Astrophysics

25 missions in this study. 63,383 tracked publications and 3,416,710 citations over their lifetimes.

Exploring stars, galaxies and the universe beyond our solar system.


Research over time

Tracked publications Citations

Dashed: 2026 is not yet a full year.

Scope Papers published from the first full month after science operations begin through 2 years after the mission ends. Citations are counted through the third calendar year after each paper appears. Methods Papers published from the first full month after science operations begin through 2 years after the prime mission ends. Citations are counted through the third calendar year after each paper appears. Methods Every tracked publication to date, with every citation to date. Methods

Key measures

Active Mission Window
Missions25
Tracked publicationsTracked publications: peer-reviewed research papers we found for the mission. The list may not be complete. Methods49,849
CitationsCitations received by the tracked publications in the selected scope. The two windowed scopes count each paper’s citations only within its citation window. Methods1,106,317
Mean citations per publicationMean citations: total citations divided by tracked publications in the selected scope. One blockbuster paper can lift it. Methods22
Median citations per publicationMedian citations: the middle paper’s citation count in the selected scope; half the papers have more, half fewer. A single blockbuster sways it less than the mean. Methods13
Uncited publicationsUncited publications: papers with no citations in the selected scope. Methods2,452 (4.9%)
h-indexh-index: the largest h such that h papers have at least h citations each. It only grows with time, so older missions score higher. Methods220
Citations held by the top 10% of papersThe share of all citations in the selected scope that went to the 10% most-cited papers from this division’s missions. The higher it is, the more attention concentrates on a few papers. Methods44%
Percentile citation cutoffs · Active Mission Window
Top 0.1%Cutoff: the fewest citations a paper needs to rank in the top share named, among every paper from this division’s missions in the selected scope, ties included. The count beside it is the papers at or above that line. Not adjusted for publication year. Methods514 · 50 papers at or above
Top 1%Cutoff: the fewest citations a paper needs to rank in the top share named, among every paper from this division’s missions in the selected scope, ties included. The count beside it is the papers at or above that line. Not adjusted for publication year. Methods145 · 506 papers at or above
Top 5%Cutoff: the fewest citations a paper needs to rank in the top share named, among every paper from this division’s missions in the selected scope, ties included. The count beside it is the papers at or above that line. Not adjusted for publication year. Methods68 · 2,543 papers at or above
Top 10%Cutoff: the fewest citations a paper needs to rank in the top share named, among every paper from this division’s missions in the selected scope, ties included. The count beside it is the papers at or above that line. Not adjusted for publication year. Methods46 · 5,119 papers at or above
Top 25%Cutoff: the fewest citations a paper needs to rank in the top share named, among every paper from this division’s missions in the selected scope, ties included. The count beside it is the papers at or above that line. Not adjusted for publication year. Methods25 · 13,075 papers at or above
Top 50%Cutoff: the fewest citations a paper needs to rank in the top share named, among every paper from this division’s missions in the selected scope, ties included. The count beside it is the papers at or above that line. Not adjusted for publication year. Methods13 · 25,337 papers at or above

Highly cited papers per missionTop 10%: among the 10% most-cited papers from this division’s missions, ranked against papers published around the same time. A paper naming several missions is split evenly among the missions in this division that claim it, so counts can be fractional. A failed mission counts as zero and is marked with a slash; a mission whose output could not be measured is left out, not counted as zero. Methods

Top

Papers from each mission that rank in the division’s top 10% for their era.

Time to a first top-10% paperFirst top-10% paper: the earliest-published paper that ranks in its division’s top 10% today, measured from the start of science operations. A paper dated before that start was added by hand and comes from cruise or flyby science. A failed mission counts as zero and is marked with a slash; a mission whose output could not be measured is left out, not counted as zero. Cost: life-cycle cost including partner contributions, in 2025 dollars (NASA’s New Start Index). Methods

20 of 25 missions have a recorded time to a first top-10% paper and a known positive cost in this view.

Each square is a mission: higher costs more; farther left reached its first top-10% paper sooner after science operations began.

