National Environmental Policy Act; Mars 2020 Mission, 55762-55763 [2013-22116]
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Federal Register / Vol. 78, No. 176 / Wednesday, September 11, 2013 / Notices
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Dated: September 5, 2013.
Yoon Ferguson,
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Labor.
[FR Doc. 2013–22125 Filed 9–10–13; 8:45 am]
BILLING CODE 4510–CK–P
NATIONAL AERONAUTICS AND
SPACE ADMINISTRATION
[Notice 13–111]
National Environmental Policy Act;
Mars 2020 Mission
National Aeronautics and
Space Administration (NASA).
ACTION: Notice of intent to prepare an
environmental impact statement (EIS)
for the Mars 2020 mission and to
conduct scoping for the EIS.
AGENCY:
Pursuant to the National
Environmental Policy Act of 1969, as
amended (NEPA) (42 U.S.C. 4321, et
seq.), the Council on Environmental
Quality (CEQ) Regulations for
Implementing the Procedural Provisions
of NEPA (40 CFR parts 1500–1508), and
NASA policy and procedures (14 CFR
part 1216 subpart 1216.3), NASA
intends to conduct scoping and prepare
an environmental impact statement
(EIS) for the Mars 2020 mission. NASA
is seeking input on environmental
issues and concerns associated with the
proposed action, as well as alternatives
that should be addressed in the EIS. The
mission would fly a near-duplicate of
the Mars Science Laboratory mission’s
rover, Curiosity, outfitted with new
scientific instruments. The mission
would be designed to seek signs of past
life on Mars, collect and store a
compelling set of soil and rock samples
that could be returned to Earth in the
future, and test new technology to
benefit future robotic and human
exploration of Mars.
The Proposed Action is to continue
preparation for and implement the Mars
2020 mission. The Mars 2020 mission
would launch the spacecraft from the
emcdonald on DSK67QTVN1PROD with NOTICES
SUMMARY:
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Cape Canaveral Air Force Station
(CCAFS), Brevard County, Florida
during the summer of 2020. NASA
would select the launch vehicle for the
mission through NASA’s launch
services procurement process. There is
a backup launch opportunity for the
mission during the summer of 2022. The
baseline mission plan would include
the use of one multi-mission
radioisotope thermoelectric generator
(MMRTG) for rover electrical power and
temperature control while on the
surface of Mars. Some science
instruments may require the use of
small quantities of radioactive material
for instrument calibration or for
experimentation. Environmental
impacts to be considered in the EIS are
those impacts associated with a normal
launch from CCAFS, and radiological
and non-radiological risks associated
with a potential launch accident.
DATES: Interested parties are invited to
submit comments on environmental
concerns in writing on or before October
30, 2013 to assure full consideration
during the scoping process. NASA will
conduct scoping meetings to solicit and
collect comments on the scope of the
Mars 2020 mission EIS as well as the
Proposed Action in October 2013.
ADDRESSES: Written comments should
be addressed to Mr. George Tahu,
Planetary Science Division, Science
Mission Directorate, Mail Suite 3E46,
NASA Headquarters, Washington, DC
20546–0001. Comments by electronic
mail may be sent to mars2020nepa@lists.nasa.gov. Those persons
requesting to receive a hard copy of the
Mars 2020 Draft EIS should also provide
a valid US Postal Service mailing
address.
Mr.
George Tahu, by telephone at 202–358–
0016 or by electronic mail at mars2020nepa@lists.nasa.gov.
Additional information is available at
https://www.nasa.gov/agency/nepa/
mars2020eis.
