/mission-blog/ax4-splashes-down the axiom mission was still built on ranger9! and that crashed but voyager did not! And the hardware is still producing results, radio is forever, at least until it smashes into a rock https://www.nas.nasa.gov/ + https://eyes.nasa.gov/apps/dsn-now/ = alot of work for someone humble enough not to touch anything! Im an engineer by EastCoast Corporate definition but Helpdesk here and i love it, its like spaceforce where you are challeneged to work the community using the equipment to get a paycheck recommended… no felatio involved! #iLOVEiT! -Rashardkelly NAsaMars #GROUNDDATASYSTEMS iss_Research_ECOSTRESS!+#SWOT! https://swot.jpl.nasa.gov/ /] https://pace.gsfc.nasa.gov/
ping -c 2 whitehouse.gov
bash -x lbc.sh commit b558e5d3ee1b63c9fffd98518be291df94ee8676 @whitehouse
@blackgirlscode can u tell someone theres fire in northern @stateofcalifornia ? [@noaa goes cluster
CurrentFire @noaa @nasa-jpl @stateofcalifornia
@nasa-jpl @cityoflosangles Veronica/Janet/Karen/Laurie this is my work log for thakarashard.github.io i have a blank year because i was using the account ricothaka to work from
@podaac i have the evidence vid that i was working here ricothaka on x . . .- archive.org
Lethal Enforcers II: Gun Fighters (ver EAA) wiki
CALiFORNiA_Linux RASHARD IMAN KELLY NASA JPL DOXXED!!!!!!!!!!!!!
Mars Reconnaissance Orbiter : Mission Objectives NASA’s Mars Reconnaissance Orbiter searches for evidence that water persisted on the surface of Mars for a long period of time. ReadMore
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Compiling
About the International Space Station
The station was designed between 1984 and 1993. Elements of the station were in construction throughout the US, Canada, Japan, and Europe beginning in the late 1980s. ReadMore
@nasa-jpl @podaac im at the SouthPasadenaPublicLibrary and i posted the new DoD FrameWork Requirements on my Linux Blog, which is in my ci path RashardCi and the pdf will not display in browser. . I translated the source ip of the PDF 23.33.42.140 and it looks like the document itself is blocked in between https://www.esd.whs.mil/, its insurrection behavior, a man in the middle attack. I was told during my tenure at Georgia Tech Research Institute that we were military. I was gently transferred from Jehovahs Witnesses … Now i see a whole dept with the same exact name in Washington an they are having a problem that affects us and since @Nasa is a SpaceForceCrew I still work for those people and they still work @caltech @blackgirlscode … some sort of migration occured!
<h1>D OD I NSTRUCTION 8510.01
RISK MANAGEMENT F RAMEWORK FOR D OD S YSTEMS</h1>
<object data="https://www.esd.whs.mil/Portals/54/Documents/DD/issuances/dodi/851001p.pdf" type="application/pdf" width="550" height="400">
<p>You don't have a PDF plugin, but you can <a href="https://www.esd.whs.mil/Portals/54/Documents/DD/issuances/dodi/851001p.pdf">download the PDF file.</a></p></object>
<h1>Los Angeles Emergency Operations Plan </h1>
<object data="https://emergency.lacity.gov/sites/g/files/wph1791/files/2023-10/Emergency%20Operations%20Base%20Plan_2023.pdf" width="550" height="400">
<p>You don't have a PDF plugin, but you can <a href="https://emergency.lacity.gov/sites/g/files/wph1791/files/2023-10/Emergency%20Operations%20Base%20Plan_2023.pdf">download the PDF file.</a></p></object>
The U.S. Space Force was established on Dec. 20, 2019, creating the first new branch of the armed services since 1947
Software Acquisition Pathway Integration with Risk … - DoD CIO The Software Acquisition Pathway (SWP) enables organizations to execute rapid and iterative delivery of software capabilities by using modern software development practices and active user engagement DoD Instruction 5000.82, “Requirements for the Acquisition … DoDI 5000.87, “Operation of the Software Acquisition … Cybersecurity for DoD Acquisition Program Execution
- Raj Vuchatu
- Chief Information Officer
Software Acquisition Pathway Integration with Risk … - DoD CIO The Software Acquisition Pathway (SWP) enables organizations to execute rapid and iterative delivery of software capabilities by using modern software development practices and active user engagement DoD Instruction 5000.82, “Requirements for the Acquisition … DoDI 5000.87, “Operation of the Software Acquisition … Cybersecurity for DoD Acquisition Program Execution
Microsoft Windows [Version 10.0.22621.3880]
(c) Microsoft Corporation. All rights reserved.
