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| title=First results from the ESO VLTI calibrators program [[Category:Bayer objects|Eridani, Pi]] ...

...astrometric one.<ref name="Abt2006"/> More recently, a continuation of the ESO-CES survey to the [[High Accuracy Radial Velocity Planet Searcher|HARPS]] s <ref name="Endl2002">{{cite journal | title=The planet search program at the ESO Coudé Echelle spectrometer. III. The complete Long Camera survey results | ...

...=Astronomy-2011-06-29>{{cite web |title= Most distant quasar found |author=ESO |date=2011-06-29 |publisher=Astronomy Magazine |url=http://www.astronomy.co ...eater than the estimated age of the light from the most distant observable objects, yet is not in contradiction. See [[Distance measures (cosmology)]] which e ...

...ann17041/|title=ESO's SPHERE Unveils its First Exoplanet|last=|website=www.eso.org|language=en-au|access-date=2017-07-07}}</ref> It is 385 [[light-year]]s ...-mass objects at 100-200 au for [[Red dwarf|M-dwarfs]] and [[Saturn]]-mass objects at 10 au for M-dwarfs. For [[Alpha Centauri|α Cen A]] JWST might be able to ...

| credit = ESO VHS [[Category:Astronomical objects discovered in 2004]] ...

|publisher=[[NEODyS]] (Near Earth Objects{{Snd}} Dynamic Site) |publisher=NEODyS (Near Earth Objects{{Snd}} Dynamic Site) ...

...Observatory]] in Chile.<ref>{{cite web|title=Sibling Stars|url=http://www.eso.org/public/news/eso1534/|access-date=19 August 2015}}</ref> [[Category:IC objects|4651]] ...

A visual search using the [[European Southern Observatory|ESO]]'s [[Very Large Telescope]] found one potential candidate. However, a subs ...(225 to 260 K or 285 K), making Epsilon Indi Ab likely one of the coldest objects to be directly imaged outside the [[Solar System|solar system]]. At this te ...

|credit=ESO [[Category:2MASS objects|J16470892-4549585]] ...

|credit=ESO [[Category:2MASS objects|J16470468-4551238]] ...

...ean Organisation for Astronomical Research in the Southern Hemisphere]] (''ESO'') announced that they had discovered three [[super-Earth]]s in orbit aroun ...discovered with HARPS], press release, [[European Southern Observatory]], ESO 19/08, June 16, 2008. ...

...ate=1998|edition=Second}}</ref> This is also the case with other celestial objects. ...ions for the VLT 8m Unit Telescopes|year=1991|publisher=ESO|url=http://www.eso.org/sci/libraries/historicaldocuments/VLT_Reports/VLTrep63_A1b.pdf}}</ref> ...

...y]], '''minimum mass''' is the lower-bound calculated [[mass]] of observed objects such as [[planet]]s, [[star]]s, [[binary system]]s,<ref name="binary"/> [[n ...|date=1 January 2005 |page=2 |bibcode=2005eso..pres....2. |url=http://www.eso.org/public/news/eso0503/ |access-date=13 August 2006 |postscript=.}}</ref> ...

...a longstanding 'unanswered question' about the dynamics of these brilliant objects."<ref>{{Cite web |title=Scientists Solve Major Mystery of Powerful Energy B ...s|title=|source=Postdoctoral Researcher, Finnish Centre for Astronomy with ESO}} ...

| credit=[[European Southern Observatory|ESO]] [[Category:Astronomical objects discovered in 1961]] ...

|credit=ESO [[Category:2MASS objects|J04551048-6820298]] ...

...comparing WISE images at different [[Epoch (astronomy)|epoch]]s to reveal objects that have high [[proper motion]]s.{{r|PennState|Luhman2013}} ...by stars; the abundance of light sources makes it difficult to spot faint objects. This explains why an object so near to the Sun was not discovered in earli ...

...ormation process). This list does not include free-floating planetary-mass objects in star-forming regions or young associations, which are also referred to a ...t (≥100 AU) formed in [[Circumstellar disc|circumstellar disks]] and these objects are therefore more often referred as planetary-mass companions.<ref>{{Cite ...

...found by taking a series of positional determinations against more distant objects. Once the distance to a star is determined through [[astrometric]] means su * '''Mass distributions''': Through measurement of the kinematics of tracer objects such as globular clusters and the orbits of nearby [[Satellite galaxy|satel ...

| semimajor = {{val|−1.2723|0.0001|fmt=none|u=AU}}{{efn|1=Objects on hyperbolic trajectories have negative semimajor axis, giving them a posi ...ed below 27.5 mag (the limit of [[Hubble Space Telescope]] for fast-moving objects) around 1 January 2018. By late 2019, it should have dimmed to 34 mag.}} ...