FOR FURTHER INFORMATION CONTACT:
NASA
seeks to continue scientific
investigations of Mars with a long-term
landed mission to explore the planet’s
surface. On April 12, 2005, in the
Federal Register (70 FR 19102), NASA
published the Notice of Availability for
Final Programmatic EIS (PEIS) for the
Mars Exploration Program (MEP). The
Record of Decision (ROD) for the MEP
PEIS was signed on June 22, 2005,
enabling continued planning for the
MEP, which represents NASA’s overall
plans for the robotic exploration of Mars
through 2020. The PEIS for the MEP
encompasses the launch of at least one
SUPPLEMENTARY INFORMATION:
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spacecraft to Mars during each favorable
launch opportunity, which occurs
approximately every 26 months. The
Mars 2020 EIS will focus on reasonable
alternatives to implement the purpose
and need of the Mars 2020 mission and
the potential environmental impacts
associated with each.
NASA’s proposed Mars 2020 mission
would use the proven design and
technology developed for the Mars
Science Laboratory mission and rover
(Curiosity) that arrived at Mars in
August 2012. NASA would select a high
priority, scientifically important landing
site based upon data from past and
current missions.
The rover would be equipped with
new scientific instrumentation that
would: (a) Characterize the geological
processes and history of an
astrobiologically relevant ancient
environment on Mars; (b) within the
selected geological environment, assess
the past habitability of the landing
region and search for evidence of past
life; (c) assemble a scientifically
selected, well-documented, cache of
samples for potential future return to
the Earth; (d) further the preparation for
future human exploration of Mars; and
(e) demonstrate improved technical
capabilities for landing and operating on
the surface of Mars to benefit future
Mars missions.
It is anticipated that the electrical,
thermal and operational requirements of
the rover would require a radioisotope
power source (MMRTG) using
plutonium-238. This single MMRTG
would provide adequate power to
operate the rover, similar to the Mars
Curiosity rover. Some of the waste heat
from the MMRTG would be used for
temperature control of the rover
electronics, science instruments, and
other sensitive components.
Alternatives to the Proposed Action
addressed in this EIS will include, but
are not necessarily limited to, (1) the use
of alternative sources of on-board power
and heat (including solar energy); and
(2) the No Action Alternative. The Mars
2020 EIS will address the purpose and
need for the proposed Mars 2020
mission and the environmental impacts
associated with its implementation. The
environmental impacts of this mission
are anticipated to be those associated
with the normal launch of the mission.
Potential consequences of accident
situations will also be addressed.
Environmental issues to be addressed
will include, but not necessarily be
limited to, air quality, water quality,
flora and fauna, and potential
radiological effects.
NASA plans to hold two scoping
meetings to receive comments on the
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Federal Register / Vol. 78, No. 176 / Wednesday, September 11, 2013 / Notices
DEIS regarding alternatives and
environmental issues to be considered
in the Draft EIS. The scoping meetings
are scheduled as follows:
1. Cocoa Beach, FL, Wednesday,
October 9, 2013 from 6:00–8:30
p.m. at Cocoa Beach Country Club,
5000 Tom Warriner Boulevard,
Cocoa Beach, FL 32931.
2. Viera, FL, Thursday, October 10, 2013
from 6:00–8:30 p.m. at Brevard
County Government Center, 2725
Judge Fran Jamieson Way, Viera, FL
32940.
Written public input and comments
on alternatives and potential
environmental impacts and concerns
associated with the proposed Mars 2020
mission are hereby requested.
Calvin Williams,
Director, Integrated Asset Management
Division, Office Strategic Infrastructure.
[FR Doc. 2013–22116 Filed 9–10–13; 8:45 am]
BILLING CODE 7510–13–P
NATIONAL AERONAUTICS AND
SPACE ADMINISTRATION
[Notice 13–112]
National Environmental Policy Act;
Santa Susana Field Laboratory
National Aeronautics and
Space Administration (NASA).
ACTION: Notice of Extension of the
Comment Period for the Draft
Environmental Impact Statement (DEIS)
for Demolition and Environmental
Cleanup Activities for the NASAadministered portion of the Santa
Susana Field Laboratory (SSFL),
Ventura County, California.
AGENCY:
A Notice of Availability
(NOA) for the DEIS for Demolition and
Cleanup Activities for the NASAadministered portion of the Santa
Susana Field Laboratory was published
in the Federal Register by the U.S.
