prepublication copy - The Department of Astronomy & Astrophysics ...

More documents

Recommendations

Info

FIGURE 7.3 WFIRST is an infrared telescope with a three‐mirror design. It will have HgCdTe detectors with 144 megapixels in total and angular resolution of 200 milliarcseconds. The sensitivity should be about 200 nJy or 26 th magnitude, enabling shape measurements and photometric redshifts to a depth of 100,000 galaxies per square degree over half the sky. Spectroscopy will be achieved with a grism or prism and will rely mainly on measurement of H alpha out to a redshift of about 1.8 Credit: JDEM Project, NASA‐GSFC. the mission, but firmly believes it should not drive the mission hardware design or implementation cost. NASA should consider creative ways to enable the most flexible possible general investigator program consistent with the current spacecraft and instrument suite. WFIRST employs the JDEM-Omega design, conceived and developed in a collaboration between DOE and NASA. Other versions of a JDEM mission have been endorsed in two previous NRC reports. 14 Much progress has been made in defining the scientific objectives, and a variety of mission concepts have been discussed and compared. This continuing interagency collaboration on the proposed WFIRST is important both scientifically and technically. In addition, the committee is aware that plans are now underway in Europe for a similar mission, Euclid, which has many of the same scientific goals as WFIRST. Euclid is also in its definition phase and is competing with PLATO and Solar Probe for one of the two M-class launch slots of the European Space Agency’s (ESA’s) Cosmic Vision program, now scheduled for 2017 and 2018. There have been discussions between the U.S. agencies and ESA about mounting a joint mission, which could be a positive development if it leads to timely execution of a program that fully supports all of the key science goals of WFIRST (planet microlensing, dark energy science, general investigations) and leads to savings overall. It is expected that the United States will play a leading role in this top-priority mission. WFIRST addresses fundamental and pressing scientific questions and contributes to a broad range of astrophysics. It complements the proposed ground-based program in two key science areas: dark energy science and the study of exoplanets. It is an integral part of coordinated and synergistic programs in fields in which the United States has the leading role. It also presents opportunities for interagency and perhaps international collaboration that will tap complementary experience and skills. It also presents relatively low technical and cost risk, making it feasible to complete within the decade, even in a constrained budgetary environment. For these reasons it is the top-priority recommendation for a spacebased initiative. A 2013 new start should enable launch in 2020. 14 National Research Council, Connecting Quarks with the Cosmos (2003) and NASA's Beyond Einstein Program: An Architecture for Implementation (2007), The National Academies Press, Washington, D.C. PREPUBLICATION COPY—SUBJECT TO FURTHER EDITORIAL CORRECTION 7-18