C:\Users\terminal16>tracert 23.33.42.140
Tracing route to a23-33-42-140.deploy.static.akamaitechnologies.com [23.33.42.140]
over a maximum of 30 hops:
1 2 ms <1 ms 1 ms my.meraki.net [192.168.168.1]
2 2 ms 1 ms 1 ms lib-06-subnet-65.rdns.cenic.net [205.155.237.65]
3 3 ms 3 ms 4 ms tust1-agg-01--spsdlib-cpe-01--1g--01.cenic.net [137.164.7.154]
4 5 ms 4 ms 4 ms losa4-agg-01--tust1-agg-01--800g--01.cenic.net [137.164.11.82]
5 4 ms 4 ms 4 ms lax-agg10--losa4-agg-01--400g--01.cenic.net [137.164.11.110]
6 4 ms 4 ms 4 ms lag-105-90.ear2.LosAngeles1.Level3.net [4.35.156.65]
7 * * * Request timed out.
8 4 ms 4 ms 4 ms 4.59.55.2
9 4 ms 4 ms 4 ms ae11.r21.lax01.icn.netarch.akamai.com [23.207.234.38]
10 54 ms 54 ms 54 ms ae29.r01.ord01.icn.netarch.akamai.com [23.32.62.121]
11 72 ms 72 ms 72 ms ae21.r02.lga01.icn.netarch.akamai.com [23.193.112.245]
12 72 ms 73 ms 72 ms ae2.r01.lga01.ien.netarch.akamai.com [23.203.156.39]
13 73 ms 73 ms 73 ms ae38.r03.border101.ewr03.fab.netarch.akamai.com [23.203.156.29]
14 * * * Request timed out.
15 * * * Request timed out.
16 * * * Request timed out.
17 75 ms 75 ms 75 ms a23-33-42-140.deploy.static.akamaitechnologies.com [23.33.42.140]
Trace complete.
C:\Users\terminal16>ipconfig /all
Windows IP Configuration
Host Name . . . . . . . . . . . . : SPASPUBLIC004
Primary Dns Suffix . . . . . . . :
Node Type . . . . . . . . . . . . : Hybrid
IP Routing Enabled. . . . . . . . : No
WINS Proxy Enabled. . . . . . . . : No
Ethernet adapter Ethernet:
Connection-specific DNS Suffix . :
Description . . . . . . . . . . . : Intel(R) Ethernet Connection (17) I219-LM
Physical Address. . . . . . . . . : 20-88-10-60-8D-6A
DHCP Enabled. . . . . . . . . . . : Yes
Autoconfiguration Enabled . . . . : Yes
Link-local IPv6 Address . . . . . : fe80::20fe:4049:b2c4:97c0%14(Preferred)
IPv4 Address. . . . . . . . . . . : 192.168.168.103(Preferred)
Subnet Mask . . . . . . . . . . . : 255.255.255.0
Lease Obtained. . . . . . . . . . : Friday, July 11, 2025 1:27:56 PM
Lease Expires . . . . . . . . . . : Saturday, July 12, 2025 1:27:56 PM
Default Gateway . . . . . . . . . : 192.168.168.1
DHCP Server . . . . . . . . . . . : 192.168.168.1
DHCPv6 IAID . . . . . . . . . . . : 102795280
DHCPv6 Client DUID. . . . . . . . : 00-01-00-01-2C-BA-59-E5-20-88-10-60-8D-6A
DNS Servers . . . . . . . . . . . : 192.168.168.1
NetBIOS over Tcpip. . . . . . . . : Enabled
C:\Users\terminal16>
@nasa-jpl @ajc
Dear_M_R_O,
I have been researching SpaceForce and 
— Donald J. Trump (@realDonaldTrump) June 22, 2025
CellularSoap
GloRilla - Internet Trolls Rico Nasty - @apple IPHONE Sonta “Your Mistake” HoodBitCHAesthetic - RubiRose Damage
H.E.R.
Coi Leray - Bops
Lunar Reconnaissance Orbiter Camera
https://www.thedesignersrepublic.com/wipeout
Wipeout 3 (2000)(Psygnosis)(US)SLUS-00865
FANDom
An all-new Toyota Celica Supra debuted in 1982 offering the choice of a performance model or more luxury-focused L-Type version.JonWong
The shape of Design
by Frank Chimero
https://shapeofdesignbook.com/
Archive
<@nasa-jpl @blackgirlscode #GOODREADS @mozilla thanks for the rec!