Environmental Protection Agency (EPA)
on August 2, 2013, Vol. 78, No. 149,
page 46940.
NASA also published an NOA of the
DEIS in the Federal Register on the
same day (August 2, 2013, Vol. 78, No.
149, pages 47007–47009). The comment
period for the DEIS was to end on
September 16, 2013. This notice extends
the comment period an additional
fifteen days to October 1, 2013, to allow
the public further time to comment on
the DEIS.
DATES: Interested parties are invited to
submit comments on environmental
issues and concerns, preferably in
writing by October 1, 2013.
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SUMMARY:
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Comments submitted by
mail should be addressed to Allen
Elliott, SSFL Project Director, NASA
MSFC AS01, Building 4494, Huntsville,
AL 35812. Comments may be submitted
via email to msfc-ssfl-eis@
mail.nasa.gov.
The DEIS may be reviewed at the
following locations:
1. Simi Valley Library, 2969 Tapo
Canyon Road, Simi Valley, CA
93063, Web site: https://
simivalleylibrary.org/home/, Phone:
(805) 526–1735
2. Platt Library, 23600 Victory Blvd.,
Woodland Hills, CA 91367, Web
site: https://www.lapl.org/branches/
platt, Phone: (818) 340–9386
3. California State University,
Northridge Oviatt Library, 18111
Nordhoff Street, 2nd Floor, Room
265, Northridge, CA 91330, Web
site: https://library.csun.edu, Phone:
(818) 677–2285
4. Department of Toxic Substances
Control, 9211 Oakdale Avenue,
Chatsworth, CA 91311, Web site:
https://www.dtsc.ca.gov, Phone:
(818) 717–6521
The DEIS is available on the internet
in Adobe® portable document format at
https://www.nasa.gov/agency/nepa/
news/SSFL.html.
The Federal Register Notice of Intent
to prepare the DEIS, issued in the
Federal Register on July 6, 2011, is also
available on the Internet at https://
ssfl.msfc.nasa.gov/public-involvement/.
FOR FURTHER INFORMATION CONTACT:
Allen Elliott, SSFL Project Director, by
phone at (256) 544–0662 or by email at
msfc-ssfl-eis@mail.nasa.gov. Additional
information about NASA’s SSFL site,
the proposed demolition and cleanup
activities, and the associated EIS
planning process and documentation (as
available) may be found on the Internet
at https://ssfl.msfc.nasa.gov.
SUPPLEMENTARY INFORMATION:
ADDRESSES:
Decision To Be Made
This DEIS informs NASA decision
makers, regulating agencies, and the
public of the potential environmental
consequences of the proposed
demolition of SSFL buildings and
structures and the proposed
technologies for groundwater and soil
remediation, as implemented through
the Proposed Action. This DEIS
analyzes a range of remedial
technologies that might be implemented
to achieve the proposed groundwater
and soil remediation goals. NASA will
use the DEIS analysis to consider the
potential environmental, economic, and
social impacts from the Proposed
Action. On the basis of the DEIS
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55763
findings, NASA will issue a Record of
Decision (ROD) documenting the
findings. The ROD will further identify
which buildings will be demolished to
support disposition of the property, and
which remedial technology(ies) would
will be applied to meet the soil cleanup
and groundwater quality goals.
The purpose of this notice is to
apprise interested agencies,
organizations, tribal governments, and
individuals of the availability of the
DEIS and to invite comments on the
document. NASA will hold public
meetings as part of the DEIS review
process.
Site Description
The SSFL site is 2,850 acres located
in Ventura County, California,
approximately seven miles northwest of
Canoga Park and approximately 30
miles northwest of downtown Los
Angeles. SSFL is composed of four areas
known as Areas I, II, III, and IV and two
unnumbered areas known as the
‘‘undeveloped land.’’ NASA administers
41.7 acres within Area I and all 409.5
acres of Area II. The Boeing Company
manages the remaining 2,398.8 acres
within Areas I, III, and IV, and the two
undeveloped areas.