FIGURE 7.4 Science accomplishments from competitively selected astrophysics Explorer SMEX and MIDEX missions over the last decade (missions launched since 2000). In addition the Explorer program supported a Mission‐of‐ Opportunity contribution to Suzaku and will launch two new SMEX X‐ray missions, NuSTAR and GEMs, in 2012 and 2014, respectively. A MoO contribution of an X‐ray spectrometer to the Japanese Astro‐H is planned for 2014. Upper left: Credit: NASA / WMAP Science Team, Upper right left: Credit: Spectrum and NASA E/PO, Sonoma State University, Aurore Simonnet, Upper right right: Credit: NASA E/PO, Sonoma State University, Aurore Simonnet, Lower left right: Credit: NASA/JPL‐Caltech/WISE Team, Lower left left: Credit: NASA/JPL‐Caltech, Lower right: Credit: NASA/JPL‐Caltech Priority 2 (Large, Space). Explorer Program The Explorer program’s small and medium-size missions, developed and launched on few-year timescales, enable rapid response to new discoveries and provide platforms for targeted investigations essential to the breadth of NASA’s astrophysics program. From the WMAP mid-scale Explorer’s (MIDEX’s) measurements of the age and content of the universe accomplished through its mapping of the cosmic microwave background (see Figures 2.4, 2.5 in Chapter 2), to the small-scale Explorer (SMEX) GALEX’s contributions to understanding of the evolution of galaxies, Explorers are on the forefront of scientific discovery (Figure 7.4). With multiple missions launched per decade for a cost substantially less than that of a single flagship mission, the Explorer program is unique in the world for its versatility and scientific return for the investment. The Explorer program also offers highly leveraged missions of opportunity (MoOs), which enable U.S. scientists to make scientific and hardware contributions to non- NASA missions, and which provide a mechanism to develop large suborbital experiments. PREPUBLICATION COPY—SUBJECT TO FURTHER EDITORIAL CORRECTION 7-19
Page 1:
PREPUBLICATION COPY
Page 4 and 5:
THE NATIONAL ACADEMIES PRESS 500 Fi
Page 7 and 8:
COMMITTEE FOR A DECADAL SURVEY OF A
Page 9 and 10:
Panel on Stars and Stellar Evolutio
Page 11 and 12:
DOUGLAS FINKBEINER, Harvard Univers
Page 13:
SPACE STUDIES BOARD CHARLES F. KENN
Page 16 and 17:
activities 2 that have emerged from
Page 18 and 19:
In addition to the 27 panel meeting
Page 20 and 21:
Acknowledgment of Reviewers This re
Page 22 and 23:
The Accelerating Universe 2-26 The
Page 24 and 25:
APPENDIXES A Summary of Science Fro
Page 26 and 27:
light up the universe, marking the
Page 28 and 29:
RECOMMENDED PROGRAM Maintaining a b
Page 30 and 31:
TABLE ES.4 Space: Recommended Activ
Page 32 and 33:
Cosmic Dawn: Searching for the Firs
Page 34 and 35:
this imprint would both probe funda
Page 36 and 37:
important outcome will be to open u
Page 38 and 39:
estimated to be on the order of $20
Page 40 and 41:
observatories. For NASA an annual b
Page 42 and 43:
surveys of large fields, enabling s
Page 44 and 45:
RECOMMENDATION: U.S. investors in a
Page 46 and 47:
departments and the community as a
Page 48 and 49:
dominate spending; (2) private-publ
Page 50 and 51:
us was certainly evident during the
Page 52 and 53:
BOX 2-1 Other Worlds Around Other S
Page 54 and 55:
FIGURE 2‐2 The source 3C 75, show
Page 56 and 57:
FIGURE 2‐3 Numerical simulation o
Page 58 and 59:
FIGURE 2‐4 Left panel: Image of t
Page 60 and 61:
FIGURE 2‐6 Top: Schematic of the
Page 62 and 63:
Most stars with masses smaller than
Page 64 and 65:
BOX 2-2 The Origin of Planets After
Page 66 and 67:
send material raining into the cent
Page 68 and 69:
BOX 2-4 Lifecycles in Galaxies One
Page 70 and 71:
Stars Stars are the most observable
Page 72 and 73:
ubiquitous high-energy charged-part
Page 74 and 75:
The Nature of Inflation As describe
Page 76 and 77:
FIGURE 2‐11 Pie chart showing the
Page 78 and 79:
An important clue to the nature of
Page 80 and 81:
Studying the properties of neutron
Page 82 and 83:
FIGURE 2‐14 A possible pathway is
Page 84 and 85:
partners and makes recommendations
Page 86 and 87:
As astronomy research has blossomed