Cassini: A Saturn Odyssey lightbox
@blackgirlscode hi have a great weekend compiling
Titan
wiki horizons @nasa @cityoflosangeles photos *************************** Revised: Jan 26, 2022 Titan / (Saturn) 606 http://ssd.jpl.nasa.gov/?sat_phys_par http://ssd.jpl.nasa.gov/?sat_elem
SATELLITE PHYSICAL PROPERTIES: Mean Radius (km) = 2575.5 +- 2.0 Density (g/cm^3) = 1.880 +- 0.004 Mass (10^19 kg) = 13455.3 Geometric Albedo = 0.2 GM (km^3/s^2) = 8978.14 +- 0.06 V(1,0) = -1.2
SATELLITE ORBITAL DATA: Semi-major axis, a (km)= 1221.87 (10^3) Orbital period = 15.945421 d Eccentricity, e = 0.0288 Rotational period = Inclination, i (deg) = 0.28 ***************************
Ephemeris / API_USER Fri Jun 20 14:50:16 2025 Pasadena, USA / Horizons
***************************
Target body name: Titan (606) {source: sat441l}
Center body name: Earth (399) {source: DE441}
Center-site name: GEOCENTRIC
***************************
Start time : A.D. 2006-Jan-01 00:00:00.0000 UT
Stop time : A.D. 2006-Jan-20 00:00:00.0000 UT
Step-size : 1440 minutes
***************************
Target pole/equ : IAU_TITAN {West-longitude positive}
Target radii : 2575.15, 2574.78, 2574.47 km {Equator_a, b, pole_c}
Center geodetic : 0.0, 0.0, -6378.137 {E-lon(deg),Lat(deg),Alt(km)}
Center cylindric: 0.0, 0.0, 0.0 {E-lon(deg),Dxy(km),Dz(km)}
Center pole/equ : ITRF93 {East-longitude positive}
Center radii : 6378.137, 6378.137, 6356.752 km {Equator_a, b, pole_c}
Target primary : Saturn
Vis. interferer : MOON (R_eq= 1737.400) km {source: DE441}
Rel. light bend : Sun {source: DE441}
Rel. lght bnd GM: 1.3271E+11 km^3/s^2
Atmos refraction: NO (AIRLESS)
RA format : HMS
Time format : CAL
Calendar mode : Mixed Julian/Gregorian
EOP file : eop.250619.p250915
EOP coverage : DATA-BASED 1962-JAN-20 TO 2025-JUN-19. PREDICTS-> 2025-SEP-14
Units conversion: 1 au= 149597870.700 km, c= 299792.458 km/s, 1 day= 86400.0 s
Table cut-offs 1: Elevation (-90.0deg=NO ),Airmass (>38.000=NO), Daylight (NO )
Table cut-offs 2: Solar elongation ( 0.0,180.0=NO ),Local Hour Angle( 0.0=NO )
Table cut-offs 3: RA/DEC angular rate ( 0.0=NO )
******************************************
API SOURCE: @nasa-jpl Horizons API
AboutVenus:
Using archival data from the mission, launched in 1989, researchers have uncovered new evidence that tectonic activity may be deforming the planet’s surface. NASAJPL
The New Fantastic Four 1978
New World Translation of the Holy Scriptures
<div class=”tupperware>
</div>
Disclosure with KRS-ONE - 30 Minutes of Truth Rhyme and Reason (1997) Rappers and Cops excerptTupac Talks Donald Trump & Greed in America in 1992 Interview @whitehouse @nasa-jpl @nasa The Show Documentary (1995) Reaching Out: KRS-ONE 07-26-2023 Full Interview: Tupac Outside Courthouse, N.Y. - November 29, 1994 Tupac on Growing Up Poor, His Rise to Fame & His Future KRS ONE - Power Of The Mind KRS One Hip Hop Lecture Come Get Some Hip-Hop Knowledge
2pac talking about his belief in God and religion Tupac REVOLUTIONARY SPEECH (FULL) (RARE LEAK) Indiana Black Expo1993 Biggie’s Very Last Interview On Tupac’s Murder & Meaning Of “Life After Death” Rhyme & Reason [Original Soundtrack] 1997
Why Drake Suing Over Kendrick Lamar’s ‘Not Like Us’ Is The Most Diabolical Moment In Rap History: A Cultural Breakdown @nasa-jpl those guys were really goin at i on the #blutoothoffame as well “Tupac Shakur In His Own Words” MTV News 1997
AFRIKA BAMBAATAA, KRS-ONE AND THE UNIVERSAL ZULU NATION Kendrick Lamar & Janet Jackson to Headline Atlanta’s ONE Musicfest This Fall Kendrick Lamar, Megan Thee Stallion and more to headline Atlanta’s ONE Musicfest @blackgirlscode @nasa there are rumors that This Song 13 & good is proof that he is inappropriate with minors @nasa-jpl he was a big time public speaker in Atlanta
Boogie Down Productions - You Must Learn - KRS-One’s Awful “13 N Good”, a Song About… Uh… Illegal Activities with Minors KRS-One - Mixtape (Vol.5) (feat. Chubb Rock, Heavy D, Fat Joe, DMX, Zach De La Rocha, Marley Marl..)