Since the mid-1950s, when the two
federally owned areas were owned by
the U.S. Air Force, this site has been
used for developing and testing rocket
engines. Four test stand complexes were
constructed in Area II between 1954 and
1957 named Alfa, Bravo, Coca, and
Delta. Area II and the LOX Plant portion
of Area I were acquired by NASA from
the U.S. Air Force in the 1970s. These
test stands and related ancillary
structures have been found to have
historical significance based on the
historic importance of the engine testing
and the engineering and design of the
structures.
The NASA-administered areas of
SSFL also contain cultural resources not
related to rocket development. SSFL is
located near the crest of the Simi Hills
that are part of the Santa Monica
Mountains running east-west across
Southern California. The diverse terrain
consists of ridges, canyons, and
sandstone rock outcrops. The region
was occupied by Native Americans from
the earliest Chumash, Tongva, and
Tataviam cultures. NASA has
conducted several previous surveys to
locate archaeological and architectural
resources within its portion of the SSFL.
As a result, NASA has identified one
historic property, the Burro Flats
Painted Cave, that is listed on the
National Register of Historic Places
(NRHP), as well as multiple buildings
and structures that are either
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Agencies
[Federal Register Volume 78, Number 176 (Wednesday, September 11, 2013)]
[Notices]
[Pages 55762-55763]
From the Federal Register Online via the Government Printing Office [www.gpo.gov]
[FR Doc No: 2013-22116]
=======================================================================
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NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
[Notice 13-111]
National Environmental Policy Act; Mars 2020 Mission
AGENCY: National Aeronautics and Space Administration (NASA).
ACTION: Notice of intent to prepare an environmental impact statement
(EIS) for the Mars 2020 mission and to conduct scoping for the EIS.
-----------------------------------------------------------------------
SUMMARY: Pursuant to the National Environmental Policy Act of 1969, as
amended (NEPA) (42 U.S.C. 4321, et seq.), the Council on Environmental
Quality (CEQ) Regulations for Implementing the Procedural Provisions of
NEPA (40 CFR parts 1500-1508), and NASA policy and procedures (14 CFR
part 1216 subpart 1216.3), NASA intends to conduct scoping and prepare
an environmental impact statement (EIS) for the Mars 2020 mission. NASA
is seeking input on environmental issues and concerns associated with
the proposed action, as well as alternatives that should be addressed
in the EIS. The mission would fly a near-duplicate of the Mars Science
Laboratory mission's rover, Curiosity, outfitted with new scientific
instruments. The mission would be designed to seek signs of past life
on Mars, collect and store a compelling set of soil and rock samples
that could be returned to Earth in the future, and test new technology
to benefit future robotic and human exploration of Mars.
The Proposed Action is to continue preparation for and implement
the Mars 2020 mission. The Mars 2020 mission would launch the
spacecraft from the Cape Canaveral Air Force Station (CCAFS), Brevard
County, Florida during the summer of 2020. NASA would select the launch
vehicle for the mission through NASA's launch services procurement
process. There is a backup launch opportunity for the mission during
the summer of 2022. The baseline mission plan would include the use of
one multi-mission radioisotope thermoelectric generator (MMRTG) for
rover electrical power and temperature control while on the surface of
Mars. Some science instruments may require the use of small quantities
of radioactive material for instrument calibration or for
experimentation. Environmental impacts to be considered in the EIS are
those impacts associated with a normal launch from CCAFS, and
radiological and non-radiological risks associated with a potential
launch accident.
DATES: Interested parties are invited to submit comments on
environmental concerns in writing on or before October 30, 2013 to
assure full consideration during the scoping process. NASA will conduct
scoping meetings to solicit and collect comments on the scope of the
Mars 2020 mission EIS as well as the Proposed Action in October 2013.