Page 88 and 89:
are increasingly relevant. The Euro
Page 90 and 91:
TABLE 3-1 Currently Operating OIR F
Page 92 and 93:
29% 1990 44% US Priv US Fed Other E
Page 94 and 95:
CONCLUSION: Complex and high-cost f
Page 96 and 97:
Space Observatories The Laser Inter
Page 98 and 99:
Physics Division (PHY); the Mathema
Page 101 and 102:
4 Astronomy in Society Astronomy of
Page 103 and 104:
FIGURE 4‐2 The dust sculptures of
Page 105 and 106:
FIGURE 4‐5 President Obama takes
Page 107 and 108:
Astronomy Inspires in the Classroom
Page 109 and 110:
teaching the scientific method. The
Page 111 and 112:
where the fraction of astronomers h
Page 113 and 114:
Percentage of AAS Membership by Fie
Page 115 and 116:
0.4 0.3 0.2 0.1 PL SO IM AG SF IN S
Page 117 and 118:
FIGURE 4‐12 Number (top panel) an
Page 119 and 120:
Professional training needs to acco
Page 121:
assistant and associate professor p
Page 124 and 125:
fluctuating level of funding for as
Page 126 and 127:
THEORY Emerging Trends in Theoretic
Page 128 and 129: Central to the Galaxies across Cosm
Page 130 and 131: TABLE 5‐2 Support for astrophysic
Page 132 and 133: would normally be for a five-year p
Page 134 and 135: FIGURE 5‐7 Highly cited HST publi
Page 136 and 137: y optical and radio astronomers are
Page 138 and 139: FIGURE 5‐8 Number of PhDs per yea
Page 140 and 141: ated by the Program Prioritization
Page 142 and 143: nulling interferometry. The appropr
Page 144 and 145: FIGURE 5‐9 The richness of the su
Page 146 and 147: RECOMMENDATION: NASA and NSF suppor
Page 148 and 149: FIGURE 6‐1. All sky map as observ
Page 150 and 151: FIGURE 6‐3 NASA mission cost over
Page 152 and 153: FIGURE 6‐5 Gemini North with Sout
Page 154 and 155: TOWARD FUTURE PROJECTS, MISSIONS, A
Page 156 and 157: 3. Investment in new and upgraded i
Page 158 and 159: etween several competing elements i
Page 161 and 162: 7 Realizing the Opportunities The p
Page 163 and 164: FIGURE 7.1 Survey time line showing
Page 165 and 166: SCIENCE OBJECTIVES FOR THE DECADE T
Page 167 and 168: Box 7.1 Implementing a Cosmic Dawn
Page 169 and 170: JWST, with its superb mid-infrared
Page 171 and 172: optical imaging of brighter galaxie
Page 173 and 174: Box 7.3 Implementing the Physics of
Page 175 and 176: FIGURE 7.2 Multiwavelength images o
Page 177: Recommendations for New Space Activ
Page 181 and 182: significance of mergers in the buil
Page 183 and 184: independent advice committee review
Page 185 and 186: committee review. It could range be
Page 187 and 188: Laboratory Astrophysics As describe
Page 189 and 190: Recommendations for New Ground-Base
Page 191 and 192: Program for instrumentation and fac
Page 193 and 194: excel at high spectral and spatial
Page 195 and 196: The committee reviewed a technical
Page 197 and 198: FIGURE 7.10 ACTA would be, like the
Page 199 and 200: Advanced Technologies and Instrumen
Page 201 and 202: LISA as soon as possible subject to
Page 203: FIGURE 7.14 DOE recommended program
Page 207 and 208: A Summary of Science Frontiers Pane
Page 209 and 210: PLANETARY SYSTEMS AND STAR FORMATIO
Page 211 and 212: A preliminary recommended program w
Page 213 and 214: certified as independent work perfo
Page 215 and 216: penalty based on an assessment of s
Page 217 and 218: The results show excellent correlat
Page 219 and 220: $12 MILLION TO $40 MILLION RANGE CM
Page 221 and 222: decadal research strategy with reco
Page 223 and 224: CFP CHIPSat CIP CGRO CMB CMU CoBRA
Page 225 and 226: NRC NSB NSF NSF-AGS NSF-ARC NSF-AST
show all

prepublication copy - The Department of Astronomy & Astrophysics ...

Create successful ePaper yourself

Delete template?

Save as template?