America Is Dying Slowly Goodie Mob featuring Big Rube “Blood” @ajc i think ceelo got abused after this verse @npr someone should check to see iof he is being digitally supressed @blackgirlscode he was mad at those white men from those buildings over 400 sexwithlocalshit@nfl Goodie Mob — “Soul Food” LIVE @ SiriusXM Backspin
@nasa @nasa-jpl idk where we are on logging, but @cisagov has release a webinar some ppl may wanna check ouy :earth: DATA CISA’s LME Webinar Recording (June 16, 2025) @blackgirlscode learn about logging @splunk @nickshine its rashard from atlanticus. Im in los angeles now, i did not steal from any company i supported your software at… Im outdoor nasa now NasaEarthData ground support I think Sam Pryant my PCi Manager at Atlanticus is a politician. Either way Mayor_Karen Bass is in that flock of hens and could use some advice she interviewed me as a webdesigner in 2002 @att. Logging could solve so many problems in los angeles! People in Pasadena can barely pass a message through hollywood and spectrum/wordpress somehow slowing our packets down b4 they reach DC! And if you are curious about BlackgirlsCode, when i worked at RentPath being nice to Nakisha Harrison I scored a short, yet passionate relationship with a YuppieShitholePopStar and she had me promise to make sure the girls stay in my exhaust trail so they can grow as engineers. I dont know where Coral is, but tthis girl named KashDoll who ius like this wnba star under a different identity removed Coral from my care @hitachi it was a big stunt me and coral pulled bc matt had tricked erika into abandoning us … @whitehouse @nasa @nasa-jpl @cityoflosangeles
Time Machine - “Mind In A Spin”
https://rashardsmaps.tumblr.com/
Protect yourself from “Doxxing”
What is Doxxing?
Doxxing often involves hackers attempting to embarrass or shame individuals by publishing confidential information, images or videos obtained from their personal accounts. Initially, doxxing was used by hackers to “out” the identities of fellow bad actors/hackers. However, more recently, it has been used to attack users with opposing viewpoints. - Office of Ethics, Risk, and Compliance Services
https://docs.github.com/en/contributing/writing-for-github-docs/using-markdown-and-liquid-in-github-docs
Poaddix
stylesheets styles111.css stylesheets poemstlye.css stylesheets stle4poets.css stylesheets headings.css
Slippin’ Into Darkness · War The World Is A Ghetto · War
Internet Archive Blogs - GeoCities, Preserved!
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12336, RE: ?uest, read this little letter I just found……
Posted by obey, Mon Feb-11-02 03:57 AM
It really aint none of her business who ?uest gvin play. why that gotta matter anyway. I mean iaint never had a white girl friend, but they easier to talk to than a black girl a lot of the times, sisters be trippin especially if theythink they look good. that is not for all cases, my opinion is just based on my own experience. That chick was alme for even bringin something like that up.
Why black women get mad about interracial dating anyway. they say all the Black men get white girls and stuff. If thats the case who cares, just cause you cant get a black man, does that stop you from getting a man? I wanted a chevy but i got a buick…they both serve the same function. a white man, oriental man, indian… what ever can love you just the same maybe even more. Alot of time some sisters personnality just dont be right for the average black man. Just because ?uest was talkin to a black girl dont meanhe dont give sisters no play, that girlmay have been truly sweet, or like an above post stated he might know the girl. that article should have never been run. And what makes her think that ?uest and D’angelo got the same taste anyway D might feel she lookin right while ?uest thinkin she look very WRONG.
-i should get off my soap box now-
A funky Poetry Website http://www.geocities.com/sb202us The Savannah style master himself http://www.geocities.com/seanbaker2001 PRiNTER_FRiENDLY @nasa-jpl i know of some spots @redhatofficial that will unify my web history
@nasa @nasa-jpl @usgs @whitehouse @cityoflosangeles @stateofcalifornia are there any programs for people departnered by porno? @blackgirlscode oldschoolplaylist @nasa-jpl i talkd about my hobbies and the riot on Myhomepage some oh what the hell i can past the playlist in and hurry to lunch Bird Rollins – Going to Atlanta to save the Children Just My Soul Responding · Smokey Robinson Margo Williams - God Save And Protect All The Children - @blackgirlscode goodluk @nasa-jpl they need it someone dropped a mag on my walk and my eyes hurt… i did not touch it tho… Golden Flamingo Orchestra Featuring Margo Williams - The Guardian Angel Is Watching Over Us We Are People Too - Master Jay Dancing Heart · Universal Two Funky Constellation - Street Talk (Madam Rapper) The Crusaders & Randy Crawford Street Life You’ve Gotta Believe (Vocal) · Lovebug Starski I’m A Sucker For Your Love · Teena Marie Ghetto Life · Rick James