ADDRESSES: Written comments should be addressed to Mr. George Tahu,
Planetary Science Division, Science Mission Directorate, Mail Suite
3E46, NASA Headquarters, Washington, DC 20546-0001. Comments by
electronic mail may be sent to mars2020-nepa@lists.nasa.gov. Those
persons requesting to receive a hard copy of the Mars 2020 Draft EIS
should also provide a valid US Postal Service mailing address.
FOR FURTHER INFORMATION CONTACT: Mr. George Tahu, by telephone at 202-
358-0016 or by electronic mail at mars2020-nepa@lists.nasa.gov.
Additional information is available at https://www.nasa.gov/agency/nepa/mars2020eis.
SUPPLEMENTARY INFORMATION: NASA seeks to continue scientific
investigations of Mars with a long-term landed mission to explore the
planet's surface. On April 12, 2005, in the Federal Register (70 FR
19102), NASA published the Notice of Availability for Final
Programmatic EIS (PEIS) for the Mars Exploration Program (MEP). The
Record of Decision (ROD) for the MEP PEIS was signed on June 22, 2005,
enabling continued planning for the MEP, which represents NASA's
overall plans for the robotic exploration of Mars through 2020. The
PEIS for the MEP encompasses the launch of at least one spacecraft to
Mars during each favorable launch opportunity, which occurs
approximately every 26 months. The Mars 2020 EIS will focus on
reasonable alternatives to implement the purpose and need of the Mars
2020 mission and the potential environmental impacts associated with
each.
NASA's proposed Mars 2020 mission would use the proven design and
technology developed for the Mars Science Laboratory mission and rover
(Curiosity) that arrived at Mars in August 2012. NASA would select a
high priority, scientifically important landing site based upon data
from past and current missions.
The rover would be equipped with new scientific instrumentation
that would: (a) Characterize the geological processes and history of an
astrobiologically relevant ancient environment on Mars; (b) within the
selected geological environment, assess the past habitability of the
landing region and search for evidence of past life; (c) assemble a
scientifically selected, well-documented, cache of samples for
potential future return to the Earth; (d) further the preparation for
future human exploration of Mars; and (e) demonstrate improved
technical capabilities for landing and operating on the surface of Mars
to benefit future Mars missions.
It is anticipated that the electrical, thermal and operational
requirements of the rover would require a radioisotope power source
(MMRTG) using plutonium-238. This single MMRTG would provide adequate
power to operate the rover, similar to the Mars Curiosity rover. Some
of the waste heat from the MMRTG would be used for temperature control
of the rover electronics, science instruments, and other sensitive
components. Alternatives to the Proposed Action addressed in this EIS
will include, but are not necessarily limited to, (1) the use of
alternative sources of on-board power and heat (including solar
energy); and (2) the No Action Alternative. The Mars 2020 EIS will
address the purpose and need for the proposed Mars 2020 mission and the
environmental impacts associated with its implementation. The
environmental impacts of this mission are anticipated to be those
associated with the normal launch of the mission. Potential
consequences of accident situations will also be addressed.
Environmental issues to be addressed will include, but not necessarily
be limited to, air quality, water quality, flora and fauna, and
potential radiological effects.
NASA plans to hold two scoping meetings to receive comments on the
[[Page 55763]]
DEIS regarding alternatives and environmental issues to be considered
in the Draft EIS. The scoping meetings are scheduled as follows:
1. Cocoa Beach, FL, Wednesday, October 9, 2013 from 6:00-8:30 p.m. at
Cocoa Beach Country Club, 5000 Tom Warriner Boulevard, Cocoa Beach, FL
32931.
2. Viera, FL, Thursday, October 10, 2013 from 6:00-8:30 p.m. at Brevard
County Government Center, 2725 Judge Fran Jamieson Way, Viera, FL
32940.
Written public input and comments on alternatives and potential
environmental impacts and concerns associated with the proposed Mars
2020 mission are hereby requested.
Calvin Williams,
Director, Integrated Asset Management Division, Office Strategic
Infrastructure.
[FR Doc. 2013-22116 Filed 9-10-13; 8:45 am]
BILLING CODE 7510-13-P