Adjusted mission cost · log scale ↑

SWAS $136M · 18.3 months after science start First top-10% paper: August 2000; HETE 2 $158M · 23.8 months after science start First top-10% paper: February 2003; NuSTAR $248M · 10 months after science start First top-10% paper: June 2013; GALEX $282M · 17 months after science start First top-10% paper: January 2005; FUSE $298M · 7 months after science start First top-10% paper: July 2000; WMAP $303M · 17 months after science start First top-10% paper: January 2003; TESS $387M · 0.2 months after science start First top-10% paper: August 2018; Swift $456M · 1.9 months after science start First top-10% paper: June 2005; WISE $484M · 0.8 months after science start First top-10% paper: February 2010; RXTE $490M · 7.1 months after science start First top-10% paper: September 1996; COBE $589M · 5.3 months after science start First top-10% paper: May 1990; EUVE $720M · 18.3 months after science start First top-10% paper: February 1994; IRAS $816M · 12.2 months after science start First top-10% paper: March 1984; Kepler $1.1B · 2.6 months after science start First top-10% paper: August 2009; Fermi $1.3B · 0.9 months after science start First top-10% paper: September 2008; GP-B $1.4B · 1.1 months after science start First top-10% paper: October 2004; SIRTF $1.6B · 0.5 months after science start First top-10% paper: January 2004; CGRO $2.0B · 8.9 months after science start First top-10% paper: January 1992; Chandra $7.5B · 4.7 months after science start First top-10% paper: January 2000; HST $14B · 1.2 months after science start First top-10% paper: June 1990

Running total of all top papers, contributed by missionTop 10%: among the 10% most-cited papers from this division’s missions, ranked against papers published around the same time. Missions sit at their own cost on a log scale. The line is the running total of the division’s top-10% papers, adding missions from cheapest to costliest. The dashed line at $150M is an editorial comparison point, not an inferred scientific threshold. Cost: life-cycle cost including partner contributions, in 2025 dollars (NASA’s New Start Index). Methods

Running total of the division’s top-10% papers, adding missions from cheapest to costliest: 4,985 papers across 25 missions from $5.2M to $14B.

Explore missions

Lifetime totals; Top-10% credit follows the scope above (Active Mission Window).
ImageCost: life-cycle cost including partner contributions, in 2025 dollars (NASA’s New Start Index). MethodsTracked publications: peer-reviewed research papers we found for the mission. The list may not be complete. Methodsh-index: the largest h such that h papers have at least h citations each. It only grows with time, so older missions score higher. MethodsTop 10%: among the 10% most-cited papers from this division’s missions, ranked against papers published around the same time. MethodsTracked publications per yearStrip: tracked publications per year since the start of science operations. Methods
IRAS 1983Pointed Observatory$816M36720,63970 3
COBE 1989Survey Observatory$589M1,413125,285159 54
HST 1990Pointed Observatory$14B18,8621,159,325350 1,697
CGRO 1991Survey Observatory$2.0B2,768149,133169 119
EUVE 1992Survey Observatory$720M47318,34973 18
RXTE 1995Survey Observatory$490M2,582121,071145 97
HETE 1 failed1996Survey Observatory$128M000 0
SWAS 1998Survey Observatory$136M762,97036 1.1
Chandra 1999Pointed Observatory$7.5B9,201455,447240 510
FUSE 1999Pointed Observatory$298M79937,65493 19
WIRE 1999Survey Observatory$149M2498116 0
HETE 2 2000Survey Observatory$158M12610,98345 15
WMAP 2001Survey Observatory$303M3,298339,100236 327
CHIPS 2003Survey Observatory$27M4814 0
GALEX 2003Survey Observatory$282M1,57391,653139 53
SIRTF 2003Pointed Observatory$1.6B6,746448,042255 582
GP-B 2004Pointed Observatory$1.4B1243,72928 2
Swift 2004Pointed Observatory$456M5,490226,035182 297
Fermi 2008Survey Observatory$1.3B6,573287,394207 499
Kepler 2009Survey Observatory$1.1B4,573232,495204 426
WISE 2009Survey Observatory$484M2,581102,751128 13
NuSTAR 2012Pointed Observatory$248M1,91952,16091 68
ASTERIA 2017Pointed Observatory$6.5M3423 0
HaloSat 2018Survey Observatory$5.2M152698 0
TESS 2018Survey Observatory$387M3,53562,15688 184