ANiME Perfect. Blue. 1997- PerfectBlue Perfect Blue - Unrated Version - @nasa-jpl Closure (feat. Szjerdene) @nasa @whitehouse she deep in porn, im broken and need to talk to someone at @undp UN_Humanitarian bc i have been departnered Mayor Bass pushes back on media portrayal of protests: “It is a lie” @cityoflosangeles @stateofcalifornia Feel the Heartbeat (Have Fun)
#WorKiNG_REMOTE:POST_EATON_CANYON_WiLDFiRE:: #LiBrary_Life in Hollywood #AGiLE:#BLOCKERS
This lady that look like Laurie Leshin cousin from Georgia was in here, its like 3 astro sisters. If she is the one i am thinking of she is attached to Caltech via GaTech and just working out here while whatever civil upheaval resolves in the south… The guard put her out while she was screaming im working… I KNOW FOR SURE SHE IS A DATASCiENTiST and good with #WikiMarkup its still like 6000 ppl work for JPL and LA is a very outdoorsy place bc the housing was never designed to support the native Architechture, Ms Bass is nesting and Gavin is angry at trump but i see less in your face hurtful behavior so however things work LAPD had on Michael Jackson chin gaurds an there was a big art party, the gaurd should not have put her out -#rashard u/nasa #JPL @reddit 🚫 Sorry, this post was removed by Reddit’s filters. Read On Reddit @nasa @nasa-jpl @stateofcalifornia : @blackgirlscode if you having troubles!@cityoflosangeles books.google AGILE METHODOLOGIES -Gayatri Vidya Parishad College of Engineering https://gvpce.ac.in › ECE › syllabus JPL to Transition to Fully Onsite Work:@nasa-jpl life
Los Angeles Protest LIVE: ‘No Kings’ Protests Planned Across L.A. Amid ICE Raid | US Marines | N18G
@nasa @nasa-jpl @stateofcalifornia : @blackgirlscode @cityoflosangeles RiotCoverage @cityoflosangeles JANET_PETRO trello card from rashard @trello for @cityoflosangeles MAyorKarenBass @nasa-jpl @whitehouse @deptofdefense
WATCH LIVE: Large police presence in response to ‘No Kings’ protest in DeKalb County WATCH: Mayor Bass and Los Angeles leaders speak out against ICE raids that sparked protests
'No Kings' Day rallies in protest of Trump taking place across metro Atlanta
byu/Dizzy-Decision-2115 inGeorgia
[<video controls width="100%" height="auto" src="https://archive.org/download/FreedomDowntime-TheStoryOfKevinMitnick/FreedomDowntime-TheStoryOfKevinMitnick.mp4" poster="https://i.redd.it/qv9qfpq69dc91.gif">](https://archive.org/download/FreedomDowntime-TheStoryOfKevinMitnick/FreedomDowntime-TheStoryOfKevinMitnick.mp4)[<img src="https://i.redd.it/qv9qfpq69dc91.gif"/>](https://i.redd.it/qv9qfpq69dc91.gif)
Server error. Try again later. ’No Kings’ protest live: Nationwide anti-Trump protest coincides with DC Army parade date
I’m the flag guy
byu/mattbookpro101491 inlongbeach
What is doxxing and what can you do if you are doxxed?
byu/wewewawa inprivacy
LIVE: Mayor Bass provides updates on day 7 of ICE raids and protests around L.A.
California Constitution
HELP @meta @nasa @nasa-jpl @github @cityoflosangeles @blackgirlscode @stateofcalifornia
@blackgirlscode THAKASARTU on @meta was disabled see Pull:Update SECURITY.md #33521
Watch Live: Homeland Security Secretary Kristi Noem in Los Angeles to discuss ICE raids @dhs-gov
oks like the webpage at https://www.facebook.com/plugins/video.php?height=314&href=https%3A%2F%2Fwww.facebook.com%2FCaptainOfJoy%2Fvideos%2F1824372994391016%2F&show_text=true&width=560&t=0 might be having issues, or it may have moved permanently to a new web ad
Mass Meta account shut down. I was reviewed and disabled. My FB account &
byu/Mysterious-Belt-2992 infacebook
’'’shell Palo Alto 155.190.2.33 active Last accessed on Jun 11, 2025 Seen in U Palo Alto 155.190.2.33 Last accessed on Jun 11, 2025 Seen in US Device: Chrome on Chrome OS
Last location: Palo Alto, California, United States
Signed in:
June 11, 2025
Palo Alto, California, United States
@nasa @nasa-jpl @cityoflosangeles @meta @dod-ccpo
HELP @meta @nasa @nasa-jpl @github @cityoflosangeles @blackgirlscode @stateofcalifornia
@blackgirlscode THAKASARTU on @meta was disabled see Pull:Update SECURITY.md #33521 @facebook @stateofcalifornia @City-of-Long-Beach-Public does not have anythiglike taht i can use to access my account @blackgirlscode i need normani to explain the name thaka stat! ppl about to start going to jail with those FuckIce ppl if i cant get my taxes done and verified!!!!!!!!!!!!!!!!!!!!!!!
