Status Report

National Environmental Policy Act; Outrigger Telescopes Project

By SpaceRef Editor
December 30, 2003
Filed under , ,

[Federal Register: December 30, 2003 (Volume 68, Number 249)]
[Notices]
[Page 75285-75286]
From the Federal Register Online via GPO Access [wais.access.gpo.gov]
[DOCID:fr30de03-121]

NATIONAL AERONAUTICS AND SPACE ADMINISTRATION

[Notice 03-155]

National Environmental Policy Act; Outrigger Telescopes Project

AGENCY: National Aeronautics and Space Administration (NASA).

ACTION: Notice of intent to prepare an environmental impact statement
(EIS) and conduct scoping for the Outrigger Telescopes Project.

SUMMARY: Pursuant to the National Environmental Policy Act of 1969
(NEPA), as amended (42 U.S.C. 4231 et seq.), the Council on
Environmental Quality 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 prepare
an EIS for the proposed Outrigger Telescopes Project (OTP). The EIS
will address environmental issues associated with the on-site
construction, installation, and operation of four to six 1.8-meter (72-
inch) Outrigger Telescopes. NASA proposes to fund the OTP at the W.M.
Keck Observatory (WMKO) site within the Astronomy Precinct of the Mauna
Kea Science Reserve on the Island of Hawaii, State of Hawaii.

DATES: Interested parties are invited to submit comments on or before
February 16, 2004, to assure full consideration during the scoping
process.

ADDRESSES: Comments should be addressed to Dr. Carl B. Pilcher, Office
of Space Science, Code SZ; NASA Headquarters; 300 E Street, SW.,
Washington, DC 20546-0001. In addition, electronic comments may be sent
to Dr. Carl B. Pilcher at otpeis@nasa.gov or by hardcopy facsimile at
202-358-3096.

FOR FURTHER INFORMATION CONTACT: Dr. Carl B. Pilcher, at telephone 877-
283-1977 (toll-free), electronically at otpeis@nasa.gov, or by hardcopy
facsimile at 202-358-3096.

SUPPLEMENTARY INFORMATION: The OTP is a key element in NASA’s Origins
Program. The Origins Program addresses two fundamental questions: (1)
How do galaxies, stars, and planets form? (i.e., “Where do we come
from?”); and (2) Are there planets, aside from ours, that have the
conditions necessary to support life? (i.e., “Are we alone?”). The
OTP has four scientific objectives that contribute to achieving the
goals of the Origins Program:

  • Detect the “wobble” of stars due to the gravity of unseen orbiting planetary companions as small as Uranus.
  • Make images of disks of gas and dust surrounding young stars and stars that are still forming.
  • Make high-resolution images of faint objects outside our galaxy.
  • Make high-resolution images of objects within our solar system, including asteroids, comets, and outer planets.

The first of these four objectives can be accomplished with the
Outrigger Telescopes alone linked together as an interferometer. (An
interferometer combines the light from two or more separate telescopes
so that they act like one big telescope.) The last three objectives
require that the Outrigger Telescopes be linked as an interferometer to
at least one 8-meter or larger telescope.

NASA proposes to fund the OTP at the W.M. Keck Observatory (WMKO)
site located within the Astronomy Precinct of the Mauna Kea Science
Reserve on the Island of Hawaii. WMKO is the site of the two largest
optical telescopes in the world–the twin 10-meter Keck I and Keck II.
The OTP, if fully implemented as proposed, would consist of up to six
1.8-meter (72-inch) telescopes placed strategically around the two
existing Keck Telescopes.

The California Association for Research in Astronomy (CARA), a non-
profit corporation established by the University of California and
California Institute of Technology (Caltech), operates and maintains
the WMKO. The approximately 2-hectare (5-acre) WMKO site is subleased
to Caltech by the University of Hawaii (UH). The WMKO site is located
within the Astronomy Precinct (approximately 212 hectares (525 acres))
of the Mauna Kea Science Reserve. The 4,500 hectare (11,000 acre)
Science Reserve, is leased to UH by the State of Hawaii.

Because of present funding constraints, only four Outrigger
Telescopes would initially be installed and operated, although the
foundations for six would be constructed. It is anticipated that the
on-site construction and installation of four of the six Outrigger
Telescopes, along with on-site construction of the underground
structures for Telescopes 5 and 6, would begin early in 2005, with
initial operations anticipated in 2006. If funding were available, NASA
would intend to complete the on-site construction, installation, and
operation of Telescopes 5 and 6, with on-site construction and
installation likely to begin no earlier than 2006.

In addition to the WMKO site, alternative sites with at least one
existing 8-meter or larger telescope will be considered in the EIS. If
NASA decides not to or cannot implement the OTP at the WMKO site or a
reasonable alternative site with an existing 8-meter or larger optical
telescope, NASA would consider sites where at least the one objective
that does not require such a large telescope (i.e.,) the survey of
stars for “wobble” due to the gravity of unseen orbiting planetary
companions as small as Uranus) can be achieved. Alternative sites to be
considered in the EIS under such a materially reduced science OTP
option will include, but not necessarily be limited to, the Mt. Wilson
Observatory in Los Angeles County, California, and the Navy Prototype
Optical Interferometer (NPOI) site near Flagstaff, Arizona. The No
Action alternative will also be addressed.

The EIS will analyze the potential environmental impacts associated
with the on-site construction, installation, and operation of the
Outrigger Telescopes at the WMKO site and other reasonable alternative
sites. The potential environmental impacts at alternative sites for the
materially reduced science OTP option will also be evaluated.
Environmental issues to be emphasized will include, but not necessarily
be limited to, cultural resources, flora and fauna, sewage, and
cumulative impacts.

Because it is evident that there is substantial environmental
controversy and concern about locating the Outrigger Telescopes on
Mauna Kea, public scoping meetings will be held in the State of Hawaii
on the following dates:

(a) January 5, 2004, King Kamehameha Beach Hotel; 75-5660 Palani
Road, Kailua-Kona, Hawaii 96740 (paid parking at the hotel will be free
for attendees);

(b) January 7, 2004, Hawaii Naniloa; 93 Banyan Drive, Hilo, Hawaii
96720 (parking is free);

(c) January 8, 2004, Waimea YMCA; 67-1435 Mamalahoa Hwy., Kamuela,
Hawaii 96743 (parking is free);

(d) January 12, 2004, Japanese Cultural Center; 2554 South
Beretania Street, Honolulu, Hawaii 96826 (paid parking at the Cultural
Center will be free for attendees);

(e) January 13, 2004, Wai-Anae District Park; 85-601 Farrington
Highway, Wai-anae, Hawaii 96792 (parking is free).

All of the meetings will begin with an informal open house from
5:15 to 6:15 p.m. The formal meetings to listen to public comments and
concerns will begin at 6:30 p.m. NASA is planning to have a Hawaiian
language translator at all of the meetings.

NASA will also consider conducting public scoping meetings near
reasonable alternative sites in the United States as Wilson and NPOI
sites, if there is sufficient public environmental interest and
concern.

Written public input and comments on alternatives and environmental
issues and concerns associated with the OTP are hereby requested.

Olga M. Dominguez,
Deputy Assistant Administrator for Management Systems.
[FR Doc. 03-32048 Filed 12-29-03; 8:45 am]

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SpaceRef staff editor.