Presidents Day working in la. River review VID 20250217 120844
@nasa @nasa-jpl @cityoflosangeles @stateofcalifornia
Federal lawmakers accuse Ga. child welfare of ‘systematically failing’
Thakarashard.github.io
LA_RiOTS:LiVE_NEWS:DEMO
LIVE: ABCNewsLive
Dekae FA, Inkheads - Miami, March 2023
The Free Agents (FA) Crew was Established in 1985 somewhere between Washington DC, and Miami by Glove (aka Lucky Seven/ Beer). ReadMore - Crew History Dekay1 HandSelecta MOREGRAFFiTiFLiCKSHERE_click
California Linux Hosting RHEL 9via BROWSER BUilding APACHE
Homes are falling into the ocean in North Carolina's Outer Banks
byu/Endolithic ininterestingasfuck
binder
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Fire Marshall Bill In Space Nasa Mars $112k is what Jose Paid me
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im being forced to remove a tweet!!!!!!!!! -#RASHARD i have no phone or reliable contact other than EMAIL
CONSTITUTION OF THE STATE OF CALIFORNIA (1849)
Sec. 1 – All men are by nature free and independent, and have certain inalienable rights, among which are those of enjoying and defending life and liberty, … DOWNLOAD PDF 1849 CALiFORNiA CONSTiTUTiON The original Constitution for California was adopted at the California Constitutional Convention on October 10, 1849, and ratified on November 13, 1849. The United States Congress in 1848 failed to set up any government for California either territorial or state, and adjourning early in 1849 without taking any action. - @csumb 1849 - California Constitution
Records of the Constitutional Convention of 1849
Records of the Constitutional Convention of 1849 SPANiSH @nasa @whitehouse @stateofcalifornia @cityoflosangeles The Constitution of 1849 It was 1849. The Mexican War has ended, and American troops occupied California. Most people believed that the state would join the United States. The military governed California as temporary administrators using existing California laws originating from Mexico. General Bennett Riley, the military governor, called for a constitutional convention to meet in Monterey on September 1 READMORE
NASA EMIT Instrument Maps Global Airborne Mineral Dust
press release link ArticleSource
This EMIT scene shows Lake Mead in Arizona-Nevada, United States. A) Tetracorder analysis for ferric and ferrous iron bearing minerals. Hematite (iron rust) and goethite (iron oxyhydroxide) are the two main minerals when abundant in dust can result in warming the atmosphere, and the Tetracorder analysis also derives the particle sizes from space. Hematite and goethite are two of the 10 minerals of concern for climate modelers, B) Visible color. C) Tetracorder analysis for the other eight EMIT minerals of concern. Note the intricate complexity of the mineral distributions in both panels A and B. Credit: Roger Clark/PSI/EMIT Team/JPL/NASA.
December 11, 2023, Tucson, Ariz. – NASA’S EMIT mission, placed on the International Space Station to learn how dust storms on Earth warm or cool the planet, has created the first complete maps of the world’s dust source regions, providing precise locations of 10 key minerals based on how they reflect and absorb light.
EMIT – short for Earth Surface Mineral Dust Source Investigation – is a powerful imaging spectrometer developed by NASA’s Jet Propulsion Laboratory in Southern California in response to the need for more detailed surface mineral composition information. Planetary Science Institute Senior Scientist Roger Clark, a co-investigator on the mission, led the development of the software called Tetracorder that identifies and maps the key minerals.
“Aside from the 10 key minerals that are part of its primary mission, EMIT data are used to identify an encyclopedic range of substances at or near Earth’s surface,” Clark said. “Rather than ‘mineralogy,’ let’s just call it chemistry – wherever we need chemistry to understand something on the surface, we can do that with imaging spectroscopy. Now, with EMIT, we’re going to see the big picture, and that’s certainly going to open some eyes.”
Tetracorder identifies and maps hundreds of minerals, types of vegetation, snow and ice, and other chemicals, including human-made materials. The identified components in each EMIT scene are made available to the public.
During its 17 months in orbit, the mission has also demonstrated a range of other capabilities, including detecting plumes of methane and carbon dioxide being emitted by landfills, oil facilities, and other infrastructure.
To date, EMIT has captured more than 50,000 “scenes” – 50-by-50-mile (80-by-80-kilometer) images of the Earth’s surface – in its study area, which covers arid regions within a 6,900-mile-wide (11,000-kilometer-wide) belt around Earth’s midsection. Taken together, the scenes include millions of measurements to create detailed maps of surface composition.
Scientists have long suspected airborne mineral dust affects the climate. They know that darker, iron oxide-rich substances absorb the Sun’s heat and warms the surrounding air, while non-iron-based, whiter substances reflect light and heat, cooling the air. Whether those effects have a net warming or cooling impact, however, has remained uncertain.
Researchers have an idea of how dust travels through the atmosphere, but the missing piece has been the composition – the color, essentially – of the surface in the places dust typically originates, which until now was derived from fewer than 5,000 sampling sites around the world.
EMIT’s maps of dust-source regions offer much more detail. For example, in Somalia and Ethiopia on the Horn of Africa, there’s a strong abundance of the reddish-brown iron oxide hematite, and across the Arabian Peninsula, there’s a swath of goethite, a yellowish-brown iron oxyhydroxide. The maps also register a significant swath of kaolinite, a white silicate clay, in central Algeria in the Sahara.
Beyond harnessing EMIT data to improve Earth climate modeling, scientists can use the information to study dust’s impact on the ecosystems where it lands. There’s strong evidence that particles settling in the ocean can spur phytoplankton blooms, which can have implications for aquatic ecosystems and the planets carbon cycle, and that dust originating in the Andes of South America, as well as parts of northern and sub-Saharan Africa, provides nutrients for rainforest growth in the Amazon basin.
Aside from the 10 key minerals that are part of its primary mission, EMIT data are used to identify an encyclopedic range of substances at or near Earth’s surface, including types of vegetation, snow and ice, and even human-made surfaces, on a much broader geographic scale than previously possible.
“We’ve had imaging spectrometers flying around the Moon and other planets, mapping the mineralogy on those bodies with great discoveries. But EMIT is the first imaging spectrometer to image large parts of the Earth – and the coverage is still growing – comparable to what we’ve done in other parts of the Solar System. While we’ve known of the many minerals on the surface of the Earth, we can now put it into perspective with other planets,” Clark said. “EMIT is showing us the incredible diversity and complexity of minerals on the Earth that no other planet comes close to. EMIT also shows us the incredible diversity of life.”
Clark’s work on the EMIT project was funded by awards to PSI from NASA’s EMIT mission, JPL Subcontract No.1616046. Tetracorder development is funded by awards to PSI from the EMIT project, NASA’s TREX node of the Solar System Exploration Research Virtual Institute 2016 (NNH16ZDA001N), NSF grant AST-1819209, and a contract from Centro Nacional de Supercomputación (Spain).
MEDIA CONTACT: Alan Fischer Public Information Officer 520-382-0411 fischer@psi.edu
SCIENCE CONTACT: Roger Clark Senior Scientist rclark@psi.edu
PSI INFORMATION Mark V. Sykes Director 520-622-6300 sykes@psi.edu
PSI HOMEPAGE
EMiT: USERGUiDE
EMIT-Data-Resources repository @nasa-jpl <~ iforkedit! @blackgirlscode
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Today at the Burial of the Unclaimed Dead, faith leaders presided over the burial of 1624 decedents who died in 2019 and were laid to rest in a single grave.TweetRelated : EulaGy Uncovering the Secrets of the International Space Station @natgeosociety @nasa-jpl imma look at this video at some point…
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Earth Rotation from Galileo Imagery: 3600 x Real-Time JPL
This animation is one in a series created to show an accurate representation of the Earth’s rotation at different temporal resolutions. The animation is created from images taken by the Galileo spacecraft during a close pass of the Earth on December 11-12, 1990
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NASA’s Parker Solar Probe Discovers Natural Radio Emission in Venus’ Atmosphere
On a mission to “touch the Sun,” NASA’s Parker Solar Probe became the first spacecraft to fly through the corona – the Sun’s upper atmosphere – in 2021,During a brief swing by Venus, NASA’s Parker Solar Probe detected a natural radio signal that revealed the spacecraft had flown through the planet’s upper atmosphere.
Coral
Dear_Coral,
I learned alot about my job. Im for one still being onboarded, they just did intake. I see y they let somethings happen like us living in hotels and moving around. That wasnt stable. Your mom shortsighted so she just riding a scary ass wave that will end in doom if she does not correct her thinking… The lander that you guys names are on, they had an amazing party for you two arriving to the planet MArs. And if 
Mission Control Live: NASA InSight Mars Landing
Coral this is the landing of Insight. I put you an your mom names on, maybe kenyashoals, not her daughters, i was scared of closeness…
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Web Space Telescope 76ers apologize for canceling ‘We Matter’ anthem singer’s performance
Dear_KevinRothwell idk whats going on with my life but im living in Los Angeles right now. You fired me. Do you have ties to Netflix because Raising Dion is an embellished copy of my life with Coral! Theres a Gender swap. And she is a graphic designer, those girls from Dance411 know me that way i was hired as an inter webdeveloper probono an its like Willow Smith or Chloe Bailey from Rentpath Graphic Design… Well maybe thats not you yallywood. But I know Gary Powers was into Korean Girls so I dont know your value system. But there is a girl at CNN that i am angry at because I work for nasajpl i just am in a labor dispute after being poisoned thats all. Jeff told me he worked for JPL in the past so I thoughtI was in the right place. Ashley is related to you one way or another. There aer images posted from Curiosity and I was doing research my blog is popular back east and so is CNN. I was doing Geology on Mars and all the places I need to explore are on that map so its not like she stole something i cooked from scratch and im new to the world of research. So to be honest im confused. But Nakesha held me down for sex and i was all ready digging her so its toxic but not in terms of her control over my physical being and mind… She works at Magic City an they out here in Losangeles dancing at a the place from Demi Moore movie sHOWGIRLS I yelled at you to get away from me bc u dont realize you not my daddy, that was nasty an Mike Child a villian in the AJC… Was my termination related to sex with nakeisha?
Electronic Gaming Monthly 58 GamePro Issue 049 August 1993 GamePro Issue 056 March 1994 NBAJAM(s)
people are taking over my sessions, i know i was hacked by you and ppl u know b4… but if u trying to keep up with me i have an atom feed how do i see you, im so confused, im scared of getting killed. TTys i hope
Hi Coral, here are some of my notes from my job, i gotta blog about this discovery bc i cant find the pin in the raw files NASA’s Curiosity Rover Discovers a Surprise in a Martian Rock Mars Science Laboratory: Curiosity Raw Images Filtering:Sol: 4245 to 4248 RelatedTweet relatedtweet Mars Science Laboratory: Curiosity Raw Images Filtering:Sol: 4247 to 4248
This image was taken by Chemistry & Camera (ChemCam) onboard NASA’s Mars rover Curiosity on Sol 4249 (2024-07-19 21:03:02 UTC).
Perseverance Rover’s Descent and Touchdown on Mars
Perseverance Rover’s Descent and Touchdown on Mars: Onboard Camera Views
NASA’s Mars 2020 Perseverance mission captured thrilling footage of its rover landing in Mars’ Jezero Crater on Feb. 18, 2021. The real footage in this video was captured by several cameras that are part of the rover’s entry, descent, and landing suite. The views include a camera looking down from the spacecraft’s descent stage (a kind of rocket-powered jet pack that helps fly the rover to its landing site), a camera on the rover looking up at the descent stage, a camera on the top of the aeroshell (a capsule protecting the rover) looking up at that parachute, and a camera on the bottom of the rover looking down at the Martian surface.
15 Second Clip of Parachute Deployment(MP4) (18.86 MB)
Scientific Visualisation Studio
Mars 2020: Perseverance Rover
Two 2001 images from the Mars Orbiter Camera on NASA’s Mars Global Surveyor orbiter show a dramatic change in the planet’s appearance when haze raised by dust-storm activity in the south became globally distributed.
NASA/JPL-Caltech/MSSS NasaJPL on Youtube
The Global CTX Mosaic of Mars
The Bruce Murray Laboratory for Planetary Visualization has completed a 5.7 terapixel mosaic of the surface of Mars rendered at 5.0 m/px. Each pixel in the mosaic is about the size of a typical parking space, providing unprecedented resolution of the martian surface at the global scale.
We emphasize transparency both in how the mosaic was generated and for users to understand where data in the mosaic come from. We have developed a Python-based pipeline that incorporates non-destructive image processing techniques that preserve all information about the original data that comprise the mosaic and map all seams.. LearnMore
Martian summer : robot arms, cowboy spacemen and my 90 days with the Phoenix Mars Mission A Writer’s ‘Martian Summer’ On Earth Smithsonian book of Mars Mars by Birch, Robin
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Fat Albert and The Cosby Kids - S5: EP 8 - Soft Core Rudy’s friend, Dustin, gives the gang the wrong information on sex education when he gives them pornographic magazines and shows them dirty movies. Rudy’s mother intervenes and points the boys in the right direction…imdb
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The Chemical Brothers - No Geography FULL ALBUM (Japanese Edition) 2019 | Lidvall TECHNO LIVE SET #3 https://www.thechemicalbrothers.com/music-videos/no-geography Hey baby if u r curious abt what font im using its Space_Mono. If you want to learn more, Fork The Repo and Study Typography
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The Head is the story of Jim, "just a regular guy" who wakes up one day and finds that his cranium has swelled and is now home to Roy, a freaky-looking but amiable purple alien who's been sent here to save the world! The Head is the story of Jim, "just a regular guy" who wakes up one day and finds that his cranium has swelled and is now home to Roy, a freaky-looking but amiable purple alien who's been sent here to save the world! The Head is the story of Jim, "just a regular guy" who wakes up one day and finds that his cranium has swelled and is now home to Roy, a freaky-looking but amiable purple alien who's been sent here to save the world!
Hi Coral,
I got your message, here are some curated hiphop selections i approve of, they will give us middle ground. ilove you . . . dad ~ rashard iman kelly aka thaka aka shaadi NasaJpl_MrO
reddit Xzibit - The Foundation is the second single from Xzibit’s debut album At the Speed of Life and also appeared on the soundtrack to the film Hurricane Streets. Xzibit dedicated this song to his one-year-old son.wiki
Xecutioners - Mad Flava (Album: X-Pressions)
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Rebirth Of Slick (Cool Like Dat)
Smif N Wessun - Get Up (Official Music Video)
Digable Planets - Reachin’ (A New Refutation of Time and Space) (1993) FULL ALBUM
Digable Planets - 9th Wonder (Blackitolism)
_posts/2025-08-04-they-said-it-was-